[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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[340] | 11 | def __init__(self, filename, 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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[340] | 23 | unit: brightness unit; must be consistent with K or Jy.
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| 24 | Over-rides the default selected by the reader
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| 25 | (input rpfits/sdfits/ms) or replaces the value
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| 26 | in existing scantables
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[102] | 27 | """
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[226] | 28 | self._vb = rcParams['verbose']
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[113] | 29 | self._p = None
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[181] | 30 | from os import stat as st
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| 31 | import stat
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| 32 | if isinstance(filename,sdtable):
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| 33 | sdtable.__init__(self, filename)
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[340] | 34 | if unit is not None:
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[346] | 35 | self.set_fluxunit(unit)
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[181] | 36 | else:
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[226] | 37 | try:
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| 38 | mode = st(filename)[stat.ST_MODE]
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| 39 | except OSError:
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| 40 | print "File not found"
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| 41 | return
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[181] | 42 | if stat.S_ISDIR(mode):
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| 43 | # crude check if asap table
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| 44 | if stat.S_ISREG(st(filename+'/table.info')[stat.ST_MODE]):
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| 45 | sdtable.__init__(self, filename)
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[340] | 46 | if unit is not None:
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| 47 | self.set_fluxunit(unit)
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[181] | 48 | else:
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| 49 | print 'The given file is not a valid asap table'
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[226] | 50 | return
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| 51 | else:
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| 52 | autoav = rcParams['scantable.autoaverage']
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| 53 |
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[181] | 54 | from asap._asap import sdreader
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[340] | 55 | ifSel = -1
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| 56 | beamSel = -1
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[345] | 57 | r = sdreader(filename,ifSel,beamSel)
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[181] | 58 | print 'Importing data...'
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| 59 | r.read([-1])
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| 60 | tbl = r.getdata()
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[346] | 61 | if unit is not None:
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| 62 | tbl.set_fluxunit(unit)
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[226] | 63 | if autoav:
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| 64 | from asap._asap import average
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| 65 | tmp = tuple([tbl])
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| 66 | print 'Auto averaging integrations...'
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| 67 | tbl2 = average(tmp,(),True,'none')
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| 68 | sdtable.__init__(self,tbl2)
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| 69 | del r,tbl
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| 70 | else:
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| 71 | sdtable.__init__(self,tbl)
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[102] | 72 |
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[256] | 73 | def save(self, name=None, format=None, overwrite=False):
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[116] | 74 | """
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[280] | 75 | Store the scantable on disk. This can be an asap (aips++) Table, SDFITS,
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| 76 | Image FITS or MS2 format.
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[116] | 77 | Parameters:
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[196] | 78 | name: the name of the outputfile. For format="FITS" this
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[280] | 79 | is the directory file name into which all the files will
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| 80 | be written (default is 'asap_FITS')
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[116] | 81 | format: an optional file format. Default is ASAP.
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[280] | 82 | Allowed are - 'ASAP' (save as ASAP [aips++] Table),
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[194] | 83 | 'SDFITS' (save as SDFITS file)
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| 84 | 'FITS' (saves each row as a FITS Image)
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[200] | 85 | 'ASCII' (saves as ascii text file)
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[226] | 86 | 'MS2' (saves as an aips++
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| 87 | MeasurementSet V2)
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[256] | 88 | overwrite: if the file should be overwritten if it exists.
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| 89 | The default False is to return with warning
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| 90 | without writing the output
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[116] | 91 | Example:
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| 92 | scan.save('myscan.asap')
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| 93 | scan.save('myscan.sdfits','SDFITS')
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| 94 | """
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[226] | 95 | if format is None: format = rcParams['scantable.save']
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[256] | 96 | suffix = '.'+format.lower()
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| 97 | if name is None or name =="":
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| 98 | name = 'scantable'+suffix
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[283] | 99 | print "No filename given. Using default name %s..." % name
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[256] | 100 | from os import path
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| 101 | if path.isfile(name) or path.isdir(name):
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| 102 | if not overwrite:
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| 103 | print "File %s already exists." % name
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| 104 | return
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[116] | 105 | if format == 'ASAP':
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| 106 | self._save(name)
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| 107 | else:
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| 108 | from asap._asap import sdwriter as _sw
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[194] | 109 | w = _sw(format)
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| 110 | w.write(self, name)
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[116] | 111 | return
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| 112 |
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[102] | 113 | def copy(self):
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| 114 | """
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| 115 | Return a copy of this scantable.
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| 116 | Parameters:
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[113] | 117 | none
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[102] | 118 | Example:
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| 119 | copiedscan = scan.copy()
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| 120 | """
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[113] | 121 | sd = scantable(sdtable._copy(self))
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| 122 | return sd
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| 123 |
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[102] | 124 | def get_scan(self, scanid=None):
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| 125 | """
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| 126 | Return a specific scan (by scanno) or collection of scans (by
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| 127 | source name) in a new scantable.
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| 128 | Parameters:
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| 129 | scanid: a scanno or a source name
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| 130 | Example:
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[113] | 131 | scan.get_scan('323p459')
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[102] | 132 | # gets all scans containing the source '323p459'
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| 133 | """
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| 134 | if scanid is None:
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| 135 | print "Please specify a scan no or name to retrieve from the scantable"
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| 136 | try:
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| 137 | if type(scanid) is str:
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[113] | 138 | s = sdtable._getsource(self,scanid)
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[102] | 139 | return scantable(s)
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| 140 | elif type(scanid) is int:
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[381] | 141 | s = sdtable._getscan(self,[scanid])
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| 142 | return scantable(s)
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| 143 | elif type(scanid) is list:
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[113] | 144 | s = sdtable._getscan(self,scanid)
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[102] | 145 | return scantable(s)
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[381] | 146 | else:
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| 147 | print "Illegal scanid type, use 'int' or 'list' if ints."
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[102] | 148 | except RuntimeError:
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| 149 | print "Couldn't find any match."
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| 150 |
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| 151 | def __str__(self):
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[381] | 152 | return sdtable._summary(self,True)
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[102] | 153 |
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[381] | 154 | def summary(self,filename=None, verbose=None):
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[102] | 155 | """
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| 156 | Print a summary of the contents of this scantable.
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| 157 | Parameters:
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| 158 | filename: the name of a file to write the putput to
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| 159 | Default - no file output
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[381] | 160 | verbose: print extra info such as the frequency table
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| 161 | The default (False) is taken from .asaprc
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[102] | 162 | """
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[381] | 163 | info = sdtable._summary(self, verbose)
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| 164 | if verbose is None: verbose = rcParams['scantable.verbosesummary']
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[102] | 165 | if filename is not None:
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[256] | 166 | if filename is "":
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| 167 | filename = 'scantable_summary.txt'
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[102] | 168 | data = open(filename, 'w')
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| 169 | data.write(info)
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| 170 | data.close()
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| 171 | print info
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| 172 |
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[256] | 173 | def set_cursor(self, thebeam=0,theif=0,thepol=0):
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[102] | 174 | """
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| 175 | Set the spectrum for individual operations.
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| 176 | Parameters:
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| 177 | thebeam,theif,thepol: a number
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| 178 | Example:
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[256] | 179 | scan.set_cursor(0,0,1)
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[135] | 180 | pol1sig = scan.stats(all=False) # returns std dev for beam=0
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[181] | 181 | # if=0, pol=1
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[102] | 182 | """
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| 183 | self.setbeam(thebeam)
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| 184 | self.setpol(thepol)
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| 185 | self.setif(theif)
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| 186 | return
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| 187 |
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[256] | 188 | def get_cursor(self):
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[113] | 189 | """
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| 190 | Return/print a the current 'cursor' into the Beam/IF/Pol cube.
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| 191 | Parameters:
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| 192 | none
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| 193 | Returns:
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| 194 | a list of values (currentBeam,currentIF,currentPol)
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| 195 | Example:
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| 196 | none
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| 197 | """
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[102] | 198 | i = self.getbeam()
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| 199 | j = self.getif()
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| 200 | k = self.getpol()
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[113] | 201 | if self._vb:
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[181] | 202 | print "--------------------------------------------------"
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[256] | 203 | print " Cursor position"
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[181] | 204 | print "--------------------------------------------------"
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[226] | 205 | out = 'Beam=%d IF=%d Pol=%d ' % (i,j,k)
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[113] | 206 | print out
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[102] | 207 | return i,j,k
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| 208 |
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[226] | 209 | def stats(self, stat='stddev', mask=None, all=None):
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[102] | 210 | """
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[135] | 211 | Determine the specified statistic of the current beam/if/pol
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[102] | 212 | Takes a 'mask' as an optional parameter to specify which
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| 213 | channels should be excluded.
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| 214 | Parameters:
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[135] | 215 | stat: 'min', 'max', 'sumsq', 'sum', 'mean'
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| 216 | 'var', 'stddev', 'avdev', 'rms', 'median'
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| 217 | mask: an optional mask specifying where the statistic
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[102] | 218 | should be determined.
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[241] | 219 | all: if true show all (default or .asaprc) rather
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| 220 | that the cursor selected spectrum of Beam/IF/Pol
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[102] | 221 |
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| 222 | Example:
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[113] | 223 | scan.set_unit('channel')
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[102] | 224 | msk = scan.create_mask([100,200],[500,600])
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[135] | 225 | scan.stats(stat='mean', mask=m)
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[102] | 226 | """
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[226] | 227 | if all is None: all = rcParams['scantable.allaxes']
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[135] | 228 | from asap._asap import stats as _stats
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[256] | 229 | from numarray import array,zeros,Float
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[102] | 230 | if mask == None:
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| 231 | mask = ones(self.nchan())
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[256] | 232 | axes = ['Beam','IF','Pol','Time']
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| 233 |
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[102] | 234 | if all:
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[256] | 235 | n = self.nbeam()*self.nif()*self.npol()*self.nrow()
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| 236 | shp = [self.nbeam(),self.nif(),self.npol(),self.nrow()]
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| 237 | arr = array(zeros(n),shape=shp,type=Float)
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| 238 |
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| 239 | for i in range(self.nbeam()):
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| 240 | self.setbeam(i)
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| 241 | for j in range(self.nif()):
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| 242 | self.setif(j)
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| 243 | for k in range(self.npol()):
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| 244 | self.setpol(k)
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| 245 | arr[i,j,k,:] = _stats(self,mask,stat,-1)
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| 246 | retval = {'axes': axes, 'data': arr, 'cursor':None}
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| 247 | tm = [self._gettime(val) for val in range(self.nrow())]
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[181] | 248 | if self._vb:
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[256] | 249 | self._print_values(retval,stat,tm)
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| 250 | return retval
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[102] | 251 |
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| 252 | else:
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[256] | 253 | i,j,k = (self.getbeam(),self.getif(),self.getpol())
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[241] | 254 | statval = _stats(self,mask,stat,-1)
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[181] | 255 | out = ''
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| 256 | for l in range(self.nrow()):
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| 257 | tm = self._gettime(l)
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| 258 | out += 'Time[%s]:\n' % (tm)
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| 259 | if self.nbeam() > 1: out += ' Beam[%d] ' % (i)
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| 260 | if self.nif() > 1: out += ' IF[%d] ' % (j)
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| 261 | if self.npol() > 1: out += ' Pol[%d] ' % (k)
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| 262 | out += '= %3.3f\n' % (statval[l])
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| 263 | out += "--------------------------------------------------\n"
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[226] | 264 |
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[181] | 265 | if self._vb:
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| 266 | print "--------------------------------------------------"
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| 267 | print " ",stat
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| 268 | print "--------------------------------------------------"
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| 269 | print out
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[256] | 270 | retval = {'axes': axes, 'data': array(statval), 'cursor':(i,j,k)}
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| 271 | return retval
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[102] | 272 |
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[226] | 273 | def stddev(self,mask=None, all=None):
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[135] | 274 | """
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| 275 | Determine the standard deviation of the current beam/if/pol
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| 276 | Takes a 'mask' as an optional parameter to specify which
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| 277 | channels should be excluded.
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| 278 | Parameters:
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| 279 | mask: an optional mask specifying where the standard
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| 280 | deviation should be determined.
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[226] | 281 | all: optional flag to show all or a cursor selected
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| 282 | spectrum of Beam/IF/Pol. Default is all or taken
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| 283 | from .asaprc
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[135] | 284 |
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| 285 | Example:
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| 286 | scan.set_unit('channel')
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| 287 | msk = scan.create_mask([100,200],[500,600])
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| 288 | scan.stddev(mask=m)
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| 289 | """
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[226] | 290 | if all is None: all = rcParams['scantable.allaxes']
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[135] | 291 | return self.stats(stat='stddev',mask=mask, all=all);
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| 292 |
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[226] | 293 | def get_tsys(self, all=None):
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[113] | 294 | """
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| 295 | Return the System temperatures.
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| 296 | Parameters:
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| 297 | all: optional parameter to get the Tsys values for all
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| 298 | Beams/IFs/Pols (default) or just the one selected
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[256] | 299 | with scantable.set_cursor()
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[113] | 300 | [True or False]
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| 301 | Returns:
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| 302 | a list of Tsys values.
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| 303 | """
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[226] | 304 | if all is None: all = rcParams['scantable.allaxes']
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[256] | 305 | from numarray import array,zeros,Float
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| 306 | axes = ['Beam','IF','Pol','Time']
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| 307 |
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[102] | 308 | if all:
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[256] | 309 | n = self.nbeam()*self.nif()*self.npol()*self.nrow()
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| 310 | shp = [self.nbeam(),self.nif(),self.npol(),self.nrow()]
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| 311 | arr = array(zeros(n),shape=shp,type=Float)
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| 312 |
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| 313 | for i in range(self.nbeam()):
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| 314 | self.setbeam(i)
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| 315 | for j in range(self.nif()):
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| 316 | self.setif(j)
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| 317 | for k in range(self.npol()):
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| 318 | self.setpol(k)
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| 319 | arr[i,j,k,:] = self._gettsys()
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| 320 | retval = {'axes': axes, 'data': arr, 'cursor':None}
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| 321 | tm = [self._gettime(val) for val in range(self.nrow())]
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[181] | 322 | if self._vb:
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[256] | 323 | self._print_values(retval,'Tsys',tm)
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| 324 | return retval
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| 325 |
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[102] | 326 | else:
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[256] | 327 | i,j,k = (self.getbeam(),self.getif(),self.getpol())
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| 328 | statval = self._gettsys()
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[181] | 329 | out = ''
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| 330 | for l in range(self.nrow()):
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| 331 | tm = self._gettime(l)
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| 332 | out += 'Time[%s]:\n' % (tm)
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| 333 | if self.nbeam() > 1: out += ' Beam[%d] ' % (i)
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| 334 | if self.nif() > 1: out += ' IF[%d] ' % (j)
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| 335 | if self.npol() > 1: out += ' Pol[%d] ' % (k)
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[256] | 336 | out += '= %3.3f\n' % (statval[l])
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| 337 | out += "--------------------------------------------------\n"
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| 338 |
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[181] | 339 | if self._vb:
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| 340 | print "--------------------------------------------------"
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[256] | 341 | print " TSys"
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[181] | 342 | print "--------------------------------------------------"
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| 343 | print out
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[256] | 344 | retval = {'axes': axes, 'data': array(statval), 'cursor':(i,j,k)}
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| 345 | return retval
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[113] | 346 |
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| 347 | def get_time(self):
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| 348 | """
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| 349 | Get a list of time stamps for the observations.
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[181] | 350 | Return a string for each integration in the scantable.
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[113] | 351 | Parameters:
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| 352 | none
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| 353 | Example:
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| 354 | none
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| 355 | """
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| 356 | out = []
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| 357 | for i in range(self.nrow()):
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| 358 | out.append(self._gettime(i))
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| 359 | return out
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[102] | 360 |
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| 361 | def set_unit(self, unit='channel'):
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| 362 | """
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| 363 | Set the unit for all following operations on this scantable
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| 364 | Parameters:
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| 365 | unit: optional unit, default is 'channel'
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[113] | 366 | one of '*Hz','km/s','channel', ''
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[102] | 367 | """
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[113] | 368 |
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| 369 | if unit in ['','pixel', 'channel']:
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| 370 | unit = ''
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| 371 | inf = list(self._getcoordinfo())
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| 372 | inf[0] = unit
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| 373 | self._setcoordinfo(inf)
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| 374 | if self._p: self.plot()
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| 375 |
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[358] | 376 | def set_instrument (self, instr):
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| 377 | """
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| 378 | Set the instrument for subsequent processing
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| 379 | Parameters:
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| 380 | instr: Select from "ATPKSMB", "ATPKSHOH", "ATMOPRA",
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| 381 | "DSS-43" (Tid), "CEDUNA", and "HOBART"
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| 382 | """
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| 383 | self._setInstrument(instr)
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| 384 |
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[276] | 385 | def set_doppler(self, doppler='RADIO'):
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| 386 | """
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| 387 | Set the doppler for all following operations on this scantable.
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| 388 | Parameters:
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| 389 | doppler: One of 'RADIO', 'OPTICAL', 'Z', 'BETA', 'GAMMA'
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| 390 | """
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| 391 |
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| 392 | inf = list(self._getcoordinfo())
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| 393 | inf[2] = doppler
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| 394 | self._setcoordinfo(inf)
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| 395 | if self._p: self.plot()
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| 396 |
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[226] | 397 | def set_freqframe(self, frame=None):
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[113] | 398 | """
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| 399 | Set the frame type of the Spectral Axis.
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| 400 | Parameters:
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| 401 | frame: an optional frame type, default 'LSRK'.
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| 402 | Examples:
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| 403 | scan.set_freqframe('BARY')
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| 404 | """
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[226] | 405 | if not frame: frame = rcParams['scantable.freqframe']
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[113] | 406 | valid = ['REST','TOPO','LSRD','LSRK','BARY', \
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| 407 | 'GEO','GALACTO','LGROUP','CMB']
|
---|
| 408 | if frame in valid:
|
---|
| 409 | inf = list(self._getcoordinfo())
|
---|
| 410 | inf[1] = frame
|
---|
| 411 | self._setcoordinfo(inf)
|
---|
[102] | 412 | else:
|
---|
[113] | 413 | print "Please specify a valid freq type. Valid types are:\n",valid
|
---|
| 414 |
|
---|
| 415 | def get_unit(self):
|
---|
| 416 | """
|
---|
| 417 | Get the default unit set in this scantable
|
---|
| 418 | Parameters:
|
---|
| 419 | Returns:
|
---|
| 420 | A unit string
|
---|
| 421 | """
|
---|
| 422 | inf = self._getcoordinfo()
|
---|
| 423 | unit = inf[0]
|
---|
| 424 | if unit == '': unit = 'channel'
|
---|
| 425 | return unit
|
---|
[102] | 426 |
|
---|
[158] | 427 | def get_abcissa(self, rowno=0):
|
---|
[102] | 428 | """
|
---|
[158] | 429 | Get the abcissa in the current coordinate setup for the currently
|
---|
[113] | 430 | selected Beam/IF/Pol
|
---|
| 431 | Parameters:
|
---|
[226] | 432 | rowno: an optional row number in the scantable. Default is the
|
---|
| 433 | first row, i.e. rowno=0
|
---|
[113] | 434 | Returns:
|
---|
[158] | 435 | The abcissa values and it's format string.
|
---|
[113] | 436 | """
|
---|
[256] | 437 | abc = self._getabcissa(rowno)
|
---|
| 438 | lbl = self._getabcissalabel(rowno)
|
---|
[158] | 439 | return abc, lbl
|
---|
[113] | 440 |
|
---|
| 441 | def create_mask(self, *args, **kwargs):
|
---|
| 442 | """
|
---|
[102] | 443 | Compute and return a mask based on [min,max] windows.
|
---|
[189] | 444 | The specified windows are to be INCLUDED, when the mask is
|
---|
[113] | 445 | applied.
|
---|
[102] | 446 | Parameters:
|
---|
| 447 | [min,max],[min2,max2],...
|
---|
| 448 | Pairs of start/end points specifying the regions
|
---|
| 449 | to be masked
|
---|
[189] | 450 | invert: optional argument. If specified as True,
|
---|
| 451 | return an inverted mask, i.e. the regions
|
---|
| 452 | specified are EXCLUDED
|
---|
[102] | 453 | Example:
|
---|
[113] | 454 | scan.set_unit('channel')
|
---|
| 455 |
|
---|
| 456 | a)
|
---|
[102] | 457 | msk = scan.set_mask([400,500],[800,900])
|
---|
[189] | 458 | # masks everything outside 400 and 500
|
---|
[113] | 459 | # and 800 and 900 in the unit 'channel'
|
---|
| 460 |
|
---|
| 461 | b)
|
---|
| 462 | msk = scan.set_mask([400,500],[800,900], invert=True)
|
---|
[189] | 463 | # masks the regions between 400 and 500
|
---|
[113] | 464 | # and 800 and 900 in the unit 'channel'
|
---|
| 465 |
|
---|
[102] | 466 | """
|
---|
[113] | 467 | u = self._getcoordinfo()[0]
|
---|
| 468 | if self._vb:
|
---|
| 469 | if u == "": u = "channel"
|
---|
| 470 | print "The current mask window unit is", u
|
---|
[102] | 471 | n = self.nchan()
|
---|
[256] | 472 | data = self._getabcissa()
|
---|
[189] | 473 | msk = zeros(n)
|
---|
[102] | 474 | for window in args:
|
---|
| 475 | if (len(window) != 2 or window[0] > window[1] ):
|
---|
| 476 | print "A window needs to be defined as [min,max]"
|
---|
| 477 | return
|
---|
| 478 | for i in range(n):
|
---|
[113] | 479 | if data[i] >= window[0] and data[i] < window[1]:
|
---|
[189] | 480 | msk[i] = 1
|
---|
[113] | 481 | if kwargs.has_key('invert'):
|
---|
| 482 | if kwargs.get('invert'):
|
---|
| 483 | from numarray import logical_not
|
---|
| 484 | msk = logical_not(msk)
|
---|
[102] | 485 | return msk
|
---|
[113] | 486 |
|
---|
[256] | 487 | def get_restfreqs(self):
|
---|
| 488 | """
|
---|
| 489 | Get the restfrequency(s) stored in this scantable.
|
---|
| 490 | The return value(s) are always of unit 'Hz'
|
---|
| 491 | Parameters:
|
---|
| 492 | none
|
---|
| 493 | Returns:
|
---|
| 494 | a list of doubles
|
---|
| 495 | """
|
---|
| 496 | return list(self._getrestfreqs())
|
---|
[102] | 497 |
|
---|
[393] | 498 | def set_restfreqs(self, freqs, unit='Hz', source=None, theif=None):
|
---|
[391] | 499 | """
|
---|
[393] | 500 | Select the restfrequency for the specified source and IF OR
|
---|
| 501 | replace for all IFs. If the 'freqs' argument holds a scalar,
|
---|
| 502 | then that rest frequency will be applied to the selected
|
---|
| 503 | data (and added to the list of available rest frequencies).
|
---|
| 504 | In this way, you can set a rest frequency for each
|
---|
| 505 | source and IF combination. If the 'freqs' argument holds
|
---|
| 506 | a vector, then it MUST be of length the number of IFs
|
---|
| 507 | (and the available restfrequencies will be replaced by
|
---|
| 508 | this vector). In this case, *all* data ('source' and
|
---|
| 509 | 'theif' are ignored) have the restfrequency set per IF according
|
---|
| 510 | to the corresponding value you give in the 'freqs' vector.
|
---|
| 511 | E.g. 'freqs=[1e9,2e9]' would mean IF 0 gets restfreq 1e9 and
|
---|
| 512 | IF 1 gets restfreq 2e9.
|
---|
[391] | 513 | Parameters:
|
---|
[393] | 514 | freqs: rest frequencies
|
---|
| 515 | unit: unit for rest frequency (default 'Hz')
|
---|
[391] | 516 | source: Source name (blank means all)
|
---|
| 517 | theif: IF (-1 means all)
|
---|
| 518 | Example:
|
---|
[393] | 519 | scan.set_restfreqs(freqs=1.4e9, source='NGC253', theif=2)
|
---|
| 520 | scan.set_restfreqs(freqs=[1.4e9,1.67e9])
|
---|
[391] | 521 | """
|
---|
| 522 | if source is None:
|
---|
| 523 | source = ""
|
---|
| 524 | if theif is None:
|
---|
| 525 | theif = -1
|
---|
[393] | 526 | t = type(freqs)
|
---|
| 527 | if t is int or t is float:
|
---|
| 528 | freqs = [freqs]
|
---|
| 529 | sdtable._setrestfreqs(self, freqs, unit, source, theif)
|
---|
[391] | 530 | return
|
---|
| 531 |
|
---|
| 532 |
|
---|
[102] | 533 | def flag_spectrum(self, thebeam, theif, thepol):
|
---|
| 534 | """
|
---|
| 535 | This flags a selected spectrum in the scan 'for good'.
|
---|
| 536 | USE WITH CARE - not reversible.
|
---|
| 537 | Use masks for non-permanent exclusion of channels.
|
---|
| 538 | Parameters:
|
---|
| 539 | thebeam,theif,thepol: all have to be explicitly
|
---|
| 540 | specified
|
---|
| 541 | Example:
|
---|
| 542 | scan.flag_spectrum(0,0,1)
|
---|
| 543 | flags the spectrum for Beam=0, IF=0, Pol=1
|
---|
| 544 | """
|
---|
| 545 | if (thebeam < self.nbeam() and theif < self.nif() and thepol < self.npol()):
|
---|
| 546 | stable.setbeam(thebeam)
|
---|
| 547 | stable.setif(theif)
|
---|
| 548 | stable.setpol(thepol)
|
---|
| 549 | stable._flag(self)
|
---|
| 550 | else:
|
---|
| 551 | print "Please specify a valid (Beam/IF/Pol)"
|
---|
| 552 | return
|
---|
[113] | 553 |
|
---|
| 554 | def plot(self, what='spectrum',col='Pol', panel=None):
|
---|
| 555 | """
|
---|
| 556 | Plot the spectra contained in the scan. Alternatively you can also
|
---|
| 557 | Plot Tsys vs Time
|
---|
| 558 | Parameters:
|
---|
| 559 | what: a choice of 'spectrum' (default) or 'tsys'
|
---|
[135] | 560 | col: which out of Beams/IFs/Pols should be colour stacked
|
---|
[113] | 561 | panel: set up multiple panels, currently not working.
|
---|
| 562 | """
|
---|
[283] | 563 | print "Warning! Not fully functional. Use plotter.plot() instead"
|
---|
| 564 |
|
---|
[113] | 565 | validcol = {'Beam':self.nbeam(),'IF':self.nif(),'Pol':self.npol()}
|
---|
[124] | 566 |
|
---|
[113] | 567 | validyax = ['spectrum','tsys']
|
---|
[189] | 568 | from asap.asaplot import ASAPlot
|
---|
[113] | 569 | if not self._p:
|
---|
| 570 | self._p = ASAPlot()
|
---|
[189] | 571 | #print "Plotting not enabled"
|
---|
| 572 | #return
|
---|
| 573 | if self._p.is_dead:
|
---|
| 574 | del self._p
|
---|
| 575 | self._p = ASAPlot()
|
---|
[113] | 576 | npan = 1
|
---|
| 577 | x = None
|
---|
| 578 | if what == 'tsys':
|
---|
| 579 | n = self.nrow()
|
---|
| 580 | if n < 2:
|
---|
| 581 | print "Only one integration. Can't plot."
|
---|
| 582 | return
|
---|
[124] | 583 | self._p.hold()
|
---|
| 584 | self._p.clear()
|
---|
[113] | 585 | if panel == 'Time':
|
---|
| 586 | npan = self.nrow()
|
---|
[124] | 587 | self._p.set_panels(rows=npan)
|
---|
[113] | 588 | xlab,ylab,tlab = None,None,None
|
---|
[226] | 589 | self._vb = False
|
---|
[256] | 590 | sel = self.get_cursor()
|
---|
[113] | 591 | for i in range(npan):
|
---|
[226] | 592 | if npan > 1:
|
---|
| 593 | self._p.subplot(i)
|
---|
[113] | 594 | for j in range(validcol[col]):
|
---|
| 595 | x = None
|
---|
| 596 | y = None
|
---|
| 597 | m = None
|
---|
| 598 | tlab = self._getsourcename(i)
|
---|
[124] | 599 | import re
|
---|
| 600 | tlab = re.sub('_S','',tlab)
|
---|
[113] | 601 | if col == 'Beam':
|
---|
| 602 | self.setbeam(j)
|
---|
| 603 | elif col == 'IF':
|
---|
| 604 | self.setif(j)
|
---|
| 605 | elif col == 'Pol':
|
---|
| 606 | self.setpol(j)
|
---|
| 607 | if what == 'tsys':
|
---|
| 608 | x = range(self.nrow())
|
---|
| 609 | xlab = 'Time [pixel]'
|
---|
| 610 | m = list(ones(len(x)))
|
---|
| 611 | y = []
|
---|
| 612 | ylab = r'$T_{sys}$'
|
---|
| 613 | for k in range(len(x)):
|
---|
| 614 | y.append(self._gettsys(k))
|
---|
| 615 | else:
|
---|
[158] | 616 | x,xlab = self.get_abcissa(i)
|
---|
[256] | 617 | y = self._getspectrum(i)
|
---|
[113] | 618 | ylab = r'Flux'
|
---|
[256] | 619 | m = self._getmask(i)
|
---|
[113] | 620 | llab = col+' '+str(j)
|
---|
| 621 | self._p.set_line(label=llab)
|
---|
| 622 | self._p.plot(x,y,m)
|
---|
[124] | 623 | self._p.set_axes('xlabel',xlab)
|
---|
| 624 | self._p.set_axes('ylabel',ylab)
|
---|
| 625 | self._p.set_axes('title',tlab)
|
---|
[113] | 626 | self._p.release()
|
---|
[256] | 627 | self.set_cursor(sel[0],sel[1],sel[2])
|
---|
[226] | 628 | self._vb = rcParams['verbose']
|
---|
[113] | 629 | return
|
---|
[256] | 630 |
|
---|
| 631 | print out
|
---|
| 632 |
|
---|
| 633 | def _print_values(self, dat, label='', timestamps=[]):
|
---|
| 634 | d = dat['data']
|
---|
| 635 | a = dat['axes']
|
---|
| 636 | shp = d.getshape()
|
---|
| 637 | out = ''
|
---|
| 638 | for i in range(shp[3]):
|
---|
| 639 | out += '%s [%s]:\n' % (a[3],timestamps[i])
|
---|
| 640 | t = d[:,:,:,i]
|
---|
| 641 | for j in range(shp[0]):
|
---|
| 642 | if shp[0] > 1: out += ' %s[%d] ' % (a[0],j)
|
---|
| 643 | for k in range(shp[1]):
|
---|
| 644 | if shp[1] > 1: out += ' %s[%d] ' % (a[1],k)
|
---|
| 645 | for l in range(shp[2]):
|
---|
| 646 | if shp[2] > 1: out += ' %s[%d] ' % (a[2],l)
|
---|
| 647 | out += '= %3.3f\n' % (t[j,k,l])
|
---|
| 648 | out += "--------------------------------------------------\n"
|
---|
| 649 | print "--------------------------------------------------"
|
---|
| 650 | print " ", label
|
---|
| 651 | print "--------------------------------------------------"
|
---|
| 652 | print out
|
---|