[100] | 1 | """
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| 2 | This is the ATNF Single Dish Analysis package.
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| 3 |
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| 4 | """
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[1080] | 5 | import os,sys,shutil, platform
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[1691] | 6 | try:
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| 7 | from functools import wraps as wraps_dec
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| 8 | except ImportError:
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| 9 | from asap.compatibility import wraps as wraps_dec
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[226] | 10 |
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[1080] | 11 | # Set up AIPSPATH and first time use of asap i.e. ~/.asap/*
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| 12 | plf = None
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| 13 | if sys.platform == "linux2":
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| 14 | if platform.architecture()[0] == '64bit':
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| 15 | plf = 'linux_64b'
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| 16 | else:
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| 17 | plf = 'linux_gnu'
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| 18 | elif sys.platform == 'darwin':
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| 19 | plf = 'darwin'
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| 20 | else:
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| 21 | # Shouldn't happen - default to linux
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| 22 | plf = 'linux'
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| 23 | asapdata = __path__[-1]
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[1171] | 24 | # Allow user defined data location
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| 25 | if os.environ.has_key("ASAPDATA"):
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| 26 | if os.path.exists(os.environ["ASAPDATA"]):
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| 27 | asapdata = os.environ["ASAPDATA"]
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[1371] | 28 | # use AIPSPATH if defined and "data" dir present
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| 29 | if not os.environ.has_key("AIPSPATH") or \
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| 30 | not os.path.exists(os.environ["AIPSPATH"].split()[0]+"/data"):
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[1316] | 31 | os.environ["AIPSPATH"] = "%s %s somwhere" % ( asapdata, plf)
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[1171] | 32 | # set up user space
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[1080] | 33 | userdir = os.environ["HOME"]+"/.asap"
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| 34 | if not os.path.exists(userdir):
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| 35 | print 'First time ASAP use. Setting up ~/.asap'
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| 36 | os.mkdir(userdir)
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| 37 | shutil.copyfile(asapdata+"/data/ipythonrc-asap", userdir+"/ipythonrc-asap")
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[1588] | 38 | shutil.copyfile(asapdata+"/data/ipy_user_conf.py",
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[1434] | 39 | userdir+"/ipy_user_conf.py")
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[1080] | 40 | f = file(userdir+"/asapuserfuncs.py", "w")
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| 41 | f.close()
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| 42 | f = file(userdir+"/ipythonrc", "w")
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| 43 | f.close()
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[1472] | 44 | else:
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| 45 | # upgrade to support later ipython versions
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| 46 | if not os.path.exists(userdir+"/ipy_user_conf.py"):
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[1588] | 47 | shutil.copyfile(asapdata+"/data/ipy_user_conf.py",
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[1472] | 48 | userdir+"/ipy_user_conf.py")
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| 49 |
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[1171] | 50 | # remove from namespace
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[1080] | 51 | del asapdata, userdir, shutil, platform
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| 52 |
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[513] | 53 | def _validate_bool(b):
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[226] | 54 | 'Convert b to a boolean or raise'
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| 55 | bl = b.lower()
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| 56 | if bl in ('f', 'no', 'false', '0', 0): return False
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| 57 | elif bl in ('t', 'yes', 'true', '1', 1): return True
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| 58 | else:
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| 59 | raise ValueError('Could not convert "%s" to boolean' % b)
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| 60 |
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[513] | 61 | def _validate_int(s):
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[226] | 62 | 'convert s to int or raise'
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| 63 | try: return int(s)
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| 64 | except ValueError:
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| 65 | raise ValueError('Could not convert "%s" to int' % s)
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| 66 |
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[513] | 67 | def _asap_fname():
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[226] | 68 | """
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| 69 | Return the path to the rc file
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| 70 |
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| 71 | Search order:
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| 72 |
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| 73 | * current working dir
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| 74 | * environ var ASAPRC
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[274] | 75 | * HOME/.asaprc
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[706] | 76 |
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[226] | 77 | """
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| 78 |
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| 79 | fname = os.path.join( os.getcwd(), '.asaprc')
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| 80 | if os.path.exists(fname): return fname
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| 81 |
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| 82 | if os.environ.has_key('ASAPRC'):
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| 83 | path = os.environ['ASAPRC']
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| 84 | if os.path.exists(path):
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| 85 | fname = os.path.join(path, '.asaprc')
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| 86 | if os.path.exists(fname):
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| 87 | return fname
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| 88 |
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| 89 | if os.environ.has_key('HOME'):
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| 90 | home = os.environ['HOME']
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| 91 | fname = os.path.join(home, '.asaprc')
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| 92 | if os.path.exists(fname):
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| 93 | return fname
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| 94 | return None
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| 95 |
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[706] | 96 |
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[226] | 97 | defaultParams = {
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| 98 | # general
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[513] | 99 | 'verbose' : [True, _validate_bool],
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| 100 | 'useplotter' : [True, _validate_bool],
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[542] | 101 | 'insitu' : [True, _validate_bool],
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[706] | 102 |
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[226] | 103 | # plotting
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[706] | 104 | 'plotter.gui' : [True, _validate_bool],
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[226] | 105 | 'plotter.stacking' : ['p', str],
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| 106 | 'plotter.panelling' : ['s', str],
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[700] | 107 | 'plotter.colours' : ['', str],
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| 108 | 'plotter.linestyles' : ['', str],
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[710] | 109 | 'plotter.decimate' : [False, _validate_bool],
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| 110 | 'plotter.ganged' : [True, _validate_bool],
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[1022] | 111 | 'plotter.histogram' : [False, _validate_bool],
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[1097] | 112 | 'plotter.papertype' : ['A4', str],
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[1560] | 113 | 'plotter.axesformatting' : ['mpl', str],
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[710] | 114 |
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[226] | 115 | # scantable
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| 116 | 'scantable.save' : ['ASAP', str],
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[513] | 117 | 'scantable.autoaverage' : [True, _validate_bool],
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[226] | 118 | 'scantable.freqframe' : ['LSRK', str], #default frequency frame
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[1076] | 119 | 'scantable.verbosesummary' : [False, _validate_bool],
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[1422] | 120 | 'scantable.storage' : ['memory', str],
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[1504] | 121 | 'scantable.history' : [True, _validate_bool],
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[1586] | 122 | 'scantable.reference' : ['.*(e|w|_R)$', str],
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| 123 | 'scantable.parallactify' : [False, _validate_bool]
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[226] | 124 | # fitter
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| 125 | }
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| 126 |
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[255] | 127 | def list_rcparameters():
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[706] | 128 |
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[255] | 129 | print """
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[737] | 130 | # general
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| 131 | # print verbose output
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| 132 | verbose : True
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[255] | 133 |
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[737] | 134 | # preload a default plotter
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| 135 | useplotter : True
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[255] | 136 |
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[737] | 137 | # apply operations on the input scantable or return new one
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| 138 | insitu : True
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[706] | 139 |
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[737] | 140 | # plotting
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[710] | 141 |
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[737] | 142 | # do we want a GUI or plot to a file
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| 143 | plotter.gui : True
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[710] | 144 |
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[737] | 145 | # default mode for colour stacking
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| 146 | plotter.stacking : Pol
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[255] | 147 |
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[737] | 148 | # default mode for panelling
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| 149 | plotter.panelling : scan
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[255] | 150 |
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[1560] | 151 | # push panels together, to share axis labels
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[737] | 152 | plotter.ganged : True
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[710] | 153 |
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[1513] | 154 | # decimate the number of points plotted by a factor of
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[737] | 155 | # nchan/1024
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| 156 | plotter.decimate : False
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[733] | 157 |
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[737] | 158 | # default colours/linestyles
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| 159 | plotter.colours :
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| 160 | plotter.linestyles :
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[700] | 161 |
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[1022] | 162 | # enable/disable histogram plotting
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| 163 | plotter.histogram : False
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| 164 |
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[1097] | 165 | # ps paper type
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| 166 | plotter.papertype : A4
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| 167 |
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[1513] | 168 | # The formatting style of the xaxis
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[1560] | 169 | plotter.axesformatting : 'mpl' (default) or 'asap' (for old versions of matplotlib)
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[1513] | 170 |
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[737] | 171 | # scantable
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[1076] | 172 |
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[1259] | 173 | # default storage of scantable ('memory'/'disk')
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[1076] | 174 | scantable.storage : memory
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[1422] | 175 |
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| 176 | # write history of each call to scantable
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| 177 | scantable.history : True
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| 178 |
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[737] | 179 | # default ouput format when saving
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| 180 | scantable.save : ASAP
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[1422] | 181 |
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[737] | 182 | # auto averaging on read
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| 183 | scantable.autoaverage : True
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[255] | 184 |
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[737] | 185 | # default frequency frame to set when function
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[1097] | 186 | # scantable.set_freqframe is called
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[737] | 187 | scantable.freqframe : LSRK
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[255] | 188 |
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[737] | 189 | # Control the level of information printed by summary
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| 190 | scantable.verbosesummary : False
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[706] | 191 |
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[1504] | 192 | # Control the identification of reference (off) scans
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| 193 | # This is has to be a regular expression
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[1595] | 194 | scantable.reference : .*(e|w|_R)$
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[1560] | 195 |
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[1595] | 196 | # Indicate whether the data was parallactified (total phase offest == 0.0)
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| 197 | scantable.parallactify : False
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| 198 |
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[737] | 199 | # Fitter
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| 200 | """
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[706] | 201 |
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[226] | 202 | def rc_params():
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| 203 | 'Return the default params updated from the values in the rc file'
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[706] | 204 |
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[513] | 205 | fname = _asap_fname()
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[706] | 206 |
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[226] | 207 | if fname is None or not os.path.exists(fname):
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| 208 | message = 'could not find rc file; returning defaults'
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| 209 | ret = dict([ (key, tup[0]) for key, tup in defaultParams.items()])
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| 210 | #print message
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| 211 | return ret
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[706] | 212 |
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[226] | 213 | cnt = 0
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| 214 | for line in file(fname):
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| 215 | cnt +=1
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| 216 | line = line.strip()
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| 217 | if not len(line): continue
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| 218 | if line.startswith('#'): continue
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| 219 | tup = line.split(':',1)
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| 220 | if len(tup) !=2:
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| 221 | print ('Illegal line #%d\n\t%s\n\tin file "%s"' % (cnt, line, fname))
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| 222 | continue
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[706] | 223 |
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[226] | 224 | key, val = tup
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| 225 | key = key.strip()
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| 226 | if not defaultParams.has_key(key):
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| 227 | print ('Bad key "%s" on line %d in %s' % (key, cnt, fname))
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| 228 | continue
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[706] | 229 |
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[226] | 230 | default, converter = defaultParams[key]
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| 231 |
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| 232 | ind = val.find('#')
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| 233 | if ind>=0: val = val[:ind] # ignore trailing comments
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| 234 | val = val.strip()
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| 235 | try: cval = converter(val) # try to convert to proper type or raise
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[1080] | 236 | except ValueError, msg:
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[226] | 237 | print ('Bad val "%s" on line #%d\n\t"%s"\n\tin file "%s"\n\t%s' % (val, cnt, line, fname, msg))
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| 238 | continue
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| 239 | else:
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| 240 | # Alles Klar, update dict
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| 241 | defaultParams[key][0] = cval
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| 242 |
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| 243 | # strip the conveter funcs and return
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| 244 | ret = dict([ (key, tup[0]) for key, tup in defaultParams.items()])
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[466] | 245 | print ('loaded rc file %s'%fname)
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[226] | 246 |
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| 247 | return ret
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| 248 |
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| 249 |
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| 250 | # this is the instance used by the asap classes
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[706] | 251 | rcParams = rc_params()
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[226] | 252 |
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| 253 | rcParamsDefault = dict(rcParams.items()) # a copy
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| 254 |
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| 255 | def rc(group, **kwargs):
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| 256 | """
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| 257 | Set the current rc params. Group is the grouping for the rc, eg
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[379] | 258 | for scantable.save the group is 'scantable', for plotter.stacking, the
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| 259 | group is 'plotter', and so on. kwargs is a list of attribute
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[226] | 260 | name/value pairs, eg
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| 261 |
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[379] | 262 | rc('scantable', save='SDFITS')
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[226] | 263 |
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| 264 | sets the current rc params and is equivalent to
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[706] | 265 |
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[379] | 266 | rcParams['scantable.save'] = 'SDFITS'
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[226] | 267 |
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| 268 | Use rcdefaults to restore the default rc params after changes.
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| 269 | """
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| 270 |
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[379] | 271 | aliases = {}
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[706] | 272 |
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[226] | 273 | for k,v in kwargs.items():
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| 274 | name = aliases.get(k) or k
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[1422] | 275 | if len(group):
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| 276 | key = '%s.%s' % (group, name)
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| 277 | else:
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| 278 | key = name
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[226] | 279 | if not rcParams.has_key(key):
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| 280 | raise KeyError('Unrecognized key "%s" for group "%s" and name "%s"' % (key, group, name))
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[706] | 281 |
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[226] | 282 | rcParams[key] = v
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| 283 |
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| 284 |
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| 285 | def rcdefaults():
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| 286 | """
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| 287 | Restore the default rc params - the ones that were created at
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| 288 | asap load time
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| 289 | """
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| 290 | rcParams.update(rcParamsDefault)
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| 291 |
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[1295] | 292 | def _n_bools(n, val):
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[1588] | 293 | return [ val for i in xrange(n) ]
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[513] | 294 |
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| 295 | def _is_sequence_or_number(param, ptype=int):
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| 296 | if isinstance(param,tuple) or isinstance(param,list):
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[928] | 297 | if len(param) == 0: return True # empty list
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[513] | 298 | out = True
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| 299 | for p in param:
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| 300 | out &= isinstance(p,ptype)
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| 301 | return out
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| 302 | elif isinstance(param, ptype):
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| 303 | return True
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| 304 | return False
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| 305 |
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[928] | 306 | def _to_list(param, ptype=int):
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| 307 | if isinstance(param, ptype):
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| 308 | if ptype is str: return param.split()
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| 309 | else: return [param]
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| 310 | if _is_sequence_or_number(param, ptype):
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| 311 | return param
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| 312 | return None
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[715] | 313 |
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[944] | 314 | def unique(x):
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[992] | 315 | """
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| 316 | Return the unique values in a list
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| 317 | Parameters:
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| 318 | x: the list to reduce
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| 319 | Examples:
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| 320 | x = [1,2,3,3,4]
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| 321 | print unique(x)
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| 322 | [1,2,3,4]
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| 323 | """
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[944] | 324 | return dict([ (val, 1) for val in x]).keys()
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| 325 |
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[992] | 326 | def list_files(path=".",suffix="rpf"):
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| 327 | """
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| 328 | Return a list files readable by asap, such as rpf, sdfits, mbf, asap
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| 329 | Parameters:
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| 330 | path: The directory to list (default '.')
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| 331 | suffix: The file extension (default rpf)
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| 332 | Example:
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| 333 | files = list_files("data/","sdfits")
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| 334 | print files
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| 335 | ['data/2001-09-01_0332_P363.sdfits',
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| 336 | 'data/2003-04-04_131152_t0002.sdfits',
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| 337 | 'data/Sgr_86p262_best_SPC.sdfits']
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| 338 | """
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| 339 | if not os.path.isdir(path):
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| 340 | return None
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[1295] | 341 | valid = "rpf rpf.1 rpf.2 sdf sdfits mbf asap".split()
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[992] | 342 | if not suffix in valid:
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| 343 | return None
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| 344 | files = [os.path.expanduser(os.path.expandvars(path+"/"+f)) for f in os.listdir(path)]
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| 345 | return filter(lambda x: x.endswith(suffix),files)
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| 346 |
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[715] | 347 | # workaround for ipython, which redirects this if banner=0 in ipythonrc
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| 348 | sys.stdout = sys.__stdout__
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| 349 | sys.stderr = sys.__stderr__
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| 350 |
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| 351 | # Logging
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| 352 | from asap._asap import Log as _asaplog
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| 353 | global asaplog
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[710] | 354 | asaplog=_asaplog()
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[715] | 355 | if rcParams['verbose']:
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| 356 | asaplog.enable()
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| 357 | else:
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| 358 | asaplog.disable()
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| 359 |
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[1589] | 360 |
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| 361 | def print_log_dec(f):
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[1691] | 362 | @wraps_dec(f)
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[1589] | 363 | def wrap_it(*args, **kw):
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| 364 | val = f(*args, **kw)
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| 365 | print_log()
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| 366 | return val
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| 367 | return wrap_it
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| 368 |
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[715] | 369 | def print_log():
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[1589] | 370 | log = asaplog.pop().strip()
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[715] | 371 | if len(log) and rcParams['verbose']: print log
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| 372 | return
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| 373 |
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[1295] | 374 | def mask_and(a, b):
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| 375 | assert(len(a)==len(b))
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| 376 | return [ a[i] & b[i] for i in xrange(len(a)) ]
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[1134] | 377 |
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[1295] | 378 | def mask_or(a, b):
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| 379 | assert(len(a)==len(b))
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| 380 | return [ a[i] | b[i] for i in xrange(len(a)) ]
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| 381 |
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| 382 | def mask_not(a):
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| 383 | return [ not i for i in a ]
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| 384 |
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[1117] | 385 | from asapfitter import fitter
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[895] | 386 | from asapreader import reader
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[944] | 387 | from selector import selector
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[710] | 388 |
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[100] | 389 | from asapmath import *
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[1080] | 390 | from scantable import scantable
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[1097] | 391 | from asaplinefind import linefinder
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[1645] | 392 | from simplelinefinder import simplelinefinder
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[1134] | 393 | from linecatalog import linecatalog
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[1689] | 394 | from opacity import skydip
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[1725] | 395 | from opacity import model as opacity_model
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[285] | 396 |
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[928] | 397 | if rcParams['useplotter']:
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[1295] | 398 | try:
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[1423] | 399 | from asapplotter import asapplotter
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| 400 | gui = os.environ.has_key('DISPLAY') and rcParams['plotter.gui']
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| 401 | if gui:
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[1422] | 402 | import matplotlib
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| 403 | matplotlib.use("TkAgg")
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[1691] | 404 | from matplotlib import pylab
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[1422] | 405 | xyplotter = pylab
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[1423] | 406 | plotter = asapplotter(gui)
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| 407 | del gui
|
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[1295] | 408 | except ImportError:
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[1423] | 409 | print "Matplotlib not installed. No plotting available"
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[285] | 410 |
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[574] | 411 | __date__ = '$Date: 2010-04-27 05:48:24 +0000 (Tue, 27 Apr 2010) $'.split()[1]
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[1560] | 412 | __version__ = '$Revision: 1725 $'
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[100] | 413 |
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[1193] | 414 | def is_ipython():
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[1725] | 415 | return 'IPython' in sys.modules.keys()
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[1589] | 416 |
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[1193] | 417 | if is_ipython():
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[1014] | 418 | def version(): print "ASAP %s(%s)"% (__version__, __date__)
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[1588] | 419 |
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| 420 | def list_scans(t = scantable):
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[1560] | 421 | import inspect
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| 422 | print "The user created scantables are: ",
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| 423 | globs=inspect.currentframe().f_back.f_locals.copy()
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| 424 | out = [ k for k,v in globs.iteritems() \
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| 425 | if isinstance(v, scantable) and not k.startswith("_") ]
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| 426 | print out
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| 427 | return out
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[100] | 428 |
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[715] | 429 | def commands():
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| 430 | x = """
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[113] | 431 | [The scan container]
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| 432 | scantable - a container for integrations/scans
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[182] | 433 | (can open asap/rpfits/sdfits and ms files)
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[113] | 434 | copy - returns a copy of a scan
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| 435 | get_scan - gets a specific scan out of a scantable
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[984] | 436 | (by name or number)
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[1093] | 437 | drop_scan - drops a specific scan out of a scantable
|
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| 438 | (by number)
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[984] | 439 | set_selection - set a new subselection of the data
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| 440 | get_selection - get the current selection object
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[113] | 441 | summary - print info about the scantable contents
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[182] | 442 | stats - get specified statistic of the spectra in
|
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| 443 | the scantable
|
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| 444 | stddev - get the standard deviation of the spectra
|
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| 445 | in the scantable
|
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[113] | 446 | get_tsys - get the TSys
|
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| 447 | get_time - get the timestamps of the integrations
|
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[1351] | 448 | get_inttime - get the integration time
|
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[733] | 449 | get_sourcename - get the source names of the scans
|
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[794] | 450 | get_azimuth - get the azimuth of the scans
|
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| 451 | get_elevation - get the elevation of the scans
|
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| 452 | get_parangle - get the parallactic angle of the scans
|
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[1697] | 453 | get_coordinate - get the spectral coordinate for the given row,
|
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| 454 | which can be used for coordinate conversions
|
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[876] | 455 | get_unit - get the current unit
|
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[513] | 456 | set_unit - set the abcissa unit to be used from this
|
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| 457 | point on
|
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[255] | 458 | get_abcissa - get the abcissa values and name for a given
|
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| 459 | row (time)
|
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[1259] | 460 | get_column_names - get the names of the columns in the scantable
|
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| 461 | for use with selector.set_query
|
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[113] | 462 | set_freqframe - set the frame info for the Spectral Axis
|
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| 463 | (e.g. 'LSRK')
|
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[276] | 464 | set_doppler - set the doppler to be used from this point on
|
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[984] | 465 | set_dirframe - set the frame for the direction on the sky
|
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[240] | 466 | set_instrument - set the instrument name
|
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[1190] | 467 | set_feedtype - set the feed type
|
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[255] | 468 | get_fluxunit - get the brightness flux unit
|
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[240] | 469 | set_fluxunit - set the brightness flux unit
|
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[1508] | 470 | set_sourcetype - set the type of the source - source or reference
|
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[188] | 471 | create_mask - return an mask in the current unit
|
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| 472 | for the given region. The specified regions
|
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| 473 | are NOT masked
|
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[255] | 474 | get_restfreqs - get the current list of rest frequencies
|
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| 475 | set_restfreqs - set a list of rest frequencies
|
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[1471] | 476 | shift_refpix - shift the reference pixel of the IFs
|
---|
| 477 | set_spectrum - overwrite the spectrum for a given row
|
---|
| 478 | get_spectrum - retrieve the spectrum for a given
|
---|
| 479 | get_mask - retrieve the mask for a given
|
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[1012] | 480 | flag - flag selected channels in the data
|
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[1192] | 481 | lag_flag - flag specified frequency in the data
|
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[1151] | 482 | save - save the scantable to disk as either 'ASAP',
|
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| 483 | 'SDFITS' or 'ASCII'
|
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[486] | 484 | nbeam,nif,nchan,npol - the number of beams/IFs/Pols/Chans
|
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[733] | 485 | nscan - the number of scans in the scantable
|
---|
[1422] | 486 | nrow - the number of spectra in the scantable
|
---|
[486] | 487 | history - print the history of the scantable
|
---|
[530] | 488 | get_fit - get a fit which has been stored witnh the data
|
---|
[706] | 489 | average_time - return the (weighted) time average of a scan
|
---|
[513] | 490 | or a list of scans
|
---|
| 491 | average_pol - average the polarisations together.
|
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[1144] | 492 | average_beam - average the beams together.
|
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[992] | 493 | convert_pol - convert to a different polarisation type
|
---|
[690] | 494 | auto_quotient - return the on/off quotient with
|
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[1069] | 495 | automatic detection of the on/off scans (closest
|
---|
| 496 | in time off is selected)
|
---|
[1144] | 497 | mx_quotient - Form a quotient using MX data (off beams)
|
---|
[1014] | 498 | scale, *, / - return a scan scaled by a given factor
|
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[1560] | 499 | add, + - return a scan with given value added
|
---|
| 500 | sub, - - return a scan with given value subtracted
|
---|
[513] | 501 | bin - return a scan with binned channels
|
---|
| 502 | resample - return a scan with resampled channels
|
---|
| 503 | smooth - return the spectrally smoothed scan
|
---|
| 504 | poly_baseline - fit a polynomial baseline to all Beams/IFs/Pols
|
---|
[706] | 505 | auto_poly_baseline - automatically fit a polynomial baseline
|
---|
[780] | 506 | recalc_azel - recalculate azimuth and elevation based on
|
---|
| 507 | the pointing
|
---|
[513] | 508 | gain_el - apply gain-elevation correction
|
---|
| 509 | opacity - apply opacity correction
|
---|
| 510 | convert_flux - convert to and from Jy and Kelvin brightness
|
---|
[255] | 511 | units
|
---|
[513] | 512 | freq_align - align spectra in frequency frame
|
---|
[1014] | 513 | invert_phase - Invert the phase of the cross-correlation
|
---|
[1351] | 514 | swap_linears - Swap XX and YY (or RR LL)
|
---|
[513] | 515 | rotate_xyphase - rotate XY phase of cross correlation
|
---|
| 516 | rotate_linpolphase - rotate the phase of the complex
|
---|
| 517 | polarization O=Q+iU correlation
|
---|
[733] | 518 | freq_switch - perform frequency switching on the data
|
---|
| 519 | stats - Determine the specified statistic, e.g. 'min'
|
---|
| 520 | 'max', 'rms' etc.
|
---|
| 521 | stddev - Determine the standard deviation of the current
|
---|
| 522 | beam/if/pol
|
---|
[1588] | 523 | get_row_selector - get the selection object for a specified row
|
---|
| 524 | number
|
---|
[1014] | 525 | [Selection]
|
---|
| 526 | selector - a selection object to set a subset of a scantable
|
---|
| 527 | set_scans - set (a list of) scans by index
|
---|
| 528 | set_cycles - set (a list of) cycles by index
|
---|
| 529 | set_beams - set (a list of) beamss by index
|
---|
| 530 | set_ifs - set (a list of) ifs by index
|
---|
| 531 | set_polarisations - set (a list of) polarisations by name
|
---|
| 532 | or by index
|
---|
| 533 | set_names - set a selection by name (wildcards allowed)
|
---|
| 534 | set_tsys - set a selection by tsys thresholds
|
---|
[1259] | 535 | set_query - set a selection by SQL-like query, e.g. BEAMNO==1
|
---|
[1351] | 536 | ( also get_ functions for all these )
|
---|
[1014] | 537 | reset - unset all selections
|
---|
[1351] | 538 | + - merge two selections
|
---|
[733] | 539 |
|
---|
[513] | 540 | [Math] Mainly functions which operate on more than one scantable
|
---|
[100] | 541 |
|
---|
[706] | 542 | average_time - return the (weighted) time average
|
---|
[513] | 543 | of a list of scans
|
---|
| 544 | quotient - return the on/off quotient
|
---|
| 545 | simple_math - simple mathematical operations on two scantables,
|
---|
| 546 | 'add', 'sub', 'mul', 'div'
|
---|
[1069] | 547 | quotient - build quotient of the given on and off scans
|
---|
[1351] | 548 | (matched pairs and 1 off - n on are valid)
|
---|
[1117] | 549 | merge - merge a list of scantables
|
---|
[1069] | 550 |
|
---|
[1151] | 551 | [Line Catalog]
|
---|
| 552 | linecatalog - a linecatalog wrapper, taking an ASCII or
|
---|
| 553 | internal format table
|
---|
| 554 | summary - print a summary of the current selection
|
---|
| 555 | set_name - select a subset by name pattern, e.g. '*OH*'
|
---|
| 556 | set_strength_limits - select a subset by line strength limits
|
---|
| 557 | set_frequency_limits - select a subset by frequency limits
|
---|
| 558 | reset - unset all selections
|
---|
| 559 | save - save the current subset to a table (internal
|
---|
| 560 | format)
|
---|
| 561 | get_row - get the name and frequency from a specific
|
---|
| 562 | row in the table
|
---|
[513] | 563 | [Fitting]
|
---|
[113] | 564 | fitter
|
---|
| 565 | auto_fit - return a scan where the function is
|
---|
| 566 | applied to all Beams/IFs/Pols.
|
---|
| 567 | commit - return a new scan where the fits have been
|
---|
| 568 | commited.
|
---|
| 569 | fit - execute the actual fitting process
|
---|
[984] | 570 | store_fit - store the fit parameters in the data (scantable)
|
---|
[113] | 571 | get_chi2 - get the Chi^2
|
---|
| 572 | set_scan - set the scantable to be fit
|
---|
| 573 | set_function - set the fitting function
|
---|
| 574 | set_parameters - set the parameters for the function(s), and
|
---|
| 575 | set if they should be held fixed during fitting
|
---|
[513] | 576 | set_gauss_parameters - same as above but specialised for individual
|
---|
| 577 | gaussian components
|
---|
[113] | 578 | get_parameters - get the fitted parameters
|
---|
[513] | 579 | plot - plot the resulting fit and/or components and
|
---|
| 580 | residual
|
---|
[210] | 581 | [Plotter]
|
---|
| 582 | asapplotter - a plotter for asap, default plotter is
|
---|
| 583 | called 'plotter'
|
---|
[984] | 584 | plot - plot a scantable
|
---|
[1151] | 585 | plot_lines - plot a linecatalog overlay
|
---|
[1697] | 586 | plotazel - plot azimuth and elevation versus time
|
---|
| 587 | plotpointing - plot telescope pointings
|
---|
[378] | 588 | save - save the plot to a file ('png' ,'ps' or 'eps')
|
---|
[210] | 589 | set_mode - set the state of the plotter, i.e.
|
---|
| 590 | what is to be plotted 'colour stacked'
|
---|
| 591 | and what 'panelled'
|
---|
[984] | 592 | set_selection - only plot a selected part of the data
|
---|
[733] | 593 | set_range - set a 'zoom' window [xmin,xmax,ymin,ymax]
|
---|
[255] | 594 | set_legend - specify user labels for the legend indeces
|
---|
| 595 | set_title - specify user labels for the panel indeces
|
---|
[733] | 596 | set_abcissa - specify a user label for the abcissa
|
---|
[255] | 597 | set_ordinate - specify a user label for the ordinate
|
---|
[378] | 598 | set_layout - specify the multi-panel layout (rows,cols)
|
---|
[733] | 599 | set_colors - specify a set of colours to use
|
---|
| 600 | set_linestyles - specify a set of linestyles to use if only
|
---|
| 601 | using one color
|
---|
[1151] | 602 | set_font - set general font properties, e.g. 'family'
|
---|
[1054] | 603 | set_histogram - plot in historam style
|
---|
[733] | 604 | set_mask - set a plotting mask for a specific polarization
|
---|
[1171] | 605 | text - draw text annotations either in data or relative
|
---|
| 606 | coordinates
|
---|
| 607 | arrow - draw arrow annotations either in data or relative
|
---|
| 608 | coordinates
|
---|
| 609 | axhline,axvline - draw horizontal/vertical lines
|
---|
| 610 | axhspan,axvspan - draw horizontal/vertical regions
|
---|
[1560] | 611 | annotate - draw an arrow with label
|
---|
| 612 | create_mask - create a scnatble mask interactively
|
---|
[1175] | 613 |
|
---|
| 614 | xyplotter - matplotlib/pylab plotting functions
|
---|
| 615 |
|
---|
[113] | 616 | [General]
|
---|
| 617 | commands - this command
|
---|
| 618 | print - print details about a variable
|
---|
[1560] | 619 | list_scans - list all scantables created by the user
|
---|
[992] | 620 | list_files - list all files readable by asap (default rpf)
|
---|
[113] | 621 | del - delete the given variable from memory
|
---|
| 622 | range - create a list of values, e.g.
|
---|
| 623 | range(3) = [0,1,2], range(2,5) = [2,3,4]
|
---|
| 624 | help - print help for one of the listed functions
|
---|
| 625 | execfile - execute an asap script, e.g. execfile('myscript')
|
---|
[255] | 626 | list_rcparameters - print out a list of possible values to be
|
---|
[274] | 627 | put into $HOME/.asaprc
|
---|
[1171] | 628 | rc - set rc parameters from within asap
|
---|
[466] | 629 | mask_and,mask_or,
|
---|
| 630 | mask_not - boolean operations on masks created with
|
---|
| 631 | scantable.create_mask
|
---|
[1697] | 632 | skydip - gain opacity values from a sky dip observation
|
---|
[1725] | 633 | opacity_model - compute opacities fro given frequencies based on
|
---|
| 634 | atmospheric model
|
---|
[706] | 635 |
|
---|
[210] | 636 | Note:
|
---|
| 637 | How to use this with help:
|
---|
| 638 | # function 'summary'
|
---|
| 639 | [xxx] is just a category
|
---|
| 640 | Every 'sub-level' in this list should be replaces by a '.' Period when
|
---|
[706] | 641 | using help
|
---|
[210] | 642 | Example:
|
---|
| 643 | ASAP> help scantable # to get info on ths scantable
|
---|
| 644 | ASAP> help scantable.summary # to get help on the scantable's
|
---|
| 645 | ASAP> help average_time
|
---|
| 646 |
|
---|
[715] | 647 | """
|
---|
[1151] | 648 | if rcParams['verbose']:
|
---|
| 649 | try:
|
---|
| 650 | from IPython.genutils import page as pager
|
---|
| 651 | except ImportError:
|
---|
| 652 | from pydoc import pager
|
---|
| 653 | pager(x)
|
---|
| 654 | else:
|
---|
| 655 | print x
|
---|
[715] | 656 | return
|
---|
[113] | 657 |
|
---|
[706] | 658 | def welcome():
|
---|
| 659 | return """Welcome to ASAP v%s (%s) - the ATNF Spectral Analysis Package
|
---|
[100] | 660 |
|
---|
[1035] | 661 | Please report any bugs via:
|
---|
[1378] | 662 | http://svn.atnf.csiro.au/trac/asap/simpleticket
|
---|
[100] | 663 |
|
---|
[378] | 664 | [IMPORTANT: ASAP is 0-based]
|
---|
[706] | 665 | Type commands() to get a list of all available ASAP commands.""" % (__version__, __date__)
|
---|