| 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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| 5 | import os,sys
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| 6 | 
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| 7 | def validate_bool(b):
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| 8 |     'Convert b to a boolean or raise'
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| 9 |     bl = b.lower()
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| 10 |     if bl in ('f', 'no', 'false', '0', 0): return False
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| 11 |     elif bl in ('t', 'yes', 'true', '1', 1): return True
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| 12 |     else:
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| 13 |         raise ValueError('Could not convert "%s" to boolean' % b)
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| 14 | 
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| 15 | def validate_int(s):
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| 16 |     'convert s to int or raise'
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| 17 |     try: return int(s)
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| 18 |     except ValueError:
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| 19 |         raise ValueError('Could not convert "%s" to int' % s)
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| 20 | 
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| 21 | def asap_fname():
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| 22 |     """
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| 23 |     Return the path to the rc file
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| 24 | 
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| 25 |     Search order:
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| 26 | 
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| 27 |      * current working dir
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| 28 |      * environ var ASAPRC
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| 29 |      * HOME/.matplotlibrc
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| 30 |      
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| 31 |     """
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| 32 | 
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| 33 |     fname = os.path.join( os.getcwd(), '.asaprc')
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| 34 |     if os.path.exists(fname): return fname
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| 35 | 
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| 36 |     if os.environ.has_key('ASAPRC'):
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| 37 |         path =  os.environ['ASAPRC']
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| 38 |         if os.path.exists(path):
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| 39 |             fname = os.path.join(path, '.asaprc')
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| 40 |             if os.path.exists(fname):
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| 41 |                 return fname
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| 42 | 
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| 43 |     if os.environ.has_key('HOME'):
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| 44 |         home =  os.environ['HOME']
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| 45 |         fname = os.path.join(home, '.asaprc')
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| 46 |         if os.path.exists(fname):
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| 47 |             return fname
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| 48 |     return None
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| 49 |         
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| 50 | 
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| 51 | defaultParams = {
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| 52 |     # general
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| 53 |     'verbose'             : [True, validate_bool],
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| 54 |     'useplotter'          : [True, validate_bool],
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| 55 | 
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| 56 |     # plotting
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| 57 |     'plotter.stacking'    : ['p', str],
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| 58 |     'plotter.panelling'   : ['s', str],
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| 59 | 
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| 60 |     # scantable
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| 61 |     'scantable.save'      : ['ASAP', str],
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| 62 |     'scantable.autoaverage'      : [True, validate_bool],
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| 63 |     'scantable.freqframe' : ['LSRK', str],  #default frequency frame
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| 64 |     'scantable.allaxes'   : [True, validate_bool],  # apply action to all axes
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| 65 |     'scantable.plotter'   : [True, validate_bool], # use internal plotter
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| 66 | 
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| 67 |     # math
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| 68 |     'math.insitu'         : [False, validate_bool],
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| 69 | 
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| 70 |     # fitter
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| 71 |     'fitter.polyorder'    : [0, validate_int],
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| 72 |     'fitter.ncomponents'  : [1, validate_int]
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| 73 |     }
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| 74 | 
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| 75 | def rc_params():
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| 76 |     'Return the default params updated from the values in the rc file'
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| 77 |     
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| 78 |     fname = asap_fname()
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| 79 |     
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| 80 |     if fname is None or not os.path.exists(fname):
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| 81 |         message = 'could not find rc file; returning defaults'
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| 82 |         ret =  dict([ (key, tup[0]) for key, tup in defaultParams.items()])
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| 83 |         #print message
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| 84 |         return ret
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| 85 |         
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| 86 |     cnt = 0
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| 87 |     for line in file(fname):
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| 88 |         cnt +=1
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| 89 |         line = line.strip()
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| 90 |         if not len(line): continue
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| 91 |         if line.startswith('#'): continue
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| 92 |         tup = line.split(':',1)
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| 93 |         if len(tup) !=2:
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| 94 |             print ('Illegal line #%d\n\t%s\n\tin file "%s"' % (cnt, line, fname))
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| 95 |             continue
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| 96 |         
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| 97 |         key, val = tup
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| 98 |         key = key.strip()
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| 99 |         if not defaultParams.has_key(key):
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| 100 |             print ('Bad key "%s" on line %d in %s' % (key, cnt, fname))
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| 101 |             continue
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| 102 |         
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| 103 |         default, converter =  defaultParams[key]
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| 104 | 
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| 105 |         ind = val.find('#')
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| 106 |         if ind>=0: val = val[:ind]   # ignore trailing comments
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| 107 |         val = val.strip()
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| 108 |         try: cval = converter(val)   # try to convert to proper type or raise
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| 109 |         except Exception, msg:
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| 110 |             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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| 111 |             continue
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| 112 |         else:
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| 113 |             # Alles Klar, update dict
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| 114 |             defaultParams[key][0] = cval
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| 115 | 
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| 116 |     # strip the conveter funcs and return
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| 117 |     ret =  dict([ (key, tup[0]) for key, tup in defaultParams.items()])
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| 118 |     verbose.report('loaded rc file %s'%fname)
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| 119 | 
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| 120 |     return ret
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| 121 | 
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| 122 | 
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| 123 | # this is the instance used by the asap classes
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| 124 | rcParams = rc_params() 
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| 125 | 
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| 126 | rcParamsDefault = dict(rcParams.items()) # a copy
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| 127 | 
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| 128 | def rc(group, **kwargs):
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| 129 |     """
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| 130 |     Set the current rc params.  Group is the grouping for the rc, eg
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| 131 |     for lines.linewidth the group is 'lines', for axes.facecolor, the
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| 132 |     group is 'axes', and so on.  kwargs is a list of attribute
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| 133 |     name/value pairs, eg
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| 134 | 
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| 135 |       rc('lines', linewidth=2, color='r')
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| 136 | 
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| 137 |     sets the current rc params and is equivalent to
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| 138 |     
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| 139 |       rcParams['lines.linewidth'] = 2
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| 140 |       rcParams['lines.color'] = 'r'
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| 141 | 
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| 142 | 
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| 143 |     Note you can use python's kwargs dictionary facility to store
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| 144 |     dictionaries of default parameters.  Eg, you can customize the
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| 145 |     font rc as follows
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| 146 | 
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| 147 |       font = {'family' : 'monospace',
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| 148 |               'weight' : 'bold',
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| 149 |               'size'   : 'larger',
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| 150 |              }
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| 151 | 
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| 152 |       rc('font', **font)  # pass in the font dict as kwargs
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| 153 | 
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| 154 |     This enables you to easily switch between several configurations.
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| 155 |     Use rcdefaults to restore the default rc params after changes.
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| 156 |     """
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| 157 | 
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| 158 |     aliases = {
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| 159 |         }
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| 160 |     
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| 161 |     for k,v in kwargs.items():
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| 162 |         name = aliases.get(k) or k
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| 163 |         key = '%s.%s' % (group, name)
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| 164 |         if not rcParams.has_key(key):
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| 165 |             raise KeyError('Unrecognized key "%s" for group "%s" and name "%s"' % (key, group, name))
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| 166 |         
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| 167 |         rcParams[key] = v
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| 168 | 
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| 169 | 
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| 170 | def rcdefaults():
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| 171 |     """
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| 172 |     Restore the default rc params - the ones that were created at
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| 173 |     asap load time
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| 174 |     """
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| 175 |     rcParams.update(rcParamsDefault)
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| 176 | 
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| 177 | from asapfitter import *
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| 178 | from asapreader import reader
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| 179 | from asapmath import *
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| 180 | from scantable import *
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| 181 | if rcParams['useplotter']:
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| 182 |     print "Initialising plotter..."
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| 183 |     from asapplotter import *
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| 184 |     plotter = asapplotter()
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| 185 | #from numarray ones,zeros
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| 186 | 
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| 187 | __date__ = '$Date: 2005-01-21 01:28:57 +0000 (Fri, 21 Jan 2005) $'
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| 188 | __version__  = '0.1a'
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| 189 | 
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| 190 | def list_scans(t = scantable):
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| 191 |     import sys, types
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| 192 |     #meta_t = type(t)
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| 193 |     #if meta_t == types.InstanceType:
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| 194 |     #    t = t.__class__
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| 195 |     #elif meta_t not in [types.ClassType, types.TypeType]:
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| 196 |     #    t = meta_t
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| 197 |     globs = sys.modules['__main__'].__dict__.iteritems()
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| 198 |     print "The user created scantables are:"
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| 199 |     x = map(lambda x: x[0], filter(lambda x: isinstance(x[1], t), globs))
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| 200 |     print x
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| 201 | 
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| 202 | def commands():
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| 203 |     x = """    
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| 204 |     [The scan container]
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| 205 |         scantable           - a container for integrations/scans
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| 206 |                               (can open asap/rpfits/sdfits and ms files)
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| 207 |             copy            - returns a copy of a scan
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| 208 |             get_scan        - gets a specific scan out of a scantable
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| 209 |             summary         - print info about the scantable contents
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| 210 |             set_selection   - set a specific Beam/IF/Pol for furthrt use
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| 211 |             get_selection   - print out the current selection
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| 212 |             stats           - get specified statistic of the spectra in
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| 213 |                               the scantable
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| 214 |             stddev          - get the standard deviation of the spectra
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| 215 |                               in the scantable
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| 216 |             get_tsys        - get the TSys
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| 217 |             get_time        - get the timestamps of the integrations
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| 218 |             set_unit        - set the units to be used from this point on
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| 219 |             set_freqframe   - set the frame info for the Spectral Axis
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| 220 |                               (e.g. 'LSRK')
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| 221 |             set_instrument  - set the instrument name
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| 222 |             set_fluxunit    - set the brightness flux unit
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| 223 |             create_mask     - return an mask in the current unit
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| 224 |                               for the given region. The specified regions
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| 225 |                               are NOT masked
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| 226 |             set_restfreqs   - give a list of rest frequencies
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| 227 |             flag_spectrum   - flag a whole Beam/IF/Pol
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| 228 |             save            - save the scantable to disk as either 'ASAP'
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| 229 |                               or 'SDFITS'
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| 230 |             nbeam,nif,nchan,npol - the number of beams/IFs/Pols/Chans 
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| 231 |     [Math]
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| 232 |         average_time       - return the (weighted) time average of a scan 
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| 233 |                              or a list of scans
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| 234 |         average_pol         - average the polarisations together.
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| 235 |                               The dimension won't be reduced and
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| 236 |                               all polarisations will contain the
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| 237 |                               averaged spectrum.
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| 238 |         quotient            - return the on/off quotient
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| 239 |         b_operate           - simple mathematical operations on two scan tables
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| 240 |         scale               - returns a scan scaled by a given factor
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| 241 |         add                 - returns a scan with given value added 
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| 242 |         bin                 - return a scan with binned channels
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| 243 |         smooth              - return the spectrally smoothed scan
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| 244 |         poly_baseline       - fit a polynomial baseline to all Beams/IFs/Pols
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| 245 |         gain_el             - apply gain-elevation correction
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| 246 |         opacity             - apply opacity correction
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| 247 |         convert_flux        - convert to and from Jy and Kelvin brightness units
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| 248 | 
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| 249 |         fitter
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| 250 |             auto_fit        - return a scan where the function is
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| 251 |                               applied to all Beams/IFs/Pols.
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| 252 |             commit          - return a new scan where the fits have been
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| 253 |                               commited.
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| 254 |             fit             - execute the actual fitting process
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| 255 |             get_chi2        - get the Chi^2
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| 256 |             set_scan        - set the scantable to be fit
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| 257 |             set_function    - set the fitting function
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| 258 |             set_parameters  - set the parameters for the function(s), and
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| 259 |                               set if they should be held fixed during fitting
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| 260 |             get_parameters  - get the fitted parameters
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| 261 |     [Plotter]
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| 262 |         asapplotter         - a plotter for asap, default plotter is
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| 263 |                               called 'plotter'
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| 264 |             plot            - plot a (list of) scantable
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| 265 |             set_mode        - set the state of the plotter, i.e.
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| 266 |                               what is to be plotted 'colour stacked'
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| 267 |                               and what 'panelled'
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| 268 |             set_range       - set the abcissa 'zoom' range
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| 269 |             set_legend_map  - specify user labels for the legend indeces
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| 270 |             
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| 271 |     [Reading files]
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| 272 |         reader              - access rpfits/sdfits files
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| 273 |             read            - read in integrations
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| 274 |             summary         - list info about all integrations
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| 275 | 
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| 276 |     [General]
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| 277 |         commands            - this command
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| 278 |         print               - print details about a variable
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| 279 |         list_scans          - list all scantables created bt the user
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| 280 |         del                 - delete the given variable from memory
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| 281 |         range               - create a list of values, e.g.
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| 282 |                               range(3) = [0,1,2], range(2,5) = [2,3,4]
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| 283 |         help                - print help for one of the listed functions
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| 284 |         execfile            - execute an asap script, e.g. execfile('myscript')
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| 285 |     Note:
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| 286 |         How to use this with help:
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| 287 |                                          # function 'summary'
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| 288 |         [xxx] is just a category
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| 289 |         Every 'sub-level' in this list should be replaces by a '.' Period when
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| 290 |         using help 
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| 291 |         Example:
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| 292 |             ASAP> help scantable # to get info on ths scantable
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| 293 |             ASAP> help scantable.summary # to get help on the scantable's
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| 294 |             ASAP> help average_time
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| 295 | 
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| 296 |     """
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| 297 |     print x
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| 298 |     return
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| 299 | 
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| 300 | print """Welcome to ASAP - the ATNF Single Dish Analysis Package
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| 301 | This is a testing pre-release v0.1a
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| 302 | 
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| 303 | Please report any bugs to:
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| 304 | Malte.Marquarding@csiro.au
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| 305 | 
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| 306 | [NOTE: ASAP is 0-based]
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| 307 | Type commands() to get a list of all available ASAP commands.
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| 308 | """
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