[102] | 1 | from asap._asap import sdtable
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[226] | 2 | from asap import rcParams
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[189] | 3 | from numarray import ones,zeros
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[102] | 4 | import sys
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| 5 |
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| 6 | class scantable(sdtable):
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| 7 | """
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| 8 | The ASAP container for scans
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| 9 | """
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[113] | 10 |
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[484] | 11 | def __init__(self, filename, average=None, unit=None):
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[102] | 12 | """
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| 13 | Create a scantable from a saved one or make a reference
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| 14 | Parameters:
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[181] | 15 | filename: the name of an asap table on disk
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| 16 | or
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| 17 | the name of a rpfits/sdfits/ms file
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| 18 | (integrations within scans are auto averaged
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| 19 | and the whole file is read)
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| 20 | or
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| 21 | [advanced] a reference to an existing
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[102] | 22 | scantable
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[484] | 23 | average: average all integrations withinb a scan on read.
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| 24 | The default (True) is taken from .asaprc.
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| 25 | unit: brightness unit; must be consistent with K or Jy.
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[340] | 26 | Over-rides the default selected by the reader
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| 27 | (input rpfits/sdfits/ms) or replaces the value
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| 28 | in existing scantables
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[489] | 29 | """
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| 30 | if average is None or type(average) is not bool:
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| 31 | average = rcParams['scantable.autoaverage']
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| 32 |
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[484] | 33 | varlist = vars()
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[226] | 34 | self._vb = rcParams['verbose']
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[113] | 35 | self._p = None
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[484] | 36 |
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[181] | 37 | if isinstance(filename,sdtable):
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| 38 | sdtable.__init__(self, filename)
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[340] | 39 | if unit is not None:
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[346] | 40 | self.set_fluxunit(unit)
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[181] | 41 | else:
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[411] | 42 | import os.path
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| 43 | if not os.path.exists(filename):
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| 44 | print "File '%s' not found." % (filename)
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[226] | 45 | return
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[411] | 46 | filename = os.path.expandvars(filename)
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| 47 | if os.path.isdir(filename):
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[181] | 48 | # crude check if asap table
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[411] | 49 | if os.path.exists(filename+'/table.info'):
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[181] | 50 | sdtable.__init__(self, filename)
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[340] | 51 | if unit is not None:
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| 52 | self.set_fluxunit(unit)
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[181] | 53 | else:
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[411] | 54 | print "The given file '%s'is not a valid asap table." % (filename)
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[226] | 55 | return
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[484] | 56 | else:
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[181] | 57 | from asap._asap import sdreader
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[340] | 58 | ifSel = -1
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| 59 | beamSel = -1
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[345] | 60 | r = sdreader(filename,ifSel,beamSel)
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[181] | 61 | print 'Importing data...'
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[411] | 62 | r._read([-1])
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| 63 | tbl = r._getdata()
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[346] | 64 | if unit is not None:
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| 65 | tbl.set_fluxunit(unit)
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[489] | 66 | if average:
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| 67 | from asap._asap import average as _av
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[226] | 68 | tmp = tuple([tbl])
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| 69 | print 'Auto averaging integrations...'
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[489] | 70 | tbl2 = _av(tmp,(),True,'none')
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[226] | 71 | sdtable.__init__(self,tbl2)
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| 72 | del r,tbl
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| 73 | else:
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| 74 | sdtable.__init__(self,tbl)
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[484] | 75 | self._add_history("scantable", varlist)
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[102] | 76 |
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[451] | 77 | def save(self, name=None, format=None, stokes=False, overwrite=False):
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[116] | 78 | """
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[280] | 79 | Store the scantable on disk. This can be an asap (aips++) Table, SDFITS,
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| 80 | Image FITS or MS2 format.
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[116] | 81 | Parameters:
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[196] | 82 | name: the name of the outputfile. For format="FITS" this
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[489] | 83 | is the directory file name into which all the files
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| 84 | will be written (default is 'asap_FITS')
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[116] | 85 | format: an optional file format. Default is ASAP.
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[280] | 86 | Allowed are - 'ASAP' (save as ASAP [aips++] Table),
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[194] | 87 | 'SDFITS' (save as SDFITS file)
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| 88 | 'FITS' (saves each row as a FITS Image)
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[200] | 89 | 'ASCII' (saves as ascii text file)
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[226] | 90 | 'MS2' (saves as an aips++
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| 91 | MeasurementSet V2)
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[489] | 92 | stokes: Convert to Stokes parameters (only available
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| 93 | currently with FITS and ASCII formats.
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| 94 | Default is False.
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[411] | 95 | overwrite: If the file should be overwritten if it exists.
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[256] | 96 | The default False is to return with warning
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[411] | 97 | without writing the output. USE WITH CARE.
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[116] | 98 | Example:
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| 99 | scan.save('myscan.asap')
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| 100 | scan.save('myscan.sdfits','SDFITS')
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| 101 | """
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[411] | 102 | from os import path
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[226] | 103 | if format is None: format = rcParams['scantable.save']
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[256] | 104 | suffix = '.'+format.lower()
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| 105 | if name is None or name =="":
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| 106 | name = 'scantable'+suffix
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[283] | 107 | print "No filename given. Using default name %s..." % name
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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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| 111 | print "File %s already exists." % name
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| 112 | return
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[451] | 113 | format2 = format.upper()
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| 114 | if format2 == 'ASAP':
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[116] | 115 | self._save(name)
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| 116 | else:
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| 117 | from asap._asap import sdwriter as _sw
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[451] | 118 | w = _sw(format2)
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[445] | 119 | w.write(self, name, stokes)
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[116] | 120 | return
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| 121 |
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[102] | 122 | def copy(self):
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| 123 | """
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| 124 | Return a copy of this scantable.
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| 125 | Parameters:
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[113] | 126 | none
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[102] | 127 | Example:
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| 128 | copiedscan = scan.copy()
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| 129 | """
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[113] | 130 | sd = scantable(sdtable._copy(self))
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| 131 | return sd
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| 132 |
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[102] | 133 | def get_scan(self, scanid=None):
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| 134 | """
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| 135 | Return a specific scan (by scanno) or collection of scans (by
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| 136 | source name) in a new scantable.
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| 137 | Parameters:
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| 138 | scanid: a scanno or a source name
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| 139 | Example:
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[113] | 140 | scan.get_scan('323p459')
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[102] | 141 | # gets all scans containing the source '323p459'
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| 142 | """
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| 143 | if scanid is None:
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| 144 | print "Please specify a scan no or name to retrieve from the scantable"
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| 145 | try:
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| 146 | if type(scanid) is str:
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[113] | 147 | s = sdtable._getsource(self,scanid)
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[102] | 148 | return scantable(s)
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| 149 | elif type(scanid) is int:
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[381] | 150 | s = sdtable._getscan(self,[scanid])
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| 151 | return scantable(s)
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| 152 | elif type(scanid) is list:
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[113] | 153 | s = sdtable._getscan(self,scanid)
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[102] | 154 | return scantable(s)
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[381] | 155 | else:
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| 156 | print "Illegal scanid type, use 'int' or 'list' if ints."
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[102] | 157 | except RuntimeError:
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| 158 | print "Couldn't find any match."
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| 159 |
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| 160 | def __str__(self):
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[381] | 161 | return sdtable._summary(self,True)
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[102] | 162 |
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[381] | 163 | def summary(self,filename=None, verbose=None):
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[102] | 164 | """
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| 165 | Print a summary of the contents of this scantable.
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| 166 | Parameters:
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| 167 | filename: the name of a file to write the putput to
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| 168 | Default - no file output
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[381] | 169 | verbose: print extra info such as the frequency table
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| 170 | The default (False) is taken from .asaprc
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[102] | 171 | """
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[381] | 172 | info = sdtable._summary(self, verbose)
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| 173 | if verbose is None: verbose = rcParams['scantable.verbosesummary']
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[102] | 174 | if filename is not None:
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[256] | 175 | if filename is "":
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| 176 | filename = 'scantable_summary.txt'
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[415] | 177 | from os.path import expandvars, isdir
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[411] | 178 | filename = expandvars(filename)
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[415] | 179 | if not isdir(filename):
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[413] | 180 | data = open(filename, 'w')
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| 181 | data.write(info)
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| 182 | data.close()
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| 183 | else:
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| 184 | print "Illegal file name '%s'." % (filename)
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[102] | 185 | print info
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[484] | 186 |
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[256] | 187 | def set_cursor(self, thebeam=0,theif=0,thepol=0):
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[102] | 188 | """
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| 189 | Set the spectrum for individual operations.
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| 190 | Parameters:
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| 191 | thebeam,theif,thepol: a number
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| 192 | Example:
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[256] | 193 | scan.set_cursor(0,0,1)
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[135] | 194 | pol1sig = scan.stats(all=False) # returns std dev for beam=0
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[181] | 195 | # if=0, pol=1
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[102] | 196 | """
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[484] | 197 | varlist = vars()
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[102] | 198 | self.setbeam(thebeam)
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| 199 | self.setpol(thepol)
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| 200 | self.setif(theif)
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[484] | 201 | self._add_history("set_cursor",varlist)
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[102] | 202 | return
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| 203 |
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[256] | 204 | def get_cursor(self):
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[113] | 205 | """
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| 206 | Return/print a the current 'cursor' into the Beam/IF/Pol cube.
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| 207 | Parameters:
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| 208 | none
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| 209 | Returns:
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| 210 | a list of values (currentBeam,currentIF,currentPol)
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| 211 | Example:
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| 212 | none
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| 213 | """
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[102] | 214 | i = self.getbeam()
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| 215 | j = self.getif()
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| 216 | k = self.getpol()
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[113] | 217 | if self._vb:
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[181] | 218 | print "--------------------------------------------------"
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[256] | 219 | print " Cursor position"
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[181] | 220 | print "--------------------------------------------------"
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[226] | 221 | out = 'Beam=%d IF=%d Pol=%d ' % (i,j,k)
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[113] | 222 | print out
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[102] | 223 | return i,j,k
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| 224 |
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[436] | 225 | def stats(self, stat='stddev', mask=None, allaxes=None):
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[102] | 226 | """
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[135] | 227 | Determine the specified statistic of the current beam/if/pol
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[102] | 228 | Takes a 'mask' as an optional parameter to specify which
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| 229 | channels should be excluded.
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| 230 | Parameters:
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[135] | 231 | stat: 'min', 'max', 'sumsq', 'sum', 'mean'
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| 232 | 'var', 'stddev', 'avdev', 'rms', 'median'
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| 233 | mask: an optional mask specifying where the statistic
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[102] | 234 | should be determined.
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[436] | 235 | allaxes: if True apply to all spectra. Otherwise
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| 236 | apply only to the selected (beam/pol/if)spectra only.
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| 237 | The default is taken from .asaprc (True if none)
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[102] | 238 | Example:
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[113] | 239 | scan.set_unit('channel')
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[102] | 240 | msk = scan.create_mask([100,200],[500,600])
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[135] | 241 | scan.stats(stat='mean', mask=m)
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[102] | 242 | """
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[436] | 243 | if allaxes is None: allaxes = rcParams['scantable.allaxes']
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[135] | 244 | from asap._asap import stats as _stats
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[256] | 245 | from numarray import array,zeros,Float
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[102] | 246 | if mask == None:
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| 247 | mask = ones(self.nchan())
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[256] | 248 | axes = ['Beam','IF','Pol','Time']
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| 249 |
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[436] | 250 | beamSel,IFSel,polSel = (self.getbeam(),self.getif(),self.getpol())
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| 251 | if allaxes:
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[256] | 252 | n = self.nbeam()*self.nif()*self.npol()*self.nrow()
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| 253 | shp = [self.nbeam(),self.nif(),self.npol(),self.nrow()]
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| 254 | arr = array(zeros(n),shape=shp,type=Float)
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| 255 |
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| 256 | for i in range(self.nbeam()):
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| 257 | self.setbeam(i)
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| 258 | for j in range(self.nif()):
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| 259 | self.setif(j)
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| 260 | for k in range(self.npol()):
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| 261 | self.setpol(k)
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| 262 | arr[i,j,k,:] = _stats(self,mask,stat,-1)
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| 263 | retval = {'axes': axes, 'data': arr, 'cursor':None}
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| 264 | tm = [self._gettime(val) for val in range(self.nrow())]
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[181] | 265 | if self._vb:
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[256] | 266 | self._print_values(retval,stat,tm)
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[436] | 267 | self.setbeam(beamSel)
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| 268 | self.setif(IFSel)
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| 269 | self.setpol(polSel)
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[256] | 270 | return retval
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[102] | 271 |
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| 272 | else:
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[241] | 273 | statval = _stats(self,mask,stat,-1)
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[181] | 274 | out = ''
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| 275 | for l in range(self.nrow()):
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| 276 | tm = self._gettime(l)
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| 277 | out += 'Time[%s]:\n' % (tm)
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[436] | 278 | if self.nbeam() > 1: out += ' Beam[%d] ' % (beamSel)
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| 279 | if self.nif() > 1: out += ' IF[%d] ' % (IFSel)
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| 280 | if self.npol() > 1: out += ' Pol[%d] ' % (polSel)
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[181] | 281 | out += '= %3.3f\n' % (statval[l])
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| 282 | out += "--------------------------------------------------\n"
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[226] | 283 |
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[181] | 284 | if self._vb:
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| 285 | print "--------------------------------------------------"
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| 286 | print " ",stat
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| 287 | print "--------------------------------------------------"
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| 288 | print out
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[256] | 289 | retval = {'axes': axes, 'data': array(statval), 'cursor':(i,j,k)}
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| 290 | return retval
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[102] | 291 |
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[436] | 292 | def stddev(self,mask=None, allaxes=None):
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[135] | 293 | """
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| 294 | Determine the standard deviation of the current beam/if/pol
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| 295 | Takes a 'mask' as an optional parameter to specify which
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| 296 | channels should be excluded.
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| 297 | Parameters:
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| 298 | mask: an optional mask specifying where the standard
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| 299 | deviation should be determined.
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[436] | 300 | allaxes: optional flag to show all or a cursor selected
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[226] | 301 | spectrum of Beam/IF/Pol. Default is all or taken
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| 302 | from .asaprc
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[135] | 303 |
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| 304 | Example:
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| 305 | scan.set_unit('channel')
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| 306 | msk = scan.create_mask([100,200],[500,600])
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| 307 | scan.stddev(mask=m)
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| 308 | """
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[436] | 309 | if allaxes is None: allaxes = rcParams['scantable.allaxes']
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| 310 | return self.stats(stat='stddev',mask=mask, allaxes=allaxes);
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[135] | 311 |
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[436] | 312 | def get_tsys(self, allaxes=None):
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[113] | 313 | """
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| 314 | Return the System temperatures.
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| 315 | Parameters:
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[436] | 316 | allaxes: if True apply to all spectra. Otherwise
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| 317 | apply only to the selected (beam/pol/if)spectra only.
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| 318 | The default is taken from .asaprc (True if none)
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[113] | 319 | Returns:
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| 320 | a list of Tsys values.
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| 321 | """
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[436] | 322 | if allaxes is None: allaxes = rcParams['scantable.allaxes']
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[256] | 323 | from numarray import array,zeros,Float
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| 324 | axes = ['Beam','IF','Pol','Time']
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| 325 |
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[436] | 326 | if allaxes:
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[256] | 327 | n = self.nbeam()*self.nif()*self.npol()*self.nrow()
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| 328 | shp = [self.nbeam(),self.nif(),self.npol(),self.nrow()]
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| 329 | arr = array(zeros(n),shape=shp,type=Float)
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| 330 |
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| 331 | for i in range(self.nbeam()):
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| 332 | self.setbeam(i)
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| 333 | for j in range(self.nif()):
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| 334 | self.setif(j)
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| 335 | for k in range(self.npol()):
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| 336 | self.setpol(k)
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| 337 | arr[i,j,k,:] = self._gettsys()
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| 338 | retval = {'axes': axes, 'data': arr, 'cursor':None}
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| 339 | tm = [self._gettime(val) for val in range(self.nrow())]
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[181] | 340 | if self._vb:
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[256] | 341 | self._print_values(retval,'Tsys',tm)
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| 342 | return retval
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| 343 |
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[102] | 344 | else:
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[256] | 345 | i,j,k = (self.getbeam(),self.getif(),self.getpol())
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| 346 | statval = self._gettsys()
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[181] | 347 | out = ''
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| 348 | for l in range(self.nrow()):
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| 349 | tm = self._gettime(l)
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| 350 | out += 'Time[%s]:\n' % (tm)
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| 351 | if self.nbeam() > 1: out += ' Beam[%d] ' % (i)
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| 352 | if self.nif() > 1: out += ' IF[%d] ' % (j)
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| 353 | if self.npol() > 1: out += ' Pol[%d] ' % (k)
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[256] | 354 | out += '= %3.3f\n' % (statval[l])
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| 355 | out += "--------------------------------------------------\n"
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| 356 |
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[181] | 357 | if self._vb:
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| 358 | print "--------------------------------------------------"
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[256] | 359 | print " TSys"
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[181] | 360 | print "--------------------------------------------------"
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| 361 | print out
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[256] | 362 | retval = {'axes': axes, 'data': array(statval), 'cursor':(i,j,k)}
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| 363 | return retval
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[113] | 364 |
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[407] | 365 | def get_time(self, row=-1):
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[113] | 366 | """
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| 367 | Get a list of time stamps for the observations.
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[181] | 368 | Return a string for each integration in the scantable.
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[113] | 369 | Parameters:
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[407] | 370 | row: row no of integration. Default -1 return all rows
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[113] | 371 | Example:
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| 372 | none
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| 373 | """
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| 374 | out = []
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[407] | 375 | if row == -1:
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| 376 | for i in range(self.nrow()):
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| 377 | out.append(self._gettime(i))
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| 378 | return out
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| 379 | else:
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| 380 | if row < self.nrow():
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| 381 | return self._gettime(row)
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[102] | 382 |
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| 383 | def set_unit(self, unit='channel'):
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| 384 | """
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| 385 | Set the unit for all following operations on this scantable
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| 386 | Parameters:
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| 387 | unit: optional unit, default is 'channel'
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[113] | 388 | one of '*Hz','km/s','channel', ''
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[102] | 389 | """
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[484] | 390 | varlist = vars()
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[113] | 391 | if unit in ['','pixel', 'channel']:
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| 392 | unit = ''
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| 393 | inf = list(self._getcoordinfo())
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| 394 | inf[0] = unit
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| 395 | self._setcoordinfo(inf)
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| 396 | if self._p: self.plot()
|
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[484] | 397 | self._add_history("set_unit",varlist)
|
---|
[113] | 398 |
|
---|
[484] | 399 | def set_instrument(self, instr):
|
---|
[358] | 400 | """
|
---|
| 401 | Set the instrument for subsequent processing
|
---|
| 402 | Parameters:
|
---|
[407] | 403 | instr: Select from 'ATPKSMB', 'ATPKSHOH', 'ATMOPRA',
|
---|
| 404 | 'DSS-43' (Tid), 'CEDUNA', and 'HOBART'
|
---|
[358] | 405 | """
|
---|
| 406 | self._setInstrument(instr)
|
---|
[484] | 407 | self._add_history("set_instument",vars())
|
---|
[358] | 408 |
|
---|
[276] | 409 | def set_doppler(self, doppler='RADIO'):
|
---|
| 410 | """
|
---|
| 411 | Set the doppler for all following operations on this scantable.
|
---|
| 412 | Parameters:
|
---|
| 413 | doppler: One of 'RADIO', 'OPTICAL', 'Z', 'BETA', 'GAMMA'
|
---|
| 414 | """
|
---|
[484] | 415 | varlist = vars()
|
---|
[276] | 416 | inf = list(self._getcoordinfo())
|
---|
| 417 | inf[2] = doppler
|
---|
| 418 | self._setcoordinfo(inf)
|
---|
| 419 | if self._p: self.plot()
|
---|
[484] | 420 | self._add_history("set_doppler",vars())
|
---|
[432] | 421 |
|
---|
[226] | 422 | def set_freqframe(self, frame=None):
|
---|
[113] | 423 | """
|
---|
| 424 | Set the frame type of the Spectral Axis.
|
---|
| 425 | Parameters:
|
---|
| 426 | frame: an optional frame type, default 'LSRK'.
|
---|
| 427 | Examples:
|
---|
| 428 | scan.set_freqframe('BARY')
|
---|
| 429 | """
|
---|
[484] | 430 | if frame is None: frame = rcParams['scantable.freqframe']
|
---|
| 431 | varlist = vars()
|
---|
[113] | 432 | valid = ['REST','TOPO','LSRD','LSRK','BARY', \
|
---|
| 433 | 'GEO','GALACTO','LGROUP','CMB']
|
---|
| 434 | if frame in valid:
|
---|
| 435 | inf = list(self._getcoordinfo())
|
---|
| 436 | inf[1] = frame
|
---|
| 437 | self._setcoordinfo(inf)
|
---|
[484] | 438 | self._add_history("set_freqframe",varlist)
|
---|
[102] | 439 | else:
|
---|
[113] | 440 | print "Please specify a valid freq type. Valid types are:\n",valid
|
---|
| 441 |
|
---|
| 442 | def get_unit(self):
|
---|
| 443 | """
|
---|
| 444 | Get the default unit set in this scantable
|
---|
| 445 | Parameters:
|
---|
| 446 | Returns:
|
---|
| 447 | A unit string
|
---|
| 448 | """
|
---|
| 449 | inf = self._getcoordinfo()
|
---|
| 450 | unit = inf[0]
|
---|
| 451 | if unit == '': unit = 'channel'
|
---|
| 452 | return unit
|
---|
[102] | 453 |
|
---|
[158] | 454 | def get_abcissa(self, rowno=0):
|
---|
[102] | 455 | """
|
---|
[158] | 456 | Get the abcissa in the current coordinate setup for the currently
|
---|
[113] | 457 | selected Beam/IF/Pol
|
---|
| 458 | Parameters:
|
---|
[226] | 459 | rowno: an optional row number in the scantable. Default is the
|
---|
| 460 | first row, i.e. rowno=0
|
---|
[113] | 461 | Returns:
|
---|
[407] | 462 | The abcissa values and it's format string (as a dictionary)
|
---|
[113] | 463 | """
|
---|
[256] | 464 | abc = self._getabcissa(rowno)
|
---|
[407] | 465 | lbl = self._getabcissalabel(rowno)
|
---|
[158] | 466 | return abc, lbl
|
---|
[407] | 467 | #return {'abcissa':abc,'label':lbl}
|
---|
[113] | 468 |
|
---|
| 469 | def create_mask(self, *args, **kwargs):
|
---|
| 470 | """
|
---|
[102] | 471 | Compute and return a mask based on [min,max] windows.
|
---|
[189] | 472 | The specified windows are to be INCLUDED, when the mask is
|
---|
[113] | 473 | applied.
|
---|
[102] | 474 | Parameters:
|
---|
| 475 | [min,max],[min2,max2],...
|
---|
| 476 | Pairs of start/end points specifying the regions
|
---|
| 477 | to be masked
|
---|
[189] | 478 | invert: optional argument. If specified as True,
|
---|
| 479 | return an inverted mask, i.e. the regions
|
---|
| 480 | specified are EXCLUDED
|
---|
[102] | 481 | Example:
|
---|
[113] | 482 | scan.set_unit('channel')
|
---|
| 483 |
|
---|
| 484 | a)
|
---|
[102] | 485 | msk = scan.set_mask([400,500],[800,900])
|
---|
[189] | 486 | # masks everything outside 400 and 500
|
---|
[113] | 487 | # and 800 and 900 in the unit 'channel'
|
---|
| 488 |
|
---|
| 489 | b)
|
---|
| 490 | msk = scan.set_mask([400,500],[800,900], invert=True)
|
---|
[189] | 491 | # masks the regions between 400 and 500
|
---|
[113] | 492 | # and 800 and 900 in the unit 'channel'
|
---|
| 493 |
|
---|
[102] | 494 | """
|
---|
[484] | 495 | varlist = vars()
|
---|
[113] | 496 | u = self._getcoordinfo()[0]
|
---|
| 497 | if self._vb:
|
---|
| 498 | if u == "": u = "channel"
|
---|
| 499 | print "The current mask window unit is", u
|
---|
[102] | 500 | n = self.nchan()
|
---|
[256] | 501 | data = self._getabcissa()
|
---|
[189] | 502 | msk = zeros(n)
|
---|
[484] | 503 | for window in args:
|
---|
[102] | 504 | if (len(window) != 2 or window[0] > window[1] ):
|
---|
| 505 | print "A window needs to be defined as [min,max]"
|
---|
| 506 | return
|
---|
| 507 | for i in range(n):
|
---|
[113] | 508 | if data[i] >= window[0] and data[i] < window[1]:
|
---|
[189] | 509 | msk[i] = 1
|
---|
[113] | 510 | if kwargs.has_key('invert'):
|
---|
| 511 | if kwargs.get('invert'):
|
---|
| 512 | from numarray import logical_not
|
---|
| 513 | msk = logical_not(msk)
|
---|
[484] | 514 | self._add_history("create_mask", varlist)
|
---|
[102] | 515 | return msk
|
---|
[113] | 516 |
|
---|
[256] | 517 | def get_restfreqs(self):
|
---|
| 518 | """
|
---|
| 519 | Get the restfrequency(s) stored in this scantable.
|
---|
| 520 | The return value(s) are always of unit 'Hz'
|
---|
| 521 | Parameters:
|
---|
| 522 | none
|
---|
| 523 | Returns:
|
---|
| 524 | a list of doubles
|
---|
| 525 | """
|
---|
| 526 | return list(self._getrestfreqs())
|
---|
[102] | 527 |
|
---|
[402] | 528 | def lines(self):
|
---|
[391] | 529 | """
|
---|
[402] | 530 | Print the list of known spectral lines
|
---|
| 531 | """
|
---|
| 532 | sdtable._lines(self)
|
---|
| 533 |
|
---|
[484] | 534 | def set_restfreqs(self, freqs=None, unit='Hz', lines=None, source=None,
|
---|
| 535 | theif=None):
|
---|
[402] | 536 | """
|
---|
[393] | 537 | Select the restfrequency for the specified source and IF OR
|
---|
| 538 | replace for all IFs. If the 'freqs' argument holds a scalar,
|
---|
| 539 | then that rest frequency will be applied to the selected
|
---|
| 540 | data (and added to the list of available rest frequencies).
|
---|
| 541 | In this way, you can set a rest frequency for each
|
---|
| 542 | source and IF combination. If the 'freqs' argument holds
|
---|
| 543 | a vector, then it MUST be of length the number of IFs
|
---|
| 544 | (and the available restfrequencies will be replaced by
|
---|
| 545 | this vector). In this case, *all* data ('source' and
|
---|
| 546 | 'theif' are ignored) have the restfrequency set per IF according
|
---|
| 547 | to the corresponding value you give in the 'freqs' vector.
|
---|
| 548 | E.g. 'freqs=[1e9,2e9]' would mean IF 0 gets restfreq 1e9 and
|
---|
| 549 | IF 1 gets restfreq 2e9.
|
---|
[402] | 550 |
|
---|
| 551 | You can also specify the frequencies via known line names
|
---|
| 552 | in the argument 'lines'. Use 'freqs' or 'lines'. 'freqs'
|
---|
| 553 | takes precedence. See the list of known names via function
|
---|
| 554 | scantable.lines()
|
---|
[391] | 555 | Parameters:
|
---|
[402] | 556 | freqs: list of rest frequencies
|
---|
[393] | 557 | unit: unit for rest frequency (default 'Hz')
|
---|
[402] | 558 | lines: list of known spectral lines names (alternative to freqs).
|
---|
| 559 | See possible list via scantable.lines()
|
---|
[391] | 560 | source: Source name (blank means all)
|
---|
| 561 | theif: IF (-1 means all)
|
---|
| 562 | Example:
|
---|
[393] | 563 | scan.set_restfreqs(freqs=1.4e9, source='NGC253', theif=2)
|
---|
| 564 | scan.set_restfreqs(freqs=[1.4e9,1.67e9])
|
---|
[391] | 565 | """
|
---|
[484] | 566 | varlist = vars()
|
---|
[391] | 567 | if source is None:
|
---|
| 568 | source = ""
|
---|
| 569 | if theif is None:
|
---|
| 570 | theif = -1
|
---|
[393] | 571 | t = type(freqs)
|
---|
| 572 | if t is int or t is float:
|
---|
| 573 | freqs = [freqs]
|
---|
[402] | 574 | if freqs is None:
|
---|
| 575 | freqs = []
|
---|
| 576 | t = type(lines)
|
---|
| 577 | if t is str:
|
---|
| 578 | lines = [lines]
|
---|
| 579 | if lines is None:
|
---|
| 580 | lines = []
|
---|
| 581 | sdtable._setrestfreqs(self, freqs, unit, lines, source, theif)
|
---|
[484] | 582 | self._add_history("set_restfreqs", varlist)
|
---|
| 583 |
|
---|
[391] | 584 |
|
---|
| 585 |
|
---|
[102] | 586 | def flag_spectrum(self, thebeam, theif, thepol):
|
---|
| 587 | """
|
---|
| 588 | This flags a selected spectrum in the scan 'for good'.
|
---|
| 589 | USE WITH CARE - not reversible.
|
---|
| 590 | Use masks for non-permanent exclusion of channels.
|
---|
| 591 | Parameters:
|
---|
| 592 | thebeam,theif,thepol: all have to be explicitly
|
---|
| 593 | specified
|
---|
| 594 | Example:
|
---|
| 595 | scan.flag_spectrum(0,0,1)
|
---|
| 596 | flags the spectrum for Beam=0, IF=0, Pol=1
|
---|
| 597 | """
|
---|
[407] | 598 | if (thebeam < self.nbeam() and
|
---|
| 599 | theif < self.nif() and
|
---|
| 600 | thepol < self.npol()):
|
---|
| 601 | sdtable.setbeam(self, thebeam)
|
---|
| 602 | sdtable.setif(self, theif)
|
---|
| 603 | sdtable.setpol(self, thepol)
|
---|
| 604 | sdtable._flag(self)
|
---|
[484] | 605 | self._add_history("flag_spectrum", vars())
|
---|
[102] | 606 | else:
|
---|
| 607 | print "Please specify a valid (Beam/IF/Pol)"
|
---|
| 608 | return
|
---|
[113] | 609 |
|
---|
| 610 | def plot(self, what='spectrum',col='Pol', panel=None):
|
---|
| 611 | """
|
---|
| 612 | Plot the spectra contained in the scan. Alternatively you can also
|
---|
| 613 | Plot Tsys vs Time
|
---|
| 614 | Parameters:
|
---|
| 615 | what: a choice of 'spectrum' (default) or 'tsys'
|
---|
[135] | 616 | col: which out of Beams/IFs/Pols should be colour stacked
|
---|
[113] | 617 | panel: set up multiple panels, currently not working.
|
---|
| 618 | """
|
---|
[283] | 619 | print "Warning! Not fully functional. Use plotter.plot() instead"
|
---|
| 620 |
|
---|
[113] | 621 | validcol = {'Beam':self.nbeam(),'IF':self.nif(),'Pol':self.npol()}
|
---|
[124] | 622 |
|
---|
[113] | 623 | validyax = ['spectrum','tsys']
|
---|
[189] | 624 | from asap.asaplot import ASAPlot
|
---|
[113] | 625 | if not self._p:
|
---|
| 626 | self._p = ASAPlot()
|
---|
[189] | 627 | #print "Plotting not enabled"
|
---|
| 628 | #return
|
---|
| 629 | if self._p.is_dead:
|
---|
| 630 | del self._p
|
---|
| 631 | self._p = ASAPlot()
|
---|
[113] | 632 | npan = 1
|
---|
| 633 | x = None
|
---|
| 634 | if what == 'tsys':
|
---|
| 635 | n = self.nrow()
|
---|
| 636 | if n < 2:
|
---|
| 637 | print "Only one integration. Can't plot."
|
---|
| 638 | return
|
---|
[124] | 639 | self._p.hold()
|
---|
| 640 | self._p.clear()
|
---|
[113] | 641 | if panel == 'Time':
|
---|
| 642 | npan = self.nrow()
|
---|
[124] | 643 | self._p.set_panels(rows=npan)
|
---|
[113] | 644 | xlab,ylab,tlab = None,None,None
|
---|
[226] | 645 | self._vb = False
|
---|
[256] | 646 | sel = self.get_cursor()
|
---|
[113] | 647 | for i in range(npan):
|
---|
[226] | 648 | if npan > 1:
|
---|
| 649 | self._p.subplot(i)
|
---|
[113] | 650 | for j in range(validcol[col]):
|
---|
| 651 | x = None
|
---|
| 652 | y = None
|
---|
| 653 | m = None
|
---|
| 654 | tlab = self._getsourcename(i)
|
---|
[124] | 655 | import re
|
---|
| 656 | tlab = re.sub('_S','',tlab)
|
---|
[113] | 657 | if col == 'Beam':
|
---|
| 658 | self.setbeam(j)
|
---|
| 659 | elif col == 'IF':
|
---|
| 660 | self.setif(j)
|
---|
| 661 | elif col == 'Pol':
|
---|
| 662 | self.setpol(j)
|
---|
| 663 | if what == 'tsys':
|
---|
| 664 | x = range(self.nrow())
|
---|
| 665 | xlab = 'Time [pixel]'
|
---|
| 666 | m = list(ones(len(x)))
|
---|
| 667 | y = []
|
---|
| 668 | ylab = r'$T_{sys}$'
|
---|
| 669 | for k in range(len(x)):
|
---|
| 670 | y.append(self._gettsys(k))
|
---|
| 671 | else:
|
---|
[158] | 672 | x,xlab = self.get_abcissa(i)
|
---|
[256] | 673 | y = self._getspectrum(i)
|
---|
[113] | 674 | ylab = r'Flux'
|
---|
[256] | 675 | m = self._getmask(i)
|
---|
[113] | 676 | llab = col+' '+str(j)
|
---|
| 677 | self._p.set_line(label=llab)
|
---|
| 678 | self._p.plot(x,y,m)
|
---|
[124] | 679 | self._p.set_axes('xlabel',xlab)
|
---|
| 680 | self._p.set_axes('ylabel',ylab)
|
---|
| 681 | self._p.set_axes('title',tlab)
|
---|
[113] | 682 | self._p.release()
|
---|
[256] | 683 | self.set_cursor(sel[0],sel[1],sel[2])
|
---|
[226] | 684 | self._vb = rcParams['verbose']
|
---|
[113] | 685 | return
|
---|
[256] | 686 |
|
---|
| 687 | print out
|
---|
| 688 |
|
---|
| 689 | def _print_values(self, dat, label='', timestamps=[]):
|
---|
| 690 | d = dat['data']
|
---|
| 691 | a = dat['axes']
|
---|
| 692 | shp = d.getshape()
|
---|
| 693 | out = ''
|
---|
| 694 | for i in range(shp[3]):
|
---|
| 695 | out += '%s [%s]:\n' % (a[3],timestamps[i])
|
---|
| 696 | t = d[:,:,:,i]
|
---|
| 697 | for j in range(shp[0]):
|
---|
| 698 | if shp[0] > 1: out += ' %s[%d] ' % (a[0],j)
|
---|
| 699 | for k in range(shp[1]):
|
---|
| 700 | if shp[1] > 1: out += ' %s[%d] ' % (a[1],k)
|
---|
| 701 | for l in range(shp[2]):
|
---|
| 702 | if shp[2] > 1: out += ' %s[%d] ' % (a[2],l)
|
---|
| 703 | out += '= %3.3f\n' % (t[j,k,l])
|
---|
[484] | 704 | out += "-"*80
|
---|
| 705 | out += "\n"
|
---|
| 706 | print "-"*80
|
---|
[256] | 707 | print " ", label
|
---|
[484] | 708 | print "-"*80
|
---|
[256] | 709 | print out
|
---|
[484] | 710 |
|
---|
| 711 | def history(self):
|
---|
| 712 | hist = list(self._gethistory())
|
---|
| 713 | print "-"*80
|
---|
| 714 | for h in hist:
|
---|
[489] | 715 | if h.startswith("---"):
|
---|
| 716 | print h
|
---|
| 717 | else:
|
---|
| 718 | items = h.split("##")
|
---|
| 719 | date = items[0]
|
---|
| 720 | func = items[1]
|
---|
| 721 | items = items[2:]
|
---|
| 722 | print date
|
---|
| 723 | print "Function: %s\n Parameters:" % (func)
|
---|
| 724 | for i in items:
|
---|
| 725 | s = i.split("=")
|
---|
| 726 | print " %s = %s" % (s[0],s[1])
|
---|
| 727 | print "-"*80
|
---|
[484] | 728 | return
|
---|
| 729 |
|
---|
| 730 | def _add_history(self, funcname, parameters):
|
---|
| 731 | # create date
|
---|
| 732 | sep = "##"
|
---|
| 733 | from datetime import datetime
|
---|
| 734 | dstr = datetime.now().strftime('%Y/%m/%d %H:%M:%S')
|
---|
| 735 | hist = dstr+sep
|
---|
| 736 | hist += funcname+sep#cdate+sep
|
---|
| 737 | if parameters.has_key('self'): del parameters['self']
|
---|
| 738 | for k,v in parameters.iteritems():
|
---|
| 739 | if type(v) is dict:
|
---|
| 740 | for k2,v2 in v.iteritems():
|
---|
| 741 | hist += k2
|
---|
| 742 | hist += "="
|
---|
| 743 | if isinstance(v2,scantable):
|
---|
| 744 | hist += 'scantable'
|
---|
| 745 | elif k2 == 'mask':
|
---|
| 746 | hist += str(self._zip_mask(v2))
|
---|
| 747 | else:
|
---|
| 748 | hist += str(v2)
|
---|
| 749 | else:
|
---|
| 750 | hist += k
|
---|
| 751 | hist += "="
|
---|
| 752 | if isinstance(v,scantable):
|
---|
| 753 | hist += 'scantable'
|
---|
| 754 | elif k == 'mask':
|
---|
| 755 | hist += str(self._zip_mask(v))
|
---|
| 756 | else:
|
---|
| 757 | hist += str(v)
|
---|
| 758 | hist += sep
|
---|
| 759 | hist = hist[:-2] # remove trailing '##'
|
---|
| 760 | self._addhistory(hist)
|
---|
| 761 |
|
---|
| 762 |
|
---|
| 763 | def _zip_mask(self, mask):
|
---|
| 764 | mask = list(mask)
|
---|
| 765 | i = 0
|
---|
| 766 | segments = []
|
---|
| 767 | while mask[i:].count(1):
|
---|
| 768 | i += mask[i:].index(1)
|
---|
| 769 | if mask[i:].count(0):
|
---|
| 770 | j = i + mask[i:].index(0)
|
---|
| 771 | else:
|
---|
| 772 | j = len(mask)
|
---|
| 773 | segments.append([i,j])
|
---|
| 774 | i = j
|
---|
| 775 | return segments
|
---|