[876] | 1 | from asap._asap import Scantable |
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[226] | 2 | from asap import rcParams |
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[1118] | 3 | from asap import print_log |
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| 4 | from asap import asaplog |
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[946] | 5 | from asap import selector |
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[1153] | 6 | from asap import linecatalog |
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[1295] | 7 | from asap import _n_bools, mask_not, mask_and, mask_or |
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[102] | 8 | |
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[876] | 9 | class scantable(Scantable): |
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[102] | 10 | """ |
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| 11 | The ASAP container for scans |
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| 12 | """ |
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[710] | 13 | |
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[1496] | 14 | def __init__(self, filename, average=None, unit=None, getpt=None): |
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[102] | 15 | """ |
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| 16 | Create a scantable from a saved one or make a reference |
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| 17 | Parameters: |
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[181] | 18 | filename: the name of an asap table on disk |
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| 19 | or |
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| 20 | the name of a rpfits/sdfits/ms file |
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| 21 | (integrations within scans are auto averaged |
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| 22 | and the whole file is read) |
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| 23 | or |
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| 24 | [advanced] a reference to an existing |
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[102] | 25 | scantable |
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[484] | 26 | average: average all integrations withinb a scan on read. |
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| 27 | The default (True) is taken from .asaprc. |
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| 28 | unit: brightness unit; must be consistent with K or Jy. |
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[340] | 29 | Over-rides the default selected by the reader |
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| 30 | (input rpfits/sdfits/ms) or replaces the value |
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| 31 | in existing scantables |
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[710] | 32 | """ |
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[976] | 33 | if average is None: |
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[710] | 34 | average = rcParams['scantable.autoaverage'] |
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[1496] | 35 | if getpt is None: |
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| 36 | getpt = False |
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[1259] | 37 | varlist = vars() |
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[876] | 38 | from asap._asap import stmath |
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| 39 | self._math = stmath() |
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| 40 | if isinstance(filename, Scantable): |
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| 41 | Scantable.__init__(self, filename) |
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[181] | 42 | else: |
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[1118] | 43 | if isinstance(filename, str): |
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[976] | 44 | import os.path |
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| 45 | filename = os.path.expandvars(filename) |
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| 46 | filename = os.path.expanduser(filename) |
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| 47 | if not os.path.exists(filename): |
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| 48 | s = "File '%s' not found." % (filename) |
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[718] | 49 | if rcParams['verbose']: |
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[976] | 50 | asaplog.push(s) |
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| 51 | print asaplog.pop().strip() |
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[718] | 52 | return |
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[976] | 53 | raise IOError(s) |
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[1115] | 54 | if os.path.isdir(filename) \ |
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[1118] | 55 | and not os.path.exists(filename+'/table.f1'): |
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[976] | 56 | # crude check if asap table |
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| 57 | if os.path.exists(filename+'/table.info'): |
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[1118] | 58 | ondisk = rcParams['scantable.storage'] == 'disk' |
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| 59 | Scantable.__init__(self, filename, ondisk) |
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[976] | 60 | if unit is not None: |
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| 61 | self.set_fluxunit(unit) |
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[1496] | 62 | # do not reset to the default freqframe |
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| 63 | #self.set_freqframe(rcParams['scantable.freqframe']) |
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[718] | 64 | else: |
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[1118] | 65 | msg = "The given file '%s'is not a valid " \ |
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| 66 | "asap table." % (filename) |
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[976] | 67 | if rcParams['verbose']: |
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| 68 | print msg |
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| 69 | return |
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| 70 | else: |
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| 71 | raise IOError(msg) |
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[226] | 72 | else: |
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[1496] | 73 | self._fill([filename], unit, average, getpt) |
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[1118] | 74 | elif (isinstance(filename, list) or isinstance(filename, tuple)) \ |
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[976] | 75 | and isinstance(filename[-1], str): |
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[1496] | 76 | self._fill(filename, unit, average, getpt) |
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[1259] | 77 | self._add_history("scantable", varlist) |
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[714] | 78 | print_log() |
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[102] | 79 | |
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[876] | 80 | def save(self, name=None, format=None, overwrite=False): |
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[116] | 81 | """ |
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[1280] | 82 | Store the scantable on disk. This can be an asap (aips++) Table, |
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| 83 | SDFITS or MS2 format. |
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[116] | 84 | Parameters: |
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[1093] | 85 | name: the name of the outputfile. For format "ASCII" |
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| 86 | this is the root file name (data in 'name'.txt |
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[497] | 87 | and header in 'name'_header.txt) |
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[116] | 88 | format: an optional file format. Default is ASAP. |
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[280] | 89 | Allowed are - 'ASAP' (save as ASAP [aips++] Table), |
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[194] | 90 | 'SDFITS' (save as SDFITS file) |
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[200] | 91 | 'ASCII' (saves as ascii text file) |
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[226] | 92 | 'MS2' (saves as an aips++ |
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| 93 | MeasurementSet V2) |
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[411] | 94 | overwrite: If the file should be overwritten if it exists. |
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[256] | 95 | The default False is to return with warning |
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[411] | 96 | without writing the output. USE WITH CARE. |
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[116] | 97 | Example: |
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| 98 | scan.save('myscan.asap') |
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[1118] | 99 | scan.save('myscan.sdfits', 'SDFITS') |
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[116] | 100 | """ |
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[411] | 101 | from os import path |
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[226] | 102 | if format is None: format = rcParams['scantable.save'] |
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[256] | 103 | suffix = '.'+format.lower() |
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[1118] | 104 | if name is None or name == "": |
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[256] | 105 | name = 'scantable'+suffix |
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[718] | 106 | msg = "No filename given. Using default name %s..." % name |
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| 107 | asaplog.push(msg) |
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[411] | 108 | name = path.expandvars(name) |
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[256] | 109 | if path.isfile(name) or path.isdir(name): |
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| 110 | if not overwrite: |
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[718] | 111 | msg = "File %s exists." % name |
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| 112 | if rcParams['verbose']: |
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| 113 | print msg |
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| 114 | return |
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| 115 | else: |
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| 116 | raise IOError(msg) |
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[451] | 117 | format2 = format.upper() |
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| 118 | if format2 == 'ASAP': |
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[116] | 119 | self._save(name) |
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| 120 | else: |
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[989] | 121 | from asap._asap import stwriter as stw |
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[1118] | 122 | writer = stw(format2) |
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| 123 | writer.write(self, name) |
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[718] | 124 | print_log() |
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[116] | 125 | return |
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| 126 | |
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[102] | 127 | def copy(self): |
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| 128 | """ |
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| 129 | Return a copy of this scantable. |
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[1348] | 130 | Note: |
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| 131 | This makes a full (deep) copy. scan2 = scan1 makes a reference. |
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[102] | 132 | Parameters: |
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[113] | 133 | none |
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[102] | 134 | Example: |
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| 135 | copiedscan = scan.copy() |
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| 136 | """ |
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[876] | 137 | sd = scantable(Scantable._copy(self)) |
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[113] | 138 | return sd |
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| 139 | |
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[1093] | 140 | def drop_scan(self, scanid=None): |
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| 141 | """ |
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| 142 | Return a new scantable where the specified scan number(s) has(have) |
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| 143 | been dropped. |
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| 144 | Parameters: |
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| 145 | scanid: a (list of) scan number(s) |
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| 146 | """ |
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| 147 | from asap import _is_sequence_or_number as _is_valid |
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| 148 | from asap import _to_list |
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| 149 | from asap import unique |
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| 150 | if not _is_valid(scanid): |
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| 151 | if rcParams['verbose']: |
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| 152 | print "Please specify a scanno to drop from the scantable" |
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| 153 | return |
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| 154 | else: |
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| 155 | raise RuntimeError("No scan given") |
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| 156 | try: |
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| 157 | scanid = _to_list(scanid) |
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| 158 | allscans = unique([ self.getscan(i) for i in range(self.nrow())]) |
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| 159 | for sid in scanid: allscans.remove(sid) |
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[1118] | 160 | if len(allscans) == 0: |
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| 161 | raise ValueError("Can't remove all scans") |
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[1093] | 162 | except ValueError: |
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| 163 | if rcParams['verbose']: |
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| 164 | print "Couldn't find any match." |
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| 165 | return |
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| 166 | else: raise |
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| 167 | try: |
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| 168 | bsel = self.get_selection() |
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| 169 | sel = selector() |
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| 170 | sel.set_scans(allscans) |
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| 171 | self.set_selection(bsel+sel) |
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| 172 | scopy = self._copy() |
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| 173 | self.set_selection(bsel) |
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| 174 | return scantable(scopy) |
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| 175 | except RuntimeError: |
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[1118] | 176 | if rcParams['verbose']: |
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| 177 | print "Couldn't find any match." |
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| 178 | else: |
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| 179 | raise |
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[1093] | 180 | |
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| 181 | |
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[102] | 182 | def get_scan(self, scanid=None): |
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| 183 | """ |
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| 184 | Return a specific scan (by scanno) or collection of scans (by |
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| 185 | source name) in a new scantable. |
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[1348] | 186 | Note: |
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| 187 | See scantable.drop_scan() for the inverse operation. |
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[102] | 188 | Parameters: |
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[513] | 189 | scanid: a (list of) scanno or a source name, unix-style |
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| 190 | patterns are accepted for source name matching, e.g. |
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| 191 | '*_R' gets all 'ref scans |
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[102] | 192 | Example: |
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[513] | 193 | # get all scans containing the source '323p459' |
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| 194 | newscan = scan.get_scan('323p459') |
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| 195 | # get all 'off' scans |
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| 196 | refscans = scan.get_scan('*_R') |
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| 197 | # get a susbset of scans by scanno (as listed in scan.summary()) |
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[1118] | 198 | newscan = scan.get_scan([0, 2, 7, 10]) |
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[102] | 199 | """ |
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| 200 | if scanid is None: |
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[718] | 201 | if rcParams['verbose']: |
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[1118] | 202 | print "Please specify a scan no or name to " \ |
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| 203 | "retrieve from the scantable" |
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[718] | 204 | return |
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| 205 | else: |
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| 206 | raise RuntimeError("No scan given") |
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| 207 | |
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[102] | 208 | try: |
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[946] | 209 | bsel = self.get_selection() |
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| 210 | sel = selector() |
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[102] | 211 | if type(scanid) is str: |
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[946] | 212 | sel.set_name(scanid) |
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| 213 | self.set_selection(bsel+sel) |
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[876] | 214 | scopy = self._copy() |
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[946] | 215 | self.set_selection(bsel) |
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[876] | 216 | return scantable(scopy) |
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[102] | 217 | elif type(scanid) is int: |
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[946] | 218 | sel.set_scans([scanid]) |
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| 219 | self.set_selection(bsel+sel) |
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[876] | 220 | scopy = self._copy() |
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[946] | 221 | self.set_selection(bsel) |
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[876] | 222 | return scantable(scopy) |
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[381] | 223 | elif type(scanid) is list: |
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[946] | 224 | sel.set_scans(scanid) |
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| 225 | self.set_selection(sel) |
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[876] | 226 | scopy = self._copy() |
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[946] | 227 | self.set_selection(bsel) |
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[876] | 228 | return scantable(scopy) |
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[381] | 229 | else: |
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[718] | 230 | msg = "Illegal scanid type, use 'int' or 'list' if ints." |
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| 231 | if rcParams['verbose']: |
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| 232 | print msg |
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| 233 | else: |
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| 234 | raise TypeError(msg) |
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[102] | 235 | except RuntimeError: |
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[718] | 236 | if rcParams['verbose']: print "Couldn't find any match." |
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| 237 | else: raise |
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[102] | 238 | |
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| 239 | def __str__(self): |
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[1118] | 240 | return Scantable._summary(self, True) |
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[102] | 241 | |
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[976] | 242 | def summary(self, filename=None): |
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[102] | 243 | """ |
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| 244 | Print a summary of the contents of this scantable. |
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| 245 | Parameters: |
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| 246 | filename: the name of a file to write the putput to |
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| 247 | Default - no file output |
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[381] | 248 | verbose: print extra info such as the frequency table |
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| 249 | The default (False) is taken from .asaprc |
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[102] | 250 | """ |
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[976] | 251 | info = Scantable._summary(self, True) |
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| 252 | #if verbose is None: verbose = rcParams['scantable.verbosesummary'] |
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[102] | 253 | if filename is not None: |
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[256] | 254 | if filename is "": |
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| 255 | filename = 'scantable_summary.txt' |
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[415] | 256 | from os.path import expandvars, isdir |
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[411] | 257 | filename = expandvars(filename) |
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[415] | 258 | if not isdir(filename): |
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[413] | 259 | data = open(filename, 'w') |
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| 260 | data.write(info) |
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| 261 | data.close() |
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| 262 | else: |
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[718] | 263 | msg = "Illegal file name '%s'." % (filename) |
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| 264 | if rcParams['verbose']: |
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| 265 | print msg |
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| 266 | else: |
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| 267 | raise IOError(msg) |
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| 268 | if rcParams['verbose']: |
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[794] | 269 | try: |
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| 270 | from IPython.genutils import page as pager |
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| 271 | except ImportError: |
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| 272 | from pydoc import pager |
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| 273 | pager(info) |
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[718] | 274 | else: |
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| 275 | return info |
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[710] | 276 | |
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[946] | 277 | |
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| 278 | def get_selection(self): |
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| 279 | """ |
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[1005] | 280 | Get the selection object currently set on this scantable. |
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| 281 | Parameters: |
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| 282 | none |
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| 283 | Example: |
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| 284 | sel = scan.get_selection() |
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| 285 | sel.set_ifs(0) # select IF 0 |
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| 286 | scan.set_selection(sel) # apply modified selection |
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[946] | 287 | """ |
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| 288 | return selector(self._getselection()) |
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| 289 | |
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[1005] | 290 | def set_selection(self, selection=selector()): |
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[946] | 291 | """ |
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[1005] | 292 | Select a subset of the data. All following operations on this scantable |
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| 293 | are only applied to thi selection. |
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| 294 | Parameters: |
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| 295 | selection: a selector object (default unset the selection) |
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| 296 | Examples: |
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| 297 | sel = selector() # create a selection object |
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[1118] | 298 | self.set_scans([0, 3]) # select SCANNO 0 and 3 |
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[1005] | 299 | scan.set_selection(sel) # set the selection |
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| 300 | scan.summary() # will only print summary of scanno 0 an 3 |
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| 301 | scan.set_selection() # unset the selection |
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[946] | 302 | """ |
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| 303 | self._setselection(selection) |
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| 304 | |
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[1446] | 305 | def get_row(self, row=0, insitu=None): |
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| 306 | """ |
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| 307 | Select a row in the scantable. |
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| 308 | Return a scantable with single row. |
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| 309 | Parameters: |
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| 310 | row: row no of integration, default is 0. |
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| 311 | insitu: if False a new scantable is returned. |
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| 312 | Otherwise, the scaling is done in-situ |
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| 313 | The default is taken from .asaprc (False) |
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| 314 | """ |
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| 315 | if insitu is None: insitu = rcParams['insitu'] |
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| 316 | if not insitu: |
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| 317 | workscan = self.copy() |
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| 318 | else: |
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| 319 | workscan = self |
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| 320 | # Select a row |
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| 321 | sel=selector() |
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| 322 | sel.set_scans([workscan.getscan(row)]) |
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| 323 | sel.set_cycles([workscan.getcycle(row)]) |
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| 324 | sel.set_beams([workscan.getbeam(row)]) |
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| 325 | sel.set_ifs([workscan.getif(row)]) |
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| 326 | sel.set_polarisations([workscan.getpol(row)]) |
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| 327 | sel.set_name(workscan._getsourcename(row)) |
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| 328 | workscan.set_selection(sel) |
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| 329 | if not workscan.nrow() == 1: |
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| 330 | msg = "Cloud not identify single row. %d rows selected."%(workscan.nrow()) |
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| 331 | raise RuntimeError(msg) |
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| 332 | del sel |
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| 333 | if insitu: |
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| 334 | self._assign(workscan) |
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| 335 | else: |
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| 336 | return workscan |
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| 337 | |
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[876] | 338 | def stats(self, stat='stddev', mask=None): |
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[102] | 339 | """ |
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[135] | 340 | Determine the specified statistic of the current beam/if/pol |
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[102] | 341 | Takes a 'mask' as an optional parameter to specify which |
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| 342 | channels should be excluded. |
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[1515] | 343 | You can get min/max values with their position |
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| 344 | (channels/frequencies/velocities) by selecting stat='minpos' |
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| 345 | or 'maxpos'. |
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[102] | 346 | Parameters: |
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[1515] | 347 | stat: 'min', 'max', 'minpos', 'maxpos', 'sumsq', 'sum', |
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| 348 | 'mean', 'var', 'stddev', 'avdev', 'rms', 'median' |
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[135] | 349 | mask: an optional mask specifying where the statistic |
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[102] | 350 | should be determined. |
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| 351 | Example: |
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[113] | 352 | scan.set_unit('channel') |
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[1118] | 353 | msk = scan.create_mask([100, 200], [500, 600]) |
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[135] | 354 | scan.stats(stat='mean', mask=m) |
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[102] | 355 | """ |
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| 356 | if mask == None: |
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[876] | 357 | mask = [] |
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[1118] | 358 | axes = ['Beam', 'IF', 'Pol', 'Time'] |
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[876] | 359 | if not self._check_ifs(): |
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[1118] | 360 | raise ValueError("Cannot apply mask as the IFs have different " |
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| 361 | "number of channels. Please use setselection() " |
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| 362 | "to select individual IFs") |
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[256] | 363 | |
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[1515] | 364 | if stat.lower().find('pos') == -1: |
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| 365 | statvals = self._math._stats(self, mask, stat) |
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| 366 | position = False |
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| 367 | sstat = str(stat) |
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| 368 | else: |
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| 369 | pos = self._math._minmaxpos(self, mask, stat) |
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| 370 | position = True |
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| 371 | statvals = [] |
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| 372 | sstat = stat.lower().strip('pos') |
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[876] | 373 | out = '' |
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| 374 | axes = [] |
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| 375 | for i in range(self.nrow()): |
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| 376 | axis = [] |
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| 377 | axis.append(self.getscan(i)) |
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| 378 | axis.append(self.getbeam(i)) |
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| 379 | axis.append(self.getif(i)) |
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| 380 | axis.append(self.getpol(i)) |
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| 381 | axis.append(self.getcycle(i)) |
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| 382 | axes.append(axis) |
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| 383 | tm = self._gettime(i) |
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| 384 | src = self._getsourcename(i) |
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[1515] | 385 | xpos = '' |
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| 386 | if position: |
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| 387 | qx, y = self.pos2data(rowno=i, pos=pos[i]) |
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| 388 | statvals.append(y) |
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| 389 | xpos = '(x = %3.3f' % (qx['value'])+' ['+qx['unit']+'])' |
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[876] | 390 | out += 'Scan[%d] (%s) ' % (axis[0], src) |
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| 391 | out += 'Time[%s]:\n' % (tm) |
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| 392 | if self.nbeam(-1) > 1: out += ' Beam[%d] ' % (axis[1]) |
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| 393 | if self.nif(-1) > 1: out += ' IF[%d] ' % (axis[2]) |
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| 394 | if self.npol(-1) > 1: out += ' Pol[%d] ' % (axis[3]) |
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[1515] | 395 | out += '= %3.3f ' % (statvals[i]) +xpos+'\n' |
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[876] | 396 | out += "--------------------------------------------------\n" |
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[256] | 397 | |
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[876] | 398 | if rcParams['verbose']: |
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| 399 | print "--------------------------------------------------" |
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[1515] | 400 | print " ", sstat |
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[876] | 401 | print "--------------------------------------------------" |
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| 402 | print out |
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[1295] | 403 | #else: |
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| 404 | #retval = { 'axesnames': ['scanno', 'beamno', 'ifno', 'polno', 'cycleno'], |
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| 405 | # 'axes' : axes, |
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| 406 | # 'data': statvals} |
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| 407 | return statvals |
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[102] | 408 | |
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[1515] | 409 | def pos2data(self, rowno=0, pos=0): |
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| 410 | """ |
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| 411 | Returns the abcissa and ordinate value of a spectrum |
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| 412 | at an arbitrary row and channel in the scantable. |
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| 413 | Parameters: |
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| 414 | rowno: a row number in the scantable. Default is the |
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| 415 | first row, i.e. rowno=0 |
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| 416 | pos: a channel in the scantable. Default is the first |
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| 417 | channel, i.e. pos=0 |
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| 418 | """ |
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| 419 | if isinstance(rowno, int) and isinstance(pos, int): |
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| 420 | x, xlbl = self.get_abcissa(rowno) |
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| 421 | qx = {'unit': xlbl, 'value': x[pos]} |
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| 422 | return qx, self._getspectrum(rowno)[pos] |
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| 423 | |
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[1118] | 424 | def stddev(self, mask=None): |
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[135] | 425 | """ |
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| 426 | Determine the standard deviation of the current beam/if/pol |
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| 427 | Takes a 'mask' as an optional parameter to specify which |
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| 428 | channels should be excluded. |
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| 429 | Parameters: |
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| 430 | mask: an optional mask specifying where the standard |
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| 431 | deviation should be determined. |
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| 432 | |
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| 433 | Example: |
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| 434 | scan.set_unit('channel') |
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[1118] | 435 | msk = scan.create_mask([100, 200], [500, 600]) |
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[135] | 436 | scan.stddev(mask=m) |
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| 437 | """ |
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[1118] | 438 | return self.stats(stat='stddev', mask=mask); |
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[135] | 439 | |
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[1003] | 440 | |
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[1259] | 441 | def get_column_names(self): |
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[1003] | 442 | """ |
---|
| 443 | Return a list of column names, which can be used for selection. |
---|
| 444 | """ |
---|
[1259] | 445 | return list(Scantable.get_column_names(self)) |
---|
[1003] | 446 | |
---|
[876] | 447 | def get_tsys(self): |
---|
[113] | 448 | """ |
---|
| 449 | Return the System temperatures. |
---|
| 450 | Returns: |
---|
[876] | 451 | a list of Tsys values for the current selection |
---|
[113] | 452 | """ |
---|
[256] | 453 | |
---|
[876] | 454 | return self._row_callback(self._gettsys, "Tsys") |
---|
[256] | 455 | |
---|
[876] | 456 | def _row_callback(self, callback, label): |
---|
| 457 | axes = [] |
---|
[1118] | 458 | axesnames = ['scanno', 'beamno', 'ifno', 'polno', 'cycleno'] |
---|
[876] | 459 | out = "" |
---|
[1118] | 460 | outvec = [] |
---|
[876] | 461 | for i in range(self.nrow()): |
---|
| 462 | axis = [] |
---|
| 463 | axis.append(self.getscan(i)) |
---|
| 464 | axis.append(self.getbeam(i)) |
---|
| 465 | axis.append(self.getif(i)) |
---|
| 466 | axis.append(self.getpol(i)) |
---|
| 467 | axis.append(self.getcycle(i)) |
---|
| 468 | axes.append(axis) |
---|
| 469 | tm = self._gettime(i) |
---|
| 470 | src = self._getsourcename(i) |
---|
| 471 | out += 'Scan[%d] (%s) ' % (axis[0], src) |
---|
| 472 | out += 'Time[%s]:\n' % (tm) |
---|
| 473 | if self.nbeam(-1) > 1: out += ' Beam[%d] ' % (axis[1]) |
---|
| 474 | if self.nif(-1) > 1: out += ' IF[%d] ' % (axis[2]) |
---|
| 475 | if self.npol(-1) > 1: out += ' Pol[%d] ' % (axis[3]) |
---|
| 476 | outvec.append(callback(i)) |
---|
| 477 | out += '= %3.3f\n' % (outvec[i]) |
---|
| 478 | out += "--------------------------------------------------\n" |
---|
| 479 | if rcParams['verbose']: |
---|
| 480 | print "--------------------------------------------------" |
---|
| 481 | print " %s" % (label) |
---|
| 482 | print "--------------------------------------------------" |
---|
| 483 | print out |
---|
[1175] | 484 | # disabled because the vector seems more useful |
---|
| 485 | #retval = {'axesnames': axesnames, 'axes': axes, 'data': outvec} |
---|
| 486 | return outvec |
---|
[256] | 487 | |
---|
[1070] | 488 | def _get_column(self, callback, row=-1): |
---|
| 489 | """ |
---|
| 490 | """ |
---|
| 491 | if row == -1: |
---|
| 492 | return [callback(i) for i in range(self.nrow())] |
---|
| 493 | else: |
---|
| 494 | if 0 <= row < self.nrow(): |
---|
| 495 | return callback(row) |
---|
[256] | 496 | |
---|
[1070] | 497 | |
---|
[1348] | 498 | def get_time(self, row=-1, asdatetime=False): |
---|
[113] | 499 | """ |
---|
| 500 | Get a list of time stamps for the observations. |
---|
[1348] | 501 | Return a datetime object for each integration time stamp in the scantable. |
---|
[113] | 502 | Parameters: |
---|
[1348] | 503 | row: row no of integration. Default -1 return all rows |
---|
| 504 | asdatetime: return values as datetime objects rather than strings |
---|
[113] | 505 | Example: |
---|
| 506 | none |
---|
| 507 | """ |
---|
[1175] | 508 | from time import strptime |
---|
| 509 | from datetime import datetime |
---|
[1457] | 510 | times = self._get_column(self._gettime, row) |
---|
[1348] | 511 | if not asdatetime: |
---|
[1457] | 512 | return times |
---|
[1175] | 513 | format = "%Y/%m/%d/%H:%M:%S" |
---|
| 514 | if isinstance(times, list): |
---|
| 515 | return [datetime(*strptime(i, format)[:6]) for i in times] |
---|
| 516 | else: |
---|
| 517 | return datetime(*strptime(times, format)[:6]) |
---|
[102] | 518 | |
---|
[1348] | 519 | |
---|
| 520 | def get_inttime(self, row=-1): |
---|
| 521 | """ |
---|
| 522 | Get a list of integration times for the observations. |
---|
| 523 | Return a time in seconds for each integration in the scantable. |
---|
| 524 | Parameters: |
---|
| 525 | row: row no of integration. Default -1 return all rows. |
---|
| 526 | Example: |
---|
| 527 | none |
---|
| 528 | """ |
---|
| 529 | return self._get_column(self._getinttime, row) |
---|
| 530 | |
---|
| 531 | |
---|
[714] | 532 | def get_sourcename(self, row=-1): |
---|
| 533 | """ |
---|
[794] | 534 | Get a list source names for the observations. |
---|
[714] | 535 | Return a string for each integration in the scantable. |
---|
| 536 | Parameters: |
---|
[1348] | 537 | row: row no of integration. Default -1 return all rows. |
---|
[714] | 538 | Example: |
---|
| 539 | none |
---|
| 540 | """ |
---|
[1070] | 541 | return self._get_column(self._getsourcename, row) |
---|
[714] | 542 | |
---|
[794] | 543 | def get_elevation(self, row=-1): |
---|
| 544 | """ |
---|
| 545 | Get a list of elevations for the observations. |
---|
| 546 | Return a float for each integration in the scantable. |
---|
| 547 | Parameters: |
---|
[1348] | 548 | row: row no of integration. Default -1 return all rows. |
---|
[794] | 549 | Example: |
---|
| 550 | none |
---|
| 551 | """ |
---|
[1070] | 552 | return self._get_column(self._getelevation, row) |
---|
[794] | 553 | |
---|
| 554 | def get_azimuth(self, row=-1): |
---|
| 555 | """ |
---|
| 556 | Get a list of azimuths for the observations. |
---|
| 557 | Return a float for each integration in the scantable. |
---|
| 558 | Parameters: |
---|
[1348] | 559 | row: row no of integration. Default -1 return all rows. |
---|
[794] | 560 | Example: |
---|
| 561 | none |
---|
| 562 | """ |
---|
[1070] | 563 | return self._get_column(self._getazimuth, row) |
---|
[794] | 564 | |
---|
| 565 | def get_parangle(self, row=-1): |
---|
| 566 | """ |
---|
| 567 | Get a list of parallactic angles for the observations. |
---|
| 568 | Return a float for each integration in the scantable. |
---|
| 569 | Parameters: |
---|
[1348] | 570 | row: row no of integration. Default -1 return all rows. |
---|
[794] | 571 | Example: |
---|
| 572 | none |
---|
| 573 | """ |
---|
[1070] | 574 | return self._get_column(self._getparangle, row) |
---|
[794] | 575 | |
---|
[1070] | 576 | def get_direction(self, row=-1): |
---|
| 577 | """ |
---|
| 578 | Get a list of Positions on the sky (direction) for the observations. |
---|
| 579 | Return a float for each integration in the scantable. |
---|
| 580 | Parameters: |
---|
| 581 | row: row no of integration. Default -1 return all rows |
---|
| 582 | Example: |
---|
| 583 | none |
---|
| 584 | """ |
---|
| 585 | return self._get_column(self._getdirection, row) |
---|
| 586 | |
---|
[1389] | 587 | def get_directionval(self, row=-1): |
---|
| 588 | """ |
---|
| 589 | Get a list of Positions on the sky (direction) for the observations. |
---|
| 590 | Return a float for each integration in the scantable. |
---|
| 591 | Parameters: |
---|
| 592 | row: row no of integration. Default -1 return all rows |
---|
| 593 | Example: |
---|
| 594 | none |
---|
| 595 | """ |
---|
| 596 | return self._get_column(self._getdirectionvec, row) |
---|
| 597 | |
---|
[102] | 598 | def set_unit(self, unit='channel'): |
---|
| 599 | """ |
---|
| 600 | Set the unit for all following operations on this scantable |
---|
| 601 | Parameters: |
---|
| 602 | unit: optional unit, default is 'channel' |
---|
[1118] | 603 | one of '*Hz', 'km/s', 'channel', '' |
---|
[102] | 604 | """ |
---|
[484] | 605 | varlist = vars() |
---|
[1118] | 606 | if unit in ['', 'pixel', 'channel']: |
---|
[113] | 607 | unit = '' |
---|
| 608 | inf = list(self._getcoordinfo()) |
---|
| 609 | inf[0] = unit |
---|
| 610 | self._setcoordinfo(inf) |
---|
[1118] | 611 | self._add_history("set_unit", varlist) |
---|
[113] | 612 | |
---|
[484] | 613 | def set_instrument(self, instr): |
---|
[358] | 614 | """ |
---|
[1348] | 615 | Set the instrument for subsequent processing. |
---|
[358] | 616 | Parameters: |
---|
[710] | 617 | instr: Select from 'ATPKSMB', 'ATPKSHOH', 'ATMOPRA', |
---|
[407] | 618 | 'DSS-43' (Tid), 'CEDUNA', and 'HOBART' |
---|
[358] | 619 | """ |
---|
| 620 | self._setInstrument(instr) |
---|
[1118] | 621 | self._add_history("set_instument", vars()) |
---|
[718] | 622 | print_log() |
---|
[358] | 623 | |
---|
[1190] | 624 | def set_feedtype(self, feedtype): |
---|
| 625 | """ |
---|
| 626 | Overwrite the feed type, which might not be set correctly. |
---|
| 627 | Parameters: |
---|
| 628 | feedtype: 'linear' or 'circular' |
---|
| 629 | """ |
---|
| 630 | self._setfeedtype(feedtype) |
---|
| 631 | self._add_history("set_feedtype", vars()) |
---|
| 632 | print_log() |
---|
| 633 | |
---|
[276] | 634 | def set_doppler(self, doppler='RADIO'): |
---|
| 635 | """ |
---|
| 636 | Set the doppler for all following operations on this scantable. |
---|
| 637 | Parameters: |
---|
| 638 | doppler: One of 'RADIO', 'OPTICAL', 'Z', 'BETA', 'GAMMA' |
---|
| 639 | """ |
---|
[484] | 640 | varlist = vars() |
---|
[276] | 641 | inf = list(self._getcoordinfo()) |
---|
| 642 | inf[2] = doppler |
---|
| 643 | self._setcoordinfo(inf) |
---|
[1118] | 644 | self._add_history("set_doppler", vars()) |
---|
[718] | 645 | print_log() |
---|
[710] | 646 | |
---|
[226] | 647 | def set_freqframe(self, frame=None): |
---|
[113] | 648 | """ |
---|
| 649 | Set the frame type of the Spectral Axis. |
---|
| 650 | Parameters: |
---|
[591] | 651 | frame: an optional frame type, default 'LSRK'. Valid frames are: |
---|
[1118] | 652 | 'REST', 'TOPO', 'LSRD', 'LSRK', 'BARY', |
---|
| 653 | 'GEO', 'GALACTO', 'LGROUP', 'CMB' |
---|
[113] | 654 | Examples: |
---|
| 655 | scan.set_freqframe('BARY') |
---|
| 656 | """ |
---|
[484] | 657 | if frame is None: frame = rcParams['scantable.freqframe'] |
---|
| 658 | varlist = vars() |
---|
[1118] | 659 | valid = ['REST', 'TOPO', 'LSRD', 'LSRK', 'BARY', \ |
---|
| 660 | 'GEO', 'GALACTO', 'LGROUP', 'CMB'] |
---|
[591] | 661 | |
---|
[989] | 662 | if frame in valid: |
---|
[113] | 663 | inf = list(self._getcoordinfo()) |
---|
| 664 | inf[1] = frame |
---|
| 665 | self._setcoordinfo(inf) |
---|
[1118] | 666 | self._add_history("set_freqframe", varlist) |
---|
[102] | 667 | else: |
---|
[1118] | 668 | msg = "Please specify a valid freq type. Valid types are:\n", valid |
---|
[718] | 669 | if rcParams['verbose']: |
---|
| 670 | print msg |
---|
| 671 | else: |
---|
| 672 | raise TypeError(msg) |
---|
| 673 | print_log() |
---|
[710] | 674 | |
---|
[989] | 675 | def set_dirframe(self, frame=""): |
---|
| 676 | """ |
---|
| 677 | Set the frame type of the Direction on the sky. |
---|
| 678 | Parameters: |
---|
| 679 | frame: an optional frame type, default ''. Valid frames are: |
---|
| 680 | 'J2000', 'B1950', 'GALACTIC' |
---|
| 681 | Examples: |
---|
| 682 | scan.set_dirframe('GALACTIC') |
---|
| 683 | """ |
---|
| 684 | varlist = vars() |
---|
| 685 | try: |
---|
| 686 | Scantable.set_dirframe(self, frame) |
---|
[1118] | 687 | except RuntimeError, msg: |
---|
[989] | 688 | if rcParams['verbose']: |
---|
| 689 | print msg |
---|
| 690 | else: |
---|
| 691 | raise |
---|
[1118] | 692 | self._add_history("set_dirframe", varlist) |
---|
[989] | 693 | |
---|
[113] | 694 | def get_unit(self): |
---|
| 695 | """ |
---|
| 696 | Get the default unit set in this scantable |
---|
| 697 | Returns: |
---|
| 698 | A unit string |
---|
| 699 | """ |
---|
| 700 | inf = self._getcoordinfo() |
---|
| 701 | unit = inf[0] |
---|
| 702 | if unit == '': unit = 'channel' |
---|
| 703 | return unit |
---|
[102] | 704 | |
---|
[158] | 705 | def get_abcissa(self, rowno=0): |
---|
[102] | 706 | """ |
---|
[158] | 707 | Get the abcissa in the current coordinate setup for the currently |
---|
[113] | 708 | selected Beam/IF/Pol |
---|
| 709 | Parameters: |
---|
[226] | 710 | rowno: an optional row number in the scantable. Default is the |
---|
| 711 | first row, i.e. rowno=0 |
---|
[113] | 712 | Returns: |
---|
[1348] | 713 | The abcissa values and the format string (as a dictionary) |
---|
[113] | 714 | """ |
---|
[256] | 715 | abc = self._getabcissa(rowno) |
---|
[710] | 716 | lbl = self._getabcissalabel(rowno) |
---|
[718] | 717 | print_log() |
---|
[158] | 718 | return abc, lbl |
---|
[113] | 719 | |
---|
[1401] | 720 | def flag(self, mask=None, unflag=False): |
---|
[1001] | 721 | """ |
---|
| 722 | Flag the selected data using an optional channel mask. |
---|
| 723 | Parameters: |
---|
| 724 | mask: an optional channel mask, created with create_mask. Default |
---|
| 725 | (no mask) is all channels. |
---|
[1401] | 726 | unflag: if True, unflag the data |
---|
[1001] | 727 | """ |
---|
| 728 | varlist = vars() |
---|
[1118] | 729 | if mask is None: |
---|
| 730 | mask = [] |
---|
[1001] | 731 | try: |
---|
[1401] | 732 | self._flag(mask, unflag) |
---|
[1118] | 733 | except RuntimeError, msg: |
---|
[1001] | 734 | if rcParams['verbose']: |
---|
| 735 | print msg |
---|
| 736 | return |
---|
| 737 | else: raise |
---|
| 738 | self._add_history("flag", varlist) |
---|
| 739 | |
---|
[1203] | 740 | def lag_flag(self, frequency, width=0.0, unit="GHz", insitu=None): |
---|
[1192] | 741 | """ |
---|
| 742 | Flag the data in 'lag' space by providing a frequency to remove. |
---|
| 743 | Flagged data in the scantable gets set to 0.0 before the fft. |
---|
| 744 | No taper is applied. |
---|
| 745 | Parameters: |
---|
[1348] | 746 | frequency: the frequency (really a period within the bandwidth) |
---|
| 747 | to remove |
---|
| 748 | width: the width of the frequency to remove, to remove a |
---|
| 749 | range of frequencies aroung the centre. |
---|
[1203] | 750 | unit: the frequency unit (default "GHz") |
---|
| 751 | Notes: |
---|
[1348] | 752 | It is recommended to flag edges of the band or strong |
---|
| 753 | signals beforehand. |
---|
[1192] | 754 | """ |
---|
| 755 | if insitu is None: insitu = rcParams['insitu'] |
---|
| 756 | self._math._setinsitu(insitu) |
---|
| 757 | varlist = vars() |
---|
[1370] | 758 | base = { "GHz": 1000000000., "MHz": 1000000., "kHz": 1000., "Hz": 1. } |
---|
[1192] | 759 | if not base.has_key(unit): |
---|
| 760 | raise ValueError("%s is not a valid unit." % unit) |
---|
| 761 | try: |
---|
[1200] | 762 | s = scantable(self._math._lag_flag(self, frequency*base[unit], |
---|
| 763 | width*base[unit])) |
---|
[1192] | 764 | except RuntimeError, msg: |
---|
| 765 | if rcParams['verbose']: |
---|
| 766 | print msg |
---|
| 767 | return |
---|
| 768 | else: raise |
---|
| 769 | s._add_history("lag_flag", varlist) |
---|
| 770 | print_log() |
---|
| 771 | if insitu: |
---|
| 772 | self._assign(s) |
---|
| 773 | else: |
---|
| 774 | return s |
---|
[1001] | 775 | |
---|
[1192] | 776 | |
---|
[113] | 777 | def create_mask(self, *args, **kwargs): |
---|
| 778 | """ |
---|
[1118] | 779 | Compute and return a mask based on [min, max] windows. |
---|
[189] | 780 | The specified windows are to be INCLUDED, when the mask is |
---|
[113] | 781 | applied. |
---|
[102] | 782 | Parameters: |
---|
[1118] | 783 | [min, max], [min2, max2], ... |
---|
[1024] | 784 | Pairs of start/end points (inclusive)specifying the regions |
---|
[102] | 785 | to be masked |
---|
[189] | 786 | invert: optional argument. If specified as True, |
---|
| 787 | return an inverted mask, i.e. the regions |
---|
| 788 | specified are EXCLUDED |
---|
[513] | 789 | row: create the mask using the specified row for |
---|
| 790 | unit conversions, default is row=0 |
---|
| 791 | only necessary if frequency varies over rows. |
---|
[102] | 792 | Example: |
---|
[113] | 793 | scan.set_unit('channel') |
---|
| 794 | a) |
---|
[1118] | 795 | msk = scan.create_mask([400, 500], [800, 900]) |
---|
[189] | 796 | # masks everything outside 400 and 500 |
---|
[113] | 797 | # and 800 and 900 in the unit 'channel' |
---|
| 798 | |
---|
| 799 | b) |
---|
[1118] | 800 | msk = scan.create_mask([400, 500], [800, 900], invert=True) |
---|
[189] | 801 | # masks the regions between 400 and 500 |
---|
[113] | 802 | # and 800 and 900 in the unit 'channel' |
---|
[1024] | 803 | c) |
---|
| 804 | mask only channel 400 |
---|
[1118] | 805 | msk = scan.create_mask([400, 400]) |
---|
[102] | 806 | """ |
---|
[513] | 807 | row = 0 |
---|
| 808 | if kwargs.has_key("row"): |
---|
| 809 | row = kwargs.get("row") |
---|
| 810 | data = self._getabcissa(row) |
---|
[113] | 811 | u = self._getcoordinfo()[0] |
---|
[718] | 812 | if rcParams['verbose']: |
---|
[113] | 813 | if u == "": u = "channel" |
---|
[718] | 814 | msg = "The current mask window unit is %s" % u |
---|
[1118] | 815 | i = self._check_ifs() |
---|
| 816 | if not i: |
---|
[876] | 817 | msg += "\nThis mask is only valid for IF=%d" % (self.getif(i)) |
---|
[718] | 818 | asaplog.push(msg) |
---|
[102] | 819 | n = self.nchan() |
---|
[1295] | 820 | msk = _n_bools(n, False) |
---|
[710] | 821 | # test if args is a 'list' or a 'normal *args - UGLY!!! |
---|
| 822 | |
---|
[1118] | 823 | ws = (isinstance(args[-1][-1], int) or isinstance(args[-1][-1], float)) \ |
---|
| 824 | and args or args[0] |
---|
[710] | 825 | for window in ws: |
---|
[102] | 826 | if (len(window) != 2 or window[0] > window[1] ): |
---|
[1118] | 827 | raise TypeError("A window needs to be defined as [min, max]") |
---|
[102] | 828 | for i in range(n): |
---|
[1024] | 829 | if data[i] >= window[0] and data[i] <= window[1]: |
---|
[1295] | 830 | msk[i] = True |
---|
[113] | 831 | if kwargs.has_key('invert'): |
---|
| 832 | if kwargs.get('invert'): |
---|
[1295] | 833 | msk = mask_not(msk) |
---|
[718] | 834 | print_log() |
---|
[102] | 835 | return msk |
---|
[710] | 836 | |
---|
[1446] | 837 | def get_masklist(self, mask=None, row=0): |
---|
[256] | 838 | """ |
---|
[1446] | 839 | Compute and return a list of mask windows, [min, max]. |
---|
| 840 | Parameters: |
---|
| 841 | mask: channel mask, created with create_mask. |
---|
| 842 | row: calcutate the masklist using the specified row |
---|
| 843 | for unit conversions, default is row=0 |
---|
| 844 | only necessary if frequency varies over rows. |
---|
| 845 | Returns: |
---|
| 846 | [min, max], [min2, max2], ... |
---|
| 847 | Pairs of start/end points (inclusive)specifying |
---|
| 848 | the masked regions |
---|
| 849 | """ |
---|
| 850 | if not (isinstance(mask,list) or isinstance(mask, tuple)): |
---|
| 851 | raise TypeError("The mask should be list or tuple.") |
---|
| 852 | if len(mask) < 2: |
---|
| 853 | raise TypeError("The mask elements should be > 1") |
---|
| 854 | if self.nchan() != len(mask): |
---|
| 855 | msg = "Number of channels in scantable != number of mask elements" |
---|
| 856 | raise TypeError(msg) |
---|
| 857 | data = self._getabcissa(row) |
---|
| 858 | u = self._getcoordinfo()[0] |
---|
| 859 | if rcParams['verbose']: |
---|
| 860 | if u == "": u = "channel" |
---|
| 861 | msg = "The current mask window unit is %s" % u |
---|
| 862 | i = self._check_ifs() |
---|
| 863 | if not i: |
---|
| 864 | msg += "\nThis mask is only valid for IF=%d" % (self.getif(i)) |
---|
| 865 | asaplog.push(msg) |
---|
| 866 | masklist=[] |
---|
| 867 | ist, ien = None, None |
---|
| 868 | ist, ien=self.get_mask_indices(mask) |
---|
| 869 | if ist is not None and ien is not None: |
---|
| 870 | for i in xrange(len(ist)): |
---|
| 871 | range=[data[ist[i]],data[ien[i]]] |
---|
| 872 | range.sort() |
---|
| 873 | masklist.append([range[0],range[1]]) |
---|
| 874 | return masklist |
---|
| 875 | |
---|
| 876 | def get_mask_indices(self, mask=None): |
---|
| 877 | """ |
---|
| 878 | Compute and Return lists of mask start indices and mask end indices. |
---|
| 879 | Parameters: |
---|
| 880 | mask: channel mask, created with create_mask. |
---|
| 881 | Returns: |
---|
| 882 | List of mask start indices and that of mask end indices, |
---|
| 883 | i.e., [istart1,istart2,....], [iend1,iend2,....]. |
---|
| 884 | """ |
---|
| 885 | if not (isinstance(mask,list) or isinstance(mask, tuple)): |
---|
| 886 | raise TypeError("The mask should be list or tuple.") |
---|
| 887 | if len(mask) < 2: |
---|
| 888 | raise TypeError("The mask elements should be > 1") |
---|
| 889 | istart=[] |
---|
| 890 | iend=[] |
---|
| 891 | if mask[0]: istart.append(0) |
---|
| 892 | for i in range(len(mask)-1): |
---|
| 893 | if not mask[i] and mask[i+1]: |
---|
| 894 | istart.append(i+1) |
---|
| 895 | elif mask[i] and not mask[i+1]: |
---|
| 896 | iend.append(i) |
---|
| 897 | if mask[len(mask)-1]: iend.append(len(mask)-1) |
---|
| 898 | if len(istart) != len(iend): |
---|
| 899 | raise RuntimeError("Numbers of mask start != mask end.") |
---|
| 900 | for i in range(len(istart)): |
---|
| 901 | if istart[i] > iend[i]: |
---|
| 902 | raise RuntimeError("Mask start index > mask end index") |
---|
| 903 | break |
---|
| 904 | return istart,iend |
---|
| 905 | |
---|
| 906 | # def get_restfreqs(self): |
---|
| 907 | # """ |
---|
| 908 | # Get the restfrequency(s) stored in this scantable. |
---|
| 909 | # The return value(s) are always of unit 'Hz' |
---|
| 910 | # Parameters: |
---|
| 911 | # none |
---|
| 912 | # Returns: |
---|
| 913 | # a list of doubles |
---|
| 914 | # """ |
---|
| 915 | # return list(self._getrestfreqs()) |
---|
| 916 | |
---|
| 917 | def get_restfreqs(self, ids=None): |
---|
| 918 | """ |
---|
[256] | 919 | Get the restfrequency(s) stored in this scantable. |
---|
| 920 | The return value(s) are always of unit 'Hz' |
---|
| 921 | Parameters: |
---|
[1446] | 922 | ids: (optional) a list of MOLECULE_ID for that restfrequency(s) to |
---|
| 923 | be retrieved |
---|
[256] | 924 | Returns: |
---|
[1446] | 925 | dictionary containing ids and a list of doubles for each id |
---|
[256] | 926 | """ |
---|
[1446] | 927 | if ids is None: |
---|
| 928 | rfreqs={} |
---|
| 929 | idlist = self.getmolnos() |
---|
| 930 | for i in idlist: |
---|
| 931 | rfreqs[i]=list(self._getrestfreqs(i)) |
---|
| 932 | return rfreqs |
---|
| 933 | else: |
---|
| 934 | if type(ids)==list or type(ids)==tuple: |
---|
| 935 | rfreqs={} |
---|
| 936 | for i in ids: |
---|
| 937 | rfreqs[i]=list(self._getrestfreqs(i)) |
---|
| 938 | return rfreqs |
---|
| 939 | else: |
---|
| 940 | return list(self._getrestfreqs(ids)) |
---|
| 941 | #return list(self._getrestfreqs(ids)) |
---|
[102] | 942 | |
---|
[931] | 943 | def set_restfreqs(self, freqs=None, unit='Hz'): |
---|
| 944 | """ |
---|
[1446] | 945 | ********NEED TO BE UPDATED begin************ |
---|
[931] | 946 | Set or replace the restfrequency specified and |
---|
| 947 | If the 'freqs' argument holds a scalar, |
---|
| 948 | then that rest frequency will be applied to all the selected |
---|
| 949 | data. If the 'freqs' argument holds |
---|
| 950 | a vector, then it MUST be of equal or smaller length than |
---|
| 951 | the number of IFs (and the available restfrequencies will be |
---|
| 952 | replaced by this vector). In this case, *all* data have |
---|
| 953 | the restfrequency set per IF according |
---|
| 954 | to the corresponding value you give in the 'freqs' vector. |
---|
[1118] | 955 | E.g. 'freqs=[1e9, 2e9]' would mean IF 0 gets restfreq 1e9 and |
---|
[931] | 956 | IF 1 gets restfreq 2e9. |
---|
[1446] | 957 | ********NEED TO BE UPDATED end************ |
---|
[1153] | 958 | You can also specify the frequencies via a linecatalog/ |
---|
| 959 | |
---|
[931] | 960 | Parameters: |
---|
| 961 | freqs: list of rest frequency values or string idenitfiers |
---|
| 962 | unit: unit for rest frequency (default 'Hz') |
---|
[402] | 963 | |
---|
[931] | 964 | Example: |
---|
[1446] | 965 | # set the given restfrequency for the all currently selected IFs |
---|
[931] | 966 | scan.set_restfreqs(freqs=1.4e9) |
---|
[1446] | 967 | # set multiple restfrequencies to all the selected data |
---|
| 968 | scan.set_restfreqs(freqs=[1.4e9, 1.41e9, 1.42e9]) |
---|
| 969 | # If the number of IFs in the data is >= 2 the IF0 gets the first |
---|
| 970 | # value IF1 the second... NOTE that freqs needs to be |
---|
| 971 | # specified in list of list (e.g. [[],[],...] ). |
---|
| 972 | scan.set_restfreqs(freqs=[[1.4e9],[1.67e9]]) |
---|
[931] | 973 | #set the given restfrequency for the whole table (by name) |
---|
| 974 | scan.set_restfreqs(freqs="OH1667") |
---|
[391] | 975 | |
---|
[931] | 976 | Note: |
---|
| 977 | To do more sophisticate Restfrequency setting, e.g. on a |
---|
| 978 | source and IF basis, use scantable.set_selection() before using |
---|
| 979 | this function. |
---|
| 980 | # provide your scantable is call scan |
---|
| 981 | selection = selector() |
---|
| 982 | selection.set_name("ORION*") |
---|
| 983 | selection.set_ifs([1]) |
---|
| 984 | scan.set_selection(selection) |
---|
| 985 | scan.set_restfreqs(freqs=86.6e9) |
---|
| 986 | |
---|
| 987 | """ |
---|
| 988 | varlist = vars() |
---|
[1157] | 989 | from asap import linecatalog |
---|
| 990 | # simple value |
---|
[1118] | 991 | if isinstance(freqs, int) or isinstance(freqs, float): |
---|
[1446] | 992 | # TT mod |
---|
| 993 | #self._setrestfreqs(freqs, "",unit) |
---|
| 994 | self._setrestfreqs([freqs], [""],unit) |
---|
[1157] | 995 | # list of values |
---|
[1118] | 996 | elif isinstance(freqs, list) or isinstance(freqs, tuple): |
---|
[1157] | 997 | # list values are scalars |
---|
[1118] | 998 | if isinstance(freqs[-1], int) or isinstance(freqs[-1], float): |
---|
[1446] | 999 | self._setrestfreqs(freqs, [""],unit) |
---|
[1157] | 1000 | # list values are tuples, (value, name) |
---|
| 1001 | elif isinstance(freqs[-1], dict): |
---|
[1446] | 1002 | #sel = selector() |
---|
| 1003 | #savesel = self._getselection() |
---|
| 1004 | #iflist = self.getifnos() |
---|
| 1005 | #for i in xrange(len(freqs)): |
---|
| 1006 | # sel.set_ifs(iflist[i]) |
---|
| 1007 | # self._setselection(sel) |
---|
| 1008 | # self._setrestfreqs(freqs[i], "",unit) |
---|
| 1009 | #self._setselection(savesel) |
---|
| 1010 | self._setrestfreqs(freqs["value"], |
---|
| 1011 | freqs["name"], "MHz") |
---|
| 1012 | elif isinstance(freqs[-1], list) or isinstance(freqs[-1], tuple): |
---|
[1157] | 1013 | sel = selector() |
---|
| 1014 | savesel = self._getselection() |
---|
[1322] | 1015 | iflist = self.getifnos() |
---|
[1446] | 1016 | if len(freqs)>len(iflist): |
---|
| 1017 | raise ValueError("number of elements in list of list exeeds the current IF selections") |
---|
[1157] | 1018 | for i in xrange(len(freqs)): |
---|
[1322] | 1019 | sel.set_ifs(iflist[i]) |
---|
[1259] | 1020 | self._setselection(sel) |
---|
[1157] | 1021 | self._setrestfreqs(freqs[i]["value"], |
---|
| 1022 | freqs[i]["name"], "MHz") |
---|
| 1023 | self._setselection(savesel) |
---|
| 1024 | # freqs are to be taken from a linecatalog |
---|
[1153] | 1025 | elif isinstance(freqs, linecatalog): |
---|
| 1026 | sel = selector() |
---|
| 1027 | savesel = self._getselection() |
---|
| 1028 | for i in xrange(freqs.nrow()): |
---|
[1322] | 1029 | sel.set_ifs(iflist[i]) |
---|
[1153] | 1030 | self._setselection(sel) |
---|
| 1031 | self._setrestfreqs(freqs.get_frequency(i), |
---|
| 1032 | freqs.get_name(i), "MHz") |
---|
| 1033 | # ensure that we are not iterating past nIF |
---|
| 1034 | if i == self.nif()-1: break |
---|
| 1035 | self._setselection(savesel) |
---|
[931] | 1036 | else: |
---|
| 1037 | return |
---|
| 1038 | self._add_history("set_restfreqs", varlist) |
---|
| 1039 | |
---|
[1360] | 1040 | def shift_refpix(self, delta): |
---|
| 1041 | """ |
---|
| 1042 | Shift the reference pixel of the Spectra Coordinate by an |
---|
| 1043 | integer amount. |
---|
| 1044 | Parameters: |
---|
| 1045 | delta: the amount to shift by |
---|
| 1046 | Note: |
---|
| 1047 | Be careful using this with broadband data. |
---|
| 1048 | """ |
---|
| 1049 | Scantable.shift(self, delta) |
---|
[931] | 1050 | |
---|
[1259] | 1051 | def history(self, filename=None): |
---|
| 1052 | """ |
---|
| 1053 | Print the history. Optionally to a file. |
---|
[1348] | 1054 | Parameters: |
---|
| 1055 | filename: The name of the file to save the history to. |
---|
[1259] | 1056 | """ |
---|
[484] | 1057 | hist = list(self._gethistory()) |
---|
[794] | 1058 | out = "-"*80 |
---|
[484] | 1059 | for h in hist: |
---|
[489] | 1060 | if h.startswith("---"): |
---|
[794] | 1061 | out += "\n"+h |
---|
[489] | 1062 | else: |
---|
| 1063 | items = h.split("##") |
---|
| 1064 | date = items[0] |
---|
| 1065 | func = items[1] |
---|
| 1066 | items = items[2:] |
---|
[794] | 1067 | out += "\n"+date+"\n" |
---|
| 1068 | out += "Function: %s\n Parameters:" % (func) |
---|
[489] | 1069 | for i in items: |
---|
| 1070 | s = i.split("=") |
---|
[1118] | 1071 | out += "\n %s = %s" % (s[0], s[1]) |
---|
[794] | 1072 | out += "\n"+"-"*80 |
---|
[1259] | 1073 | if filename is not None: |
---|
| 1074 | if filename is "": |
---|
| 1075 | filename = 'scantable_history.txt' |
---|
| 1076 | import os |
---|
| 1077 | filename = os.path.expandvars(os.path.expanduser(filename)) |
---|
| 1078 | if not os.path.isdir(filename): |
---|
| 1079 | data = open(filename, 'w') |
---|
| 1080 | data.write(out) |
---|
| 1081 | data.close() |
---|
| 1082 | else: |
---|
| 1083 | msg = "Illegal file name '%s'." % (filename) |
---|
| 1084 | if rcParams['verbose']: |
---|
| 1085 | print msg |
---|
| 1086 | else: |
---|
| 1087 | raise IOError(msg) |
---|
| 1088 | if rcParams['verbose']: |
---|
| 1089 | try: |
---|
| 1090 | from IPython.genutils import page as pager |
---|
| 1091 | except ImportError: |
---|
| 1092 | from pydoc import pager |
---|
| 1093 | pager(out) |
---|
| 1094 | else: |
---|
| 1095 | return out |
---|
[484] | 1096 | return |
---|
[513] | 1097 | # |
---|
| 1098 | # Maths business |
---|
| 1099 | # |
---|
| 1100 | |
---|
[931] | 1101 | def average_time(self, mask=None, scanav=False, weight='tint', align=False): |
---|
[513] | 1102 | """ |
---|
[1070] | 1103 | Return the (time) weighted average of a scan. |
---|
[513] | 1104 | Note: |
---|
[1070] | 1105 | in channels only - align if necessary |
---|
[513] | 1106 | Parameters: |
---|
| 1107 | mask: an optional mask (only used for 'var' and 'tsys' |
---|
| 1108 | weighting) |
---|
[558] | 1109 | scanav: True averages each scan separately |
---|
| 1110 | False (default) averages all scans together, |
---|
[1099] | 1111 | weight: Weighting scheme. |
---|
| 1112 | 'none' (mean no weight) |
---|
| 1113 | 'var' (1/var(spec) weighted) |
---|
| 1114 | 'tsys' (1/Tsys**2 weighted) |
---|
| 1115 | 'tint' (integration time weighted) |
---|
| 1116 | 'tintsys' (Tint/Tsys**2) |
---|
| 1117 | 'median' ( median averaging) |
---|
[535] | 1118 | The default is 'tint' |
---|
[931] | 1119 | align: align the spectra in velocity before averaging. It takes |
---|
| 1120 | the time of the first spectrum as reference time. |
---|
[513] | 1121 | Example: |
---|
| 1122 | # time average the scantable without using a mask |
---|
[710] | 1123 | newscan = scan.average_time() |
---|
[513] | 1124 | """ |
---|
| 1125 | varlist = vars() |
---|
[976] | 1126 | if weight is None: weight = 'TINT' |
---|
[513] | 1127 | if mask is None: mask = () |
---|
[1099] | 1128 | if scanav: scanav = "SCAN" |
---|
| 1129 | else: scanav = "NONE" |
---|
[1118] | 1130 | scan = (self, ) |
---|
[989] | 1131 | try: |
---|
[1118] | 1132 | if align: |
---|
| 1133 | scan = (self.freq_align(insitu=False), ) |
---|
| 1134 | s = None |
---|
| 1135 | if weight.upper() == 'MEDIAN': |
---|
| 1136 | s = scantable(self._math._averagechannel(scan[0], 'MEDIAN', |
---|
| 1137 | scanav)) |
---|
| 1138 | else: |
---|
| 1139 | s = scantable(self._math._average(scan, mask, weight.upper(), |
---|
| 1140 | scanav)) |
---|
| 1141 | except RuntimeError, msg: |
---|
[989] | 1142 | if rcParams['verbose']: |
---|
| 1143 | print msg |
---|
| 1144 | return |
---|
| 1145 | else: raise |
---|
[1099] | 1146 | s._add_history("average_time", varlist) |
---|
[718] | 1147 | print_log() |
---|
[513] | 1148 | return s |
---|
[710] | 1149 | |
---|
[876] | 1150 | def convert_flux(self, jyperk=None, eta=None, d=None, insitu=None): |
---|
[513] | 1151 | """ |
---|
| 1152 | Return a scan where all spectra are converted to either |
---|
| 1153 | Jansky or Kelvin depending upon the flux units of the scan table. |
---|
| 1154 | By default the function tries to look the values up internally. |
---|
| 1155 | If it can't find them (or if you want to over-ride), you must |
---|
| 1156 | specify EITHER jyperk OR eta (and D which it will try to look up |
---|
| 1157 | also if you don't set it). jyperk takes precedence if you set both. |
---|
| 1158 | Parameters: |
---|
| 1159 | jyperk: the Jy / K conversion factor |
---|
| 1160 | eta: the aperture efficiency |
---|
| 1161 | d: the geomtric diameter (metres) |
---|
| 1162 | insitu: if False a new scantable is returned. |
---|
| 1163 | Otherwise, the scaling is done in-situ |
---|
| 1164 | The default is taken from .asaprc (False) |
---|
| 1165 | """ |
---|
| 1166 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1167 | self._math._setinsitu(insitu) |
---|
[513] | 1168 | varlist = vars() |
---|
| 1169 | if jyperk is None: jyperk = -1.0 |
---|
| 1170 | if d is None: d = -1.0 |
---|
| 1171 | if eta is None: eta = -1.0 |
---|
[876] | 1172 | s = scantable(self._math._convertflux(self, d, eta, jyperk)) |
---|
| 1173 | s._add_history("convert_flux", varlist) |
---|
| 1174 | print_log() |
---|
| 1175 | if insitu: self._assign(s) |
---|
| 1176 | else: return s |
---|
[513] | 1177 | |
---|
[876] | 1178 | def gain_el(self, poly=None, filename="", method="linear", insitu=None): |
---|
[513] | 1179 | """ |
---|
| 1180 | Return a scan after applying a gain-elevation correction. |
---|
| 1181 | The correction can be made via either a polynomial or a |
---|
| 1182 | table-based interpolation (and extrapolation if necessary). |
---|
| 1183 | You specify polynomial coefficients, an ascii table or neither. |
---|
| 1184 | If you specify neither, then a polynomial correction will be made |
---|
| 1185 | with built in coefficients known for certain telescopes (an error |
---|
| 1186 | will occur if the instrument is not known). |
---|
| 1187 | The data and Tsys are *divided* by the scaling factors. |
---|
| 1188 | Parameters: |
---|
| 1189 | poly: Polynomial coefficients (default None) to compute a |
---|
| 1190 | gain-elevation correction as a function of |
---|
| 1191 | elevation (in degrees). |
---|
| 1192 | filename: The name of an ascii file holding correction factors. |
---|
| 1193 | The first row of the ascii file must give the column |
---|
| 1194 | names and these MUST include columns |
---|
| 1195 | "ELEVATION" (degrees) and "FACTOR" (multiply data |
---|
| 1196 | by this) somewhere. |
---|
| 1197 | The second row must give the data type of the |
---|
| 1198 | column. Use 'R' for Real and 'I' for Integer. |
---|
| 1199 | An example file would be |
---|
| 1200 | (actual factors are arbitrary) : |
---|
| 1201 | |
---|
| 1202 | TIME ELEVATION FACTOR |
---|
| 1203 | R R R |
---|
| 1204 | 0.1 0 0.8 |
---|
| 1205 | 0.2 20 0.85 |
---|
| 1206 | 0.3 40 0.9 |
---|
| 1207 | 0.4 60 0.85 |
---|
| 1208 | 0.5 80 0.8 |
---|
| 1209 | 0.6 90 0.75 |
---|
| 1210 | method: Interpolation method when correcting from a table. |
---|
| 1211 | Values are "nearest", "linear" (default), "cubic" |
---|
| 1212 | and "spline" |
---|
| 1213 | insitu: if False a new scantable is returned. |
---|
| 1214 | Otherwise, the scaling is done in-situ |
---|
| 1215 | The default is taken from .asaprc (False) |
---|
| 1216 | """ |
---|
| 1217 | |
---|
| 1218 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1219 | self._math._setinsitu(insitu) |
---|
[513] | 1220 | varlist = vars() |
---|
| 1221 | if poly is None: |
---|
[1118] | 1222 | poly = () |
---|
[513] | 1223 | from os.path import expandvars |
---|
| 1224 | filename = expandvars(filename) |
---|
[876] | 1225 | s = scantable(self._math._gainel(self, poly, filename, method)) |
---|
| 1226 | s._add_history("gain_el", varlist) |
---|
| 1227 | print_log() |
---|
| 1228 | if insitu: self._assign(s) |
---|
| 1229 | else: return s |
---|
[710] | 1230 | |
---|
[931] | 1231 | def freq_align(self, reftime=None, method='cubic', insitu=None): |
---|
[513] | 1232 | """ |
---|
| 1233 | Return a scan where all rows have been aligned in frequency/velocity. |
---|
| 1234 | The alignment frequency frame (e.g. LSRK) is that set by function |
---|
| 1235 | set_freqframe. |
---|
| 1236 | Parameters: |
---|
| 1237 | reftime: reference time to align at. By default, the time of |
---|
| 1238 | the first row of data is used. |
---|
| 1239 | method: Interpolation method for regridding the spectra. |
---|
| 1240 | Choose from "nearest", "linear", "cubic" (default) |
---|
| 1241 | and "spline" |
---|
| 1242 | insitu: if False a new scantable is returned. |
---|
| 1243 | Otherwise, the scaling is done in-situ |
---|
| 1244 | The default is taken from .asaprc (False) |
---|
| 1245 | """ |
---|
[931] | 1246 | if insitu is None: insitu = rcParams["insitu"] |
---|
[876] | 1247 | self._math._setinsitu(insitu) |
---|
[513] | 1248 | varlist = vars() |
---|
[931] | 1249 | if reftime is None: reftime = "" |
---|
| 1250 | s = scantable(self._math._freq_align(self, reftime, method)) |
---|
[876] | 1251 | s._add_history("freq_align", varlist) |
---|
| 1252 | print_log() |
---|
| 1253 | if insitu: self._assign(s) |
---|
| 1254 | else: return s |
---|
[513] | 1255 | |
---|
[876] | 1256 | def opacity(self, tau, insitu=None): |
---|
[513] | 1257 | """ |
---|
| 1258 | Apply an opacity correction. The data |
---|
| 1259 | and Tsys are multiplied by the correction factor. |
---|
| 1260 | Parameters: |
---|
| 1261 | tau: Opacity from which the correction factor is |
---|
| 1262 | exp(tau*ZD) |
---|
| 1263 | where ZD is the zenith-distance |
---|
| 1264 | insitu: if False a new scantable is returned. |
---|
| 1265 | Otherwise, the scaling is done in-situ |
---|
| 1266 | The default is taken from .asaprc (False) |
---|
| 1267 | """ |
---|
| 1268 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1269 | self._math._setinsitu(insitu) |
---|
[513] | 1270 | varlist = vars() |
---|
[876] | 1271 | s = scantable(self._math._opacity(self, tau)) |
---|
| 1272 | s._add_history("opacity", varlist) |
---|
| 1273 | print_log() |
---|
| 1274 | if insitu: self._assign(s) |
---|
| 1275 | else: return s |
---|
[513] | 1276 | |
---|
| 1277 | def bin(self, width=5, insitu=None): |
---|
| 1278 | """ |
---|
| 1279 | Return a scan where all spectra have been binned up. |
---|
[1348] | 1280 | Parameters: |
---|
[513] | 1281 | width: The bin width (default=5) in pixels |
---|
| 1282 | insitu: if False a new scantable is returned. |
---|
| 1283 | Otherwise, the scaling is done in-situ |
---|
| 1284 | The default is taken from .asaprc (False) |
---|
| 1285 | """ |
---|
| 1286 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1287 | self._math._setinsitu(insitu) |
---|
[513] | 1288 | varlist = vars() |
---|
[876] | 1289 | s = scantable(self._math._bin(self, width)) |
---|
[1118] | 1290 | s._add_history("bin", varlist) |
---|
[876] | 1291 | print_log() |
---|
| 1292 | if insitu: self._assign(s) |
---|
| 1293 | else: return s |
---|
[513] | 1294 | |
---|
[710] | 1295 | |
---|
[513] | 1296 | def resample(self, width=5, method='cubic', insitu=None): |
---|
| 1297 | """ |
---|
[1348] | 1298 | Return a scan where all spectra have been binned up. |
---|
| 1299 | |
---|
| 1300 | Parameters: |
---|
[513] | 1301 | width: The bin width (default=5) in pixels |
---|
| 1302 | method: Interpolation method when correcting from a table. |
---|
| 1303 | Values are "nearest", "linear", "cubic" (default) |
---|
| 1304 | and "spline" |
---|
| 1305 | insitu: if False a new scantable is returned. |
---|
| 1306 | Otherwise, the scaling is done in-situ |
---|
| 1307 | The default is taken from .asaprc (False) |
---|
| 1308 | """ |
---|
| 1309 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1310 | self._math._setinsitu(insitu) |
---|
[513] | 1311 | varlist = vars() |
---|
[876] | 1312 | s = scantable(self._math._resample(self, method, width)) |
---|
[1118] | 1313 | s._add_history("resample", varlist) |
---|
[876] | 1314 | print_log() |
---|
| 1315 | if insitu: self._assign(s) |
---|
| 1316 | else: return s |
---|
[513] | 1317 | |
---|
| 1318 | |
---|
[946] | 1319 | def average_pol(self, mask=None, weight='none'): |
---|
| 1320 | """ |
---|
| 1321 | Average the Polarisations together. |
---|
| 1322 | Parameters: |
---|
| 1323 | mask: An optional mask defining the region, where the |
---|
| 1324 | averaging will be applied. The output will have all |
---|
| 1325 | specified points masked. |
---|
| 1326 | weight: Weighting scheme. 'none' (default), 'var' (1/var(spec) |
---|
| 1327 | weighted), or 'tsys' (1/Tsys**2 weighted) |
---|
| 1328 | """ |
---|
| 1329 | varlist = vars() |
---|
| 1330 | if mask is None: |
---|
| 1331 | mask = () |
---|
[1010] | 1332 | s = scantable(self._math._averagepol(self, mask, weight.upper())) |
---|
[1118] | 1333 | s._add_history("average_pol", varlist) |
---|
[946] | 1334 | print_log() |
---|
[992] | 1335 | return s |
---|
[513] | 1336 | |
---|
[1145] | 1337 | def average_beam(self, mask=None, weight='none'): |
---|
| 1338 | """ |
---|
| 1339 | Average the Beams together. |
---|
| 1340 | Parameters: |
---|
| 1341 | mask: An optional mask defining the region, where the |
---|
| 1342 | averaging will be applied. The output will have all |
---|
| 1343 | specified points masked. |
---|
| 1344 | weight: Weighting scheme. 'none' (default), 'var' (1/var(spec) |
---|
| 1345 | weighted), or 'tsys' (1/Tsys**2 weighted) |
---|
| 1346 | """ |
---|
| 1347 | varlist = vars() |
---|
| 1348 | if mask is None: |
---|
| 1349 | mask = () |
---|
| 1350 | s = scantable(self._math._averagebeams(self, mask, weight.upper())) |
---|
| 1351 | s._add_history("average_beam", varlist) |
---|
| 1352 | print_log() |
---|
| 1353 | return s |
---|
| 1354 | |
---|
[992] | 1355 | def convert_pol(self, poltype=None): |
---|
| 1356 | """ |
---|
| 1357 | Convert the data to a different polarisation type. |
---|
| 1358 | Parameters: |
---|
| 1359 | poltype: The new polarisation type. Valid types are: |
---|
| 1360 | "linear", "stokes" and "circular" |
---|
| 1361 | """ |
---|
| 1362 | varlist = vars() |
---|
| 1363 | try: |
---|
| 1364 | s = scantable(self._math._convertpol(self, poltype)) |
---|
[1118] | 1365 | except RuntimeError, msg: |
---|
[992] | 1366 | if rcParams['verbose']: |
---|
[1118] | 1367 | print msg |
---|
| 1368 | return |
---|
[992] | 1369 | else: |
---|
| 1370 | raise |
---|
[1118] | 1371 | s._add_history("convert_pol", varlist) |
---|
[992] | 1372 | print_log() |
---|
| 1373 | return s |
---|
| 1374 | |
---|
[876] | 1375 | def smooth(self, kernel="hanning", width=5.0, insitu=None): |
---|
[513] | 1376 | """ |
---|
| 1377 | Smooth the spectrum by the specified kernel (conserving flux). |
---|
| 1378 | Parameters: |
---|
| 1379 | kernel: The type of smoothing kernel. Select from |
---|
[1373] | 1380 | 'hanning' (default), 'gaussian', 'boxcar' and |
---|
| 1381 | 'rmedian' |
---|
[513] | 1382 | width: The width of the kernel in pixels. For hanning this is |
---|
| 1383 | ignored otherwise it defauls to 5 pixels. |
---|
| 1384 | For 'gaussian' it is the Full Width Half |
---|
| 1385 | Maximum. For 'boxcar' it is the full width. |
---|
[1373] | 1386 | For 'rmedian' it is the half width. |
---|
[513] | 1387 | insitu: if False a new scantable is returned. |
---|
| 1388 | Otherwise, the scaling is done in-situ |
---|
| 1389 | The default is taken from .asaprc (False) |
---|
| 1390 | Example: |
---|
| 1391 | none |
---|
| 1392 | """ |
---|
| 1393 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1394 | self._math._setinsitu(insitu) |
---|
[513] | 1395 | varlist = vars() |
---|
[1118] | 1396 | s = scantable(self._math._smooth(self, kernel.lower(), width)) |
---|
[876] | 1397 | s._add_history("smooth", varlist) |
---|
| 1398 | print_log() |
---|
| 1399 | if insitu: self._assign(s) |
---|
| 1400 | else: return s |
---|
[513] | 1401 | |
---|
[876] | 1402 | |
---|
[1389] | 1403 | def poly_baseline(self, mask=None, order=0, plot=False, uselin=False, insitu=None): |
---|
[513] | 1404 | """ |
---|
| 1405 | Return a scan which has been baselined (all rows) by a polynomial. |
---|
| 1406 | Parameters: |
---|
[794] | 1407 | mask: an optional mask |
---|
| 1408 | order: the order of the polynomial (default is 0) |
---|
[1061] | 1409 | plot: plot the fit and the residual. In this each |
---|
| 1410 | indivual fit has to be approved, by typing 'y' |
---|
| 1411 | or 'n' |
---|
[1389] | 1412 | uselin: use linear polynomial fit |
---|
[794] | 1413 | insitu: if False a new scantable is returned. |
---|
| 1414 | Otherwise, the scaling is done in-situ |
---|
| 1415 | The default is taken from .asaprc (False) |
---|
[513] | 1416 | Example: |
---|
| 1417 | # return a scan baselined by a third order polynomial, |
---|
| 1418 | # not using a mask |
---|
| 1419 | bscan = scan.poly_baseline(order=3) |
---|
[579] | 1420 | """ |
---|
[513] | 1421 | if insitu is None: insitu = rcParams['insitu'] |
---|
| 1422 | varlist = vars() |
---|
| 1423 | if mask is None: |
---|
[1295] | 1424 | mask = [True for i in xrange(self.nchan(-1))] |
---|
[513] | 1425 | from asap.asapfitter import fitter |
---|
[1217] | 1426 | try: |
---|
| 1427 | f = fitter() |
---|
| 1428 | f.set_scan(self, mask) |
---|
[1389] | 1429 | if uselin: |
---|
| 1430 | f.set_function(lpoly=order) |
---|
| 1431 | else: |
---|
| 1432 | f.set_function(poly=order) |
---|
[1217] | 1433 | s = f.auto_fit(insitu, plot=plot) |
---|
[1446] | 1434 | # Save parameters of baseline fits as a class attribute. |
---|
| 1435 | # NOTICE: It does not reflect changes in scantable! |
---|
| 1436 | self.blpars = f.blpars |
---|
[1217] | 1437 | s._add_history("poly_baseline", varlist) |
---|
| 1438 | print_log() |
---|
| 1439 | if insitu: self._assign(s) |
---|
| 1440 | else: return s |
---|
| 1441 | except RuntimeError: |
---|
| 1442 | msg = "The fit failed, possibly because it didn't converge." |
---|
| 1443 | if rcParams['verbose']: |
---|
| 1444 | print msg |
---|
| 1445 | return |
---|
| 1446 | else: |
---|
| 1447 | raise RuntimeError(msg) |
---|
[513] | 1448 | |
---|
[1217] | 1449 | |
---|
[1118] | 1450 | def auto_poly_baseline(self, mask=[], edge=(0, 0), order=0, |
---|
[1280] | 1451 | threshold=3, chan_avg_limit=1, plot=False, |
---|
| 1452 | insitu=None): |
---|
[880] | 1453 | """ |
---|
| 1454 | Return a scan which has been baselined (all rows) by a polynomial. |
---|
| 1455 | Spectral lines are detected first using linefinder and masked out |
---|
| 1456 | to avoid them affecting the baseline solution. |
---|
| 1457 | |
---|
| 1458 | Parameters: |
---|
| 1459 | mask: an optional mask retreived from scantable |
---|
| 1460 | edge: an optional number of channel to drop at |
---|
| 1461 | the edge of spectrum. If only one value is |
---|
| 1462 | specified, the same number will be dropped from |
---|
| 1463 | both sides of the spectrum. Default is to keep |
---|
[907] | 1464 | all channels. Nested tuples represent individual |
---|
[976] | 1465 | edge selection for different IFs (a number of spectral |
---|
| 1466 | channels can be different) |
---|
[880] | 1467 | order: the order of the polynomial (default is 0) |
---|
| 1468 | threshold: the threshold used by line finder. It is better to |
---|
| 1469 | keep it large as only strong lines affect the |
---|
| 1470 | baseline solution. |
---|
[1280] | 1471 | chan_avg_limit: |
---|
| 1472 | a maximum number of consequtive spectral channels to |
---|
| 1473 | average during the search of weak and broad lines. |
---|
| 1474 | The default is no averaging (and no search for weak |
---|
| 1475 | lines). If such lines can affect the fitted baseline |
---|
| 1476 | (e.g. a high order polynomial is fitted), increase this |
---|
| 1477 | parameter (usually values up to 8 are reasonable). Most |
---|
| 1478 | users of this method should find the default value |
---|
| 1479 | sufficient. |
---|
[1061] | 1480 | plot: plot the fit and the residual. In this each |
---|
| 1481 | indivual fit has to be approved, by typing 'y' |
---|
| 1482 | or 'n' |
---|
[880] | 1483 | insitu: if False a new scantable is returned. |
---|
| 1484 | Otherwise, the scaling is done in-situ |
---|
| 1485 | The default is taken from .asaprc (False) |
---|
| 1486 | |
---|
| 1487 | Example: |
---|
| 1488 | scan2=scan.auto_poly_baseline(order=7) |
---|
| 1489 | """ |
---|
| 1490 | if insitu is None: insitu = rcParams['insitu'] |
---|
| 1491 | varlist = vars() |
---|
| 1492 | from asap.asapfitter import fitter |
---|
| 1493 | from asap.asaplinefind import linefinder |
---|
| 1494 | from asap import _is_sequence_or_number as _is_valid |
---|
| 1495 | |
---|
[976] | 1496 | # check whether edge is set up for each IF individually |
---|
[1118] | 1497 | individualedge = False; |
---|
| 1498 | if len(edge) > 1: |
---|
| 1499 | if isinstance(edge[0], list) or isinstance(edge[0], tuple): |
---|
| 1500 | individualedge = True; |
---|
[907] | 1501 | |
---|
[1118] | 1502 | if not _is_valid(edge, int) and not individualedge: |
---|
[909] | 1503 | raise ValueError, "Parameter 'edge' has to be an integer or a \ |
---|
[907] | 1504 | pair of integers specified as a tuple. Nested tuples are allowed \ |
---|
| 1505 | to make individual selection for different IFs." |
---|
[919] | 1506 | |
---|
[1118] | 1507 | curedge = (0, 0) |
---|
| 1508 | if individualedge: |
---|
| 1509 | for edgepar in edge: |
---|
| 1510 | if not _is_valid(edgepar, int): |
---|
| 1511 | raise ValueError, "Each element of the 'edge' tuple has \ |
---|
| 1512 | to be a pair of integers or an integer." |
---|
[907] | 1513 | else: |
---|
[1118] | 1514 | curedge = edge; |
---|
[880] | 1515 | |
---|
| 1516 | # setup fitter |
---|
| 1517 | f = fitter() |
---|
| 1518 | f.set_function(poly=order) |
---|
| 1519 | |
---|
| 1520 | # setup line finder |
---|
[1118] | 1521 | fl = linefinder() |
---|
[1268] | 1522 | fl.set_options(threshold=threshold,avg_limit=chan_avg_limit) |
---|
[880] | 1523 | |
---|
| 1524 | if not insitu: |
---|
[1118] | 1525 | workscan = self.copy() |
---|
[880] | 1526 | else: |
---|
[1118] | 1527 | workscan = self |
---|
[880] | 1528 | |
---|
[907] | 1529 | fl.set_scan(workscan) |
---|
| 1530 | |
---|
[1118] | 1531 | rows = range(workscan.nrow()) |
---|
[1446] | 1532 | # Save parameters of baseline fits & masklists as a class attribute. |
---|
| 1533 | # NOTICE: It does not reflect changes in scantable! |
---|
| 1534 | if len(rows) > 0: |
---|
| 1535 | self.blpars=[] |
---|
| 1536 | self.masklists=[] |
---|
[880] | 1537 | asaplog.push("Processing:") |
---|
| 1538 | for r in rows: |
---|
[1118] | 1539 | msg = " Scan[%d] Beam[%d] IF[%d] Pol[%d] Cycle[%d]" % \ |
---|
| 1540 | (workscan.getscan(r), workscan.getbeam(r), workscan.getif(r), \ |
---|
| 1541 | workscan.getpol(r), workscan.getcycle(r)) |
---|
[880] | 1542 | asaplog.push(msg, False) |
---|
[907] | 1543 | |
---|
[976] | 1544 | # figure out edge parameter |
---|
[1118] | 1545 | if individualedge: |
---|
| 1546 | if len(edge) >= workscan.getif(r): |
---|
| 1547 | raise RuntimeError, "Number of edge elements appear to " \ |
---|
| 1548 | "be less than the number of IFs" |
---|
| 1549 | curedge = edge[workscan.getif(r)] |
---|
[919] | 1550 | |
---|
[976] | 1551 | # setup line finder |
---|
[1118] | 1552 | fl.find_lines(r, mask, curedge) |
---|
[1446] | 1553 | outmask=fl.get_mask() |
---|
[880] | 1554 | f.set_scan(workscan, fl.get_mask()) |
---|
| 1555 | f.x = workscan._getabcissa(r) |
---|
| 1556 | f.y = workscan._getspectrum(r) |
---|
| 1557 | f.data = None |
---|
| 1558 | f.fit() |
---|
[1446] | 1559 | |
---|
| 1560 | # Show mask list |
---|
| 1561 | masklist=workscan.get_masklist(fl.get_mask(),row=r) |
---|
| 1562 | msg = "mask range: "+str(masklist) |
---|
| 1563 | asaplog.push(msg, False) |
---|
| 1564 | |
---|
| 1565 | fpar = f.get_parameters() |
---|
[1061] | 1566 | if plot: |
---|
| 1567 | f.plot(residual=True) |
---|
| 1568 | x = raw_input("Accept fit ( [y]/n ): ") |
---|
| 1569 | if x.upper() == 'N': |
---|
[1446] | 1570 | self.blpars.append(None) |
---|
| 1571 | self.masklists.append(None) |
---|
[1061] | 1572 | continue |
---|
[880] | 1573 | workscan._setspectrum(f.fitter.getresidual(), r) |
---|
[1446] | 1574 | self.blpars.append(fpar) |
---|
| 1575 | self.masklists.append(masklist) |
---|
[1061] | 1576 | if plot: |
---|
| 1577 | f._p.unmap() |
---|
| 1578 | f._p = None |
---|
| 1579 | workscan._add_history("auto_poly_baseline", varlist) |
---|
[880] | 1580 | if insitu: |
---|
| 1581 | self._assign(workscan) |
---|
| 1582 | else: |
---|
| 1583 | return workscan |
---|
| 1584 | |
---|
[914] | 1585 | def rotate_linpolphase(self, angle): |
---|
| 1586 | """ |
---|
| 1587 | Rotate the phase of the complex polarization O=Q+iU correlation. |
---|
| 1588 | This is always done in situ in the raw data. So if you call this |
---|
| 1589 | function more than once then each call rotates the phase further. |
---|
| 1590 | Parameters: |
---|
| 1591 | angle: The angle (degrees) to rotate (add) by. |
---|
| 1592 | Examples: |
---|
| 1593 | scan.rotate_linpolphase(2.3) |
---|
| 1594 | """ |
---|
| 1595 | varlist = vars() |
---|
[936] | 1596 | self._math._rotate_linpolphase(self, angle) |
---|
[914] | 1597 | self._add_history("rotate_linpolphase", varlist) |
---|
| 1598 | print_log() |
---|
| 1599 | return |
---|
[710] | 1600 | |
---|
[513] | 1601 | |
---|
[914] | 1602 | def rotate_xyphase(self, angle): |
---|
| 1603 | """ |
---|
| 1604 | Rotate the phase of the XY correlation. This is always done in situ |
---|
| 1605 | in the data. So if you call this function more than once |
---|
| 1606 | then each call rotates the phase further. |
---|
| 1607 | Parameters: |
---|
| 1608 | angle: The angle (degrees) to rotate (add) by. |
---|
| 1609 | Examples: |
---|
| 1610 | scan.rotate_xyphase(2.3) |
---|
| 1611 | """ |
---|
| 1612 | varlist = vars() |
---|
[936] | 1613 | self._math._rotate_xyphase(self, angle) |
---|
[914] | 1614 | self._add_history("rotate_xyphase", varlist) |
---|
| 1615 | print_log() |
---|
| 1616 | return |
---|
| 1617 | |
---|
| 1618 | def swap_linears(self): |
---|
| 1619 | """ |
---|
[1348] | 1620 | Swap the linear polarisations XX and YY, or better the first two |
---|
| 1621 | polarisations as this also works for ciculars. |
---|
[914] | 1622 | """ |
---|
| 1623 | varlist = vars() |
---|
[936] | 1624 | self._math._swap_linears(self) |
---|
[914] | 1625 | self._add_history("swap_linears", varlist) |
---|
| 1626 | print_log() |
---|
| 1627 | return |
---|
| 1628 | |
---|
| 1629 | def invert_phase(self): |
---|
| 1630 | """ |
---|
| 1631 | Invert the phase of the complex polarisation |
---|
| 1632 | """ |
---|
| 1633 | varlist = vars() |
---|
[936] | 1634 | self._math._invert_phase(self) |
---|
[914] | 1635 | self._add_history("invert_phase", varlist) |
---|
| 1636 | print_log() |
---|
| 1637 | return |
---|
| 1638 | |
---|
[876] | 1639 | def add(self, offset, insitu=None): |
---|
[513] | 1640 | """ |
---|
| 1641 | Return a scan where all spectra have the offset added |
---|
| 1642 | Parameters: |
---|
| 1643 | offset: the offset |
---|
| 1644 | insitu: if False a new scantable is returned. |
---|
| 1645 | Otherwise, the scaling is done in-situ |
---|
| 1646 | The default is taken from .asaprc (False) |
---|
| 1647 | """ |
---|
| 1648 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1649 | self._math._setinsitu(insitu) |
---|
[513] | 1650 | varlist = vars() |
---|
[876] | 1651 | s = scantable(self._math._unaryop(self, offset, "ADD", False)) |
---|
[1118] | 1652 | s._add_history("add", varlist) |
---|
[876] | 1653 | print_log() |
---|
| 1654 | if insitu: |
---|
| 1655 | self._assign(s) |
---|
| 1656 | else: |
---|
[513] | 1657 | return s |
---|
| 1658 | |
---|
[1308] | 1659 | def scale(self, factor, tsys=True, insitu=None): |
---|
[513] | 1660 | """ |
---|
| 1661 | Return a scan where all spectra are scaled by the give 'factor' |
---|
| 1662 | Parameters: |
---|
| 1663 | factor: the scaling factor |
---|
| 1664 | insitu: if False a new scantable is returned. |
---|
| 1665 | Otherwise, the scaling is done in-situ |
---|
| 1666 | The default is taken from .asaprc (False) |
---|
| 1667 | tsys: if True (default) then apply the operation to Tsys |
---|
| 1668 | as well as the data |
---|
| 1669 | """ |
---|
| 1670 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1671 | self._math._setinsitu(insitu) |
---|
[513] | 1672 | varlist = vars() |
---|
[876] | 1673 | s = scantable(self._math._unaryop(self, factor, "MUL", tsys)) |
---|
[1118] | 1674 | s._add_history("scale", varlist) |
---|
[876] | 1675 | print_log() |
---|
| 1676 | if insitu: |
---|
| 1677 | self._assign(s) |
---|
| 1678 | else: |
---|
[513] | 1679 | return s |
---|
| 1680 | |
---|
[1348] | 1681 | def auto_quotient(self, preserve=True, mode='paired'): |
---|
[670] | 1682 | """ |
---|
| 1683 | This function allows to build quotients automatically. |
---|
| 1684 | It assumes the observation to have the same numer of |
---|
| 1685 | "ons" and "offs" |
---|
| 1686 | Parameters: |
---|
[710] | 1687 | preserve: you can preserve (default) the continuum or |
---|
| 1688 | remove it. The equations used are |
---|
[670] | 1689 | preserve: Output = Toff * (on/off) - Toff |
---|
[1070] | 1690 | remove: Output = Toff * (on/off) - Ton |
---|
[1348] | 1691 | mode: the on/off detection mode |
---|
| 1692 | 'paired' (default) |
---|
| 1693 | identifies 'off' scans by the |
---|
| 1694 | trailing '_R' (Mopra/Parkes) or |
---|
| 1695 | '_e'/'_w' (Tid) and matches |
---|
| 1696 | on/off pairs from the observing pattern |
---|
| 1697 | 'time' |
---|
| 1698 | finds the closest off in time |
---|
| 1699 | |
---|
[670] | 1700 | """ |
---|
[1348] | 1701 | modes = ["time", "paired"] |
---|
[670] | 1702 | if not mode in modes: |
---|
[876] | 1703 | msg = "please provide valid mode. Valid modes are %s" % (modes) |
---|
| 1704 | raise ValueError(msg) |
---|
| 1705 | varlist = vars() |
---|
[1348] | 1706 | s = None |
---|
| 1707 | if mode.lower() == "paired": |
---|
| 1708 | basesel = self.get_selection() |
---|
[1356] | 1709 | sel = selector()+basesel |
---|
| 1710 | sel.set_query("SRCTYPE==1") |
---|
| 1711 | self.set_selection(sel) |
---|
[1348] | 1712 | offs = self.copy() |
---|
| 1713 | sel.set_query("SRCTYPE==0") |
---|
[1356] | 1714 | self.set_selection(sel) |
---|
[1348] | 1715 | ons = self.copy() |
---|
| 1716 | s = scantable(self._math._quotient(ons, offs, preserve)) |
---|
| 1717 | self.set_selection(basesel) |
---|
| 1718 | elif mode.lower() == "time": |
---|
| 1719 | s = scantable(self._math._auto_quotient(self, mode, preserve)) |
---|
[1118] | 1720 | s._add_history("auto_quotient", varlist) |
---|
[876] | 1721 | print_log() |
---|
| 1722 | return s |
---|
[710] | 1723 | |
---|
[1145] | 1724 | def mx_quotient(self, mask = None, weight='median', preserve=True): |
---|
[1141] | 1725 | """ |
---|
[1143] | 1726 | Form a quotient using "off" beams when observing in "MX" mode. |
---|
| 1727 | Parameters: |
---|
[1145] | 1728 | mask: an optional mask to be used when weight == 'stddev' |
---|
[1143] | 1729 | weight: How to average the off beams. Default is 'median'. |
---|
[1145] | 1730 | preserve: you can preserve (default) the continuum or |
---|
| 1731 | remove it. The equations used are |
---|
| 1732 | preserve: Output = Toff * (on/off) - Toff |
---|
| 1733 | remove: Output = Toff * (on/off) - Ton |
---|
[1217] | 1734 | """ |
---|
[1143] | 1735 | if mask is None: mask = () |
---|
[1141] | 1736 | varlist = vars() |
---|
| 1737 | on = scantable(self._math._mx_extract(self, 'on')) |
---|
[1143] | 1738 | preoff = scantable(self._math._mx_extract(self, 'off')) |
---|
| 1739 | off = preoff.average_time(mask=mask, weight=weight, scanav=False) |
---|
[1217] | 1740 | from asapmath import quotient |
---|
[1145] | 1741 | q = quotient(on, off, preserve) |
---|
[1143] | 1742 | q._add_history("mx_quotient", varlist) |
---|
[1145] | 1743 | print_log() |
---|
[1217] | 1744 | return q |
---|
[513] | 1745 | |
---|
[718] | 1746 | def freq_switch(self, insitu=None): |
---|
| 1747 | """ |
---|
| 1748 | Apply frequency switching to the data. |
---|
| 1749 | Parameters: |
---|
| 1750 | insitu: if False a new scantable is returned. |
---|
| 1751 | Otherwise, the swictching is done in-situ |
---|
| 1752 | The default is taken from .asaprc (False) |
---|
| 1753 | Example: |
---|
| 1754 | none |
---|
| 1755 | """ |
---|
| 1756 | if insitu is None: insitu = rcParams['insitu'] |
---|
[876] | 1757 | self._math._setinsitu(insitu) |
---|
[718] | 1758 | varlist = vars() |
---|
[876] | 1759 | s = scantable(self._math._freqswitch(self)) |
---|
[1118] | 1760 | s._add_history("freq_switch", varlist) |
---|
[876] | 1761 | print_log() |
---|
| 1762 | if insitu: self._assign(s) |
---|
| 1763 | else: return s |
---|
[718] | 1764 | |
---|
[780] | 1765 | def recalc_azel(self): |
---|
| 1766 | """ |
---|
| 1767 | Recalculate the azimuth and elevation for each position. |
---|
| 1768 | Parameters: |
---|
| 1769 | none |
---|
| 1770 | Example: |
---|
| 1771 | """ |
---|
| 1772 | varlist = vars() |
---|
[876] | 1773 | self._recalcazel() |
---|
[780] | 1774 | self._add_history("recalc_azel", varlist) |
---|
| 1775 | print_log() |
---|
| 1776 | return |
---|
| 1777 | |
---|
[513] | 1778 | def __add__(self, other): |
---|
| 1779 | varlist = vars() |
---|
| 1780 | s = None |
---|
| 1781 | if isinstance(other, scantable): |
---|
[1308] | 1782 | s = scantable(self._math._binaryop(self, other, "ADD")) |
---|
[513] | 1783 | elif isinstance(other, float): |
---|
[876] | 1784 | s = scantable(self._math._unaryop(self, other, "ADD", False)) |
---|
[513] | 1785 | else: |
---|
[718] | 1786 | raise TypeError("Other input is not a scantable or float value") |
---|
[513] | 1787 | s._add_history("operator +", varlist) |
---|
[718] | 1788 | print_log() |
---|
[513] | 1789 | return s |
---|
| 1790 | |
---|
| 1791 | def __sub__(self, other): |
---|
| 1792 | """ |
---|
| 1793 | implicit on all axes and on Tsys |
---|
| 1794 | """ |
---|
| 1795 | varlist = vars() |
---|
| 1796 | s = None |
---|
| 1797 | if isinstance(other, scantable): |
---|
[1308] | 1798 | s = scantable(self._math._binaryop(self, other, "SUB")) |
---|
[513] | 1799 | elif isinstance(other, float): |
---|
[876] | 1800 | s = scantable(self._math._unaryop(self, other, "SUB", False)) |
---|
[513] | 1801 | else: |
---|
[718] | 1802 | raise TypeError("Other input is not a scantable or float value") |
---|
[513] | 1803 | s._add_history("operator -", varlist) |
---|
[718] | 1804 | print_log() |
---|
[513] | 1805 | return s |
---|
[710] | 1806 | |
---|
[513] | 1807 | def __mul__(self, other): |
---|
| 1808 | """ |
---|
| 1809 | implicit on all axes and on Tsys |
---|
| 1810 | """ |
---|
| 1811 | varlist = vars() |
---|
| 1812 | s = None |
---|
| 1813 | if isinstance(other, scantable): |
---|
[1308] | 1814 | s = scantable(self._math._binaryop(self, other, "MUL")) |
---|
[513] | 1815 | elif isinstance(other, float): |
---|
[876] | 1816 | s = scantable(self._math._unaryop(self, other, "MUL", False)) |
---|
[513] | 1817 | else: |
---|
[718] | 1818 | raise TypeError("Other input is not a scantable or float value") |
---|
[513] | 1819 | s._add_history("operator *", varlist) |
---|
[718] | 1820 | print_log() |
---|
[513] | 1821 | return s |
---|
| 1822 | |
---|
[710] | 1823 | |
---|
[513] | 1824 | def __div__(self, other): |
---|
| 1825 | """ |
---|
| 1826 | implicit on all axes and on Tsys |
---|
| 1827 | """ |
---|
| 1828 | varlist = vars() |
---|
| 1829 | s = None |
---|
| 1830 | if isinstance(other, scantable): |
---|
[1308] | 1831 | s = scantable(self._math._binaryop(self, other, "DIV")) |
---|
[513] | 1832 | elif isinstance(other, float): |
---|
| 1833 | if other == 0.0: |
---|
[718] | 1834 | raise ZeroDivisionError("Dividing by zero is not recommended") |
---|
[876] | 1835 | s = scantable(self._math._unaryop(self, other, "DIV", False)) |
---|
[513] | 1836 | else: |
---|
[718] | 1837 | raise TypeError("Other input is not a scantable or float value") |
---|
[513] | 1838 | s._add_history("operator /", varlist) |
---|
[718] | 1839 | print_log() |
---|
[513] | 1840 | return s |
---|
| 1841 | |
---|
[530] | 1842 | def get_fit(self, row=0): |
---|
| 1843 | """ |
---|
| 1844 | Print or return the stored fits for a row in the scantable |
---|
| 1845 | Parameters: |
---|
| 1846 | row: the row which the fit has been applied to. |
---|
| 1847 | """ |
---|
| 1848 | if row > self.nrow(): |
---|
| 1849 | return |
---|
[976] | 1850 | from asap.asapfit import asapfit |
---|
[530] | 1851 | fit = asapfit(self._getfit(row)) |
---|
[718] | 1852 | if rcParams['verbose']: |
---|
[530] | 1853 | print fit |
---|
| 1854 | return |
---|
| 1855 | else: |
---|
| 1856 | return fit.as_dict() |
---|
| 1857 | |
---|
[484] | 1858 | def _add_history(self, funcname, parameters): |
---|
| 1859 | # create date |
---|
| 1860 | sep = "##" |
---|
| 1861 | from datetime import datetime |
---|
| 1862 | dstr = datetime.now().strftime('%Y/%m/%d %H:%M:%S') |
---|
| 1863 | hist = dstr+sep |
---|
| 1864 | hist += funcname+sep#cdate+sep |
---|
| 1865 | if parameters.has_key('self'): del parameters['self'] |
---|
[1118] | 1866 | for k, v in parameters.iteritems(): |
---|
[484] | 1867 | if type(v) is dict: |
---|
[1118] | 1868 | for k2, v2 in v.iteritems(): |
---|
[484] | 1869 | hist += k2 |
---|
| 1870 | hist += "=" |
---|
[1118] | 1871 | if isinstance(v2, scantable): |
---|
[484] | 1872 | hist += 'scantable' |
---|
| 1873 | elif k2 == 'mask': |
---|
[1118] | 1874 | if isinstance(v2, list) or isinstance(v2, tuple): |
---|
[513] | 1875 | hist += str(self._zip_mask(v2)) |
---|
| 1876 | else: |
---|
| 1877 | hist += str(v2) |
---|
[484] | 1878 | else: |
---|
[513] | 1879 | hist += str(v2) |
---|
[484] | 1880 | else: |
---|
| 1881 | hist += k |
---|
| 1882 | hist += "=" |
---|
[1118] | 1883 | if isinstance(v, scantable): |
---|
[484] | 1884 | hist += 'scantable' |
---|
| 1885 | elif k == 'mask': |
---|
[1118] | 1886 | if isinstance(v, list) or isinstance(v, tuple): |
---|
[513] | 1887 | hist += str(self._zip_mask(v)) |
---|
| 1888 | else: |
---|
| 1889 | hist += str(v) |
---|
[484] | 1890 | else: |
---|
| 1891 | hist += str(v) |
---|
| 1892 | hist += sep |
---|
| 1893 | hist = hist[:-2] # remove trailing '##' |
---|
| 1894 | self._addhistory(hist) |
---|
| 1895 | |
---|
[710] | 1896 | |
---|
[484] | 1897 | def _zip_mask(self, mask): |
---|
| 1898 | mask = list(mask) |
---|
| 1899 | i = 0 |
---|
| 1900 | segments = [] |
---|
| 1901 | while mask[i:].count(1): |
---|
| 1902 | i += mask[i:].index(1) |
---|
| 1903 | if mask[i:].count(0): |
---|
| 1904 | j = i + mask[i:].index(0) |
---|
| 1905 | else: |
---|
[710] | 1906 | j = len(mask) |
---|
[1118] | 1907 | segments.append([i, j]) |
---|
[710] | 1908 | i = j |
---|
[484] | 1909 | return segments |
---|
[714] | 1910 | |
---|
[626] | 1911 | def _get_ordinate_label(self): |
---|
| 1912 | fu = "("+self.get_fluxunit()+")" |
---|
| 1913 | import re |
---|
| 1914 | lbl = "Intensity" |
---|
[1118] | 1915 | if re.match(".K.", fu): |
---|
[626] | 1916 | lbl = "Brightness Temperature "+ fu |
---|
[1118] | 1917 | elif re.match(".Jy.", fu): |
---|
[626] | 1918 | lbl = "Flux density "+ fu |
---|
| 1919 | return lbl |
---|
[710] | 1920 | |
---|
[876] | 1921 | def _check_ifs(self): |
---|
| 1922 | nchans = [self.nchan(i) for i in range(self.nif(-1))] |
---|
[889] | 1923 | nchans = filter(lambda t: t > 0, nchans) |
---|
[876] | 1924 | return (sum(nchans)/len(nchans) == nchans[0]) |
---|
[976] | 1925 | |
---|
[1496] | 1926 | def _fill(self, names, unit, average, getpt): |
---|
[976] | 1927 | import os |
---|
| 1928 | from asap._asap import stfiller |
---|
| 1929 | first = True |
---|
| 1930 | fullnames = [] |
---|
| 1931 | for name in names: |
---|
| 1932 | name = os.path.expandvars(name) |
---|
| 1933 | name = os.path.expanduser(name) |
---|
| 1934 | if not os.path.exists(name): |
---|
| 1935 | msg = "File '%s' does not exists" % (name) |
---|
| 1936 | if rcParams['verbose']: |
---|
| 1937 | asaplog.push(msg) |
---|
| 1938 | print asaplog.pop().strip() |
---|
| 1939 | return |
---|
| 1940 | raise IOError(msg) |
---|
| 1941 | fullnames.append(name) |
---|
| 1942 | if average: |
---|
| 1943 | asaplog.push('Auto averaging integrations') |
---|
[1079] | 1944 | stype = int(rcParams['scantable.storage'].lower() == 'disk') |
---|
[976] | 1945 | for name in fullnames: |
---|
[1073] | 1946 | tbl = Scantable(stype) |
---|
| 1947 | r = stfiller(tbl) |
---|
[976] | 1948 | msg = "Importing %s..." % (name) |
---|
[1118] | 1949 | asaplog.push(msg, False) |
---|
[976] | 1950 | print_log() |
---|
[1496] | 1951 | r._open(name, -1, -1, getpt) |
---|
[976] | 1952 | r._read() |
---|
[1073] | 1953 | #tbl = r._getdata() |
---|
[976] | 1954 | if average: |
---|
[1118] | 1955 | tbl = self._math._average((tbl, ), (), 'NONE', 'SCAN') |
---|
[976] | 1956 | #tbl = tbl2 |
---|
| 1957 | if not first: |
---|
| 1958 | tbl = self._math._merge([self, tbl]) |
---|
| 1959 | #tbl = tbl2 |
---|
| 1960 | Scantable.__init__(self, tbl) |
---|
| 1961 | r._close() |
---|
[1118] | 1962 | del r, tbl |
---|
[976] | 1963 | first = False |
---|
| 1964 | if unit is not None: |
---|
| 1965 | self.set_fluxunit(unit) |
---|
[1446] | 1966 | #self.set_freqframe(rcParams['scantable.freqframe']) |
---|
[976] | 1967 | |
---|