source: trunk/python/__init__.py@ 240

Last change on this file since 240 was 240, checked in by kil064, 20 years ago

add set_instrument

set_fluxunit
b_operate
gain_el
opacity
convert_flux

  • Property svn:eol-style set to native
  • Property svn:keywords set to Author Date Id Revision
File size: 10.8 KB
Line 
1"""
2This is the ATNF Single Dish Analysis package.
3
4"""
5import os,sys
6
7def validate_bool(b):
8 'Convert b to a boolean or raise'
9 bl = b.lower()
10 if bl in ('f', 'no', 'false', '0', 0): return False
11 elif bl in ('t', 'yes', 'true', '1', 1): return True
12 else:
13 raise ValueError('Could not convert "%s" to boolean' % b)
14
15def validate_int(s):
16 'convert s to int or raise'
17 try: return int(s)
18 except ValueError:
19 raise ValueError('Could not convert "%s" to int' % s)
20
21def asap_fname():
22 """
23 Return the path to the rc file
24
25 Search order:
26
27 * current working dir
28 * environ var ASAPRC
29 * HOME/.matplotlibrc
30
31 """
32
33 fname = os.path.join( os.getcwd(), '.asaprc')
34 if os.path.exists(fname): return fname
35
36 if os.environ.has_key('ASAPRC'):
37 path = os.environ['ASAPRC']
38 if os.path.exists(path):
39 fname = os.path.join(path, '.asaprc')
40 if os.path.exists(fname):
41 return fname
42
43 if os.environ.has_key('HOME'):
44 home = os.environ['HOME']
45 fname = os.path.join(home, '.asaprc')
46 if os.path.exists(fname):
47 return fname
48 return None
49
50
51defaultParams = {
52 # general
53 'verbose' : [True, validate_bool],
54 'useplotter' : [True, validate_bool],
55
56 # plotting
57 'plotter.stacking' : ['p', str],
58 'plotter.panelling' : ['s', str],
59
60 # scantable
61 'scantable.save' : ['ASAP', str],
62 'scantable.autoaverage' : [True, validate_bool],
63 'scantable.freqframe' : ['LSRK', str], #default frequency frame
64 'scantable.allaxes' : [True, validate_bool], # apply action to all axes
65 'scantable.plotter' : [True, validate_bool], # use internal plotter
66
67 # math
68 'math.insitu' : [False, validate_bool],
69
70 # fitter
71 'fitter.polyorder' : [0, validate_int],
72 'fitter.ncomponents' : [1, validate_int]
73 }
74
75def rc_params():
76 'Return the default params updated from the values in the rc file'
77
78 fname = asap_fname()
79
80 if fname is None or not os.path.exists(fname):
81 message = 'could not find rc file; returning defaults'
82 ret = dict([ (key, tup[0]) for key, tup in defaultParams.items()])
83 #print message
84 return ret
85
86 cnt = 0
87 for line in file(fname):
88 cnt +=1
89 line = line.strip()
90 if not len(line): continue
91 if line.startswith('#'): continue
92 tup = line.split(':',1)
93 if len(tup) !=2:
94 print ('Illegal line #%d\n\t%s\n\tin file "%s"' % (cnt, line, fname))
95 continue
96
97 key, val = tup
98 key = key.strip()
99 if not defaultParams.has_key(key):
100 print ('Bad key "%s" on line %d in %s' % (key, cnt, fname))
101 continue
102
103 default, converter = defaultParams[key]
104
105 ind = val.find('#')
106 if ind>=0: val = val[:ind] # ignore trailing comments
107 val = val.strip()
108 try: cval = converter(val) # try to convert to proper type or raise
109 except Exception, msg:
110 print ('Bad val "%s" on line #%d\n\t"%s"\n\tin file "%s"\n\t%s' % (val, cnt, line, fname, msg))
111 continue
112 else:
113 # Alles Klar, update dict
114 defaultParams[key][0] = cval
115
116 # strip the conveter funcs and return
117 ret = dict([ (key, tup[0]) for key, tup in defaultParams.items()])
118 verbose.report('loaded rc file %s'%fname)
119
120 return ret
121
122
123# this is the instance used by the asap classes
124rcParams = rc_params()
125
126rcParamsDefault = dict(rcParams.items()) # a copy
127
128def rc(group, **kwargs):
129 """
130 Set the current rc params. Group is the grouping for the rc, eg
131 for lines.linewidth the group is 'lines', for axes.facecolor, the
132 group is 'axes', and so on. kwargs is a list of attribute
133 name/value pairs, eg
134
135 rc('lines', linewidth=2, color='r')
136
137 sets the current rc params and is equivalent to
138
139 rcParams['lines.linewidth'] = 2
140 rcParams['lines.color'] = 'r'
141
142
143 Note you can use python's kwargs dictionary facility to store
144 dictionaries of default parameters. Eg, you can customize the
145 font rc as follows
146
147 font = {'family' : 'monospace',
148 'weight' : 'bold',
149 'size' : 'larger',
150 }
151
152 rc('font', **font) # pass in the font dict as kwargs
153
154 This enables you to easily switch between several configurations.
155 Use rcdefaults to restore the default rc params after changes.
156 """
157
158 aliases = {
159 }
160
161 for k,v in kwargs.items():
162 name = aliases.get(k) or k
163 key = '%s.%s' % (group, name)
164 if not rcParams.has_key(key):
165 raise KeyError('Unrecognized key "%s" for group "%s" and name "%s"' % (key, group, name))
166
167 rcParams[key] = v
168
169
170def rcdefaults():
171 """
172 Restore the default rc params - the ones that were created at
173 asap load time
174 """
175 rcParams.update(rcParamsDefault)
176
177from asapfitter import *
178from asapreader import reader
179from asapmath import *
180from scantable import *
181if rcParams['useplotter']:
182 print "Initialising plotter..."
183 from asapplotter import *
184 plotter = asapplotter()
185#from numarray ones,zeros
186
187__date__ = '$Date: 2005-01-21 01:28:57 +0000 (Fri, 21 Jan 2005) $'
188__version__ = '0.1a'
189
190def list_scans(t = scantable):
191 import sys, types
192 #meta_t = type(t)
193 #if meta_t == types.InstanceType:
194 # t = t.__class__
195 #elif meta_t not in [types.ClassType, types.TypeType]:
196 # t = meta_t
197 globs = sys.modules['__main__'].__dict__.iteritems()
198 print "The user created scantables are:"
199 x = map(lambda x: x[0], filter(lambda x: isinstance(x[1], t), globs))
200 print x
201
202def commands():
203 x = """
204 [The scan container]
205 scantable - a container for integrations/scans
206 (can open asap/rpfits/sdfits and ms files)
207 copy - returns a copy of a scan
208 get_scan - gets a specific scan out of a scantable
209 summary - print info about the scantable contents
210 set_selection - set a specific Beam/IF/Pol for furthrt use
211 get_selection - print out the current selection
212 stats - get specified statistic of the spectra in
213 the scantable
214 stddev - get the standard deviation of the spectra
215 in the scantable
216 get_tsys - get the TSys
217 get_time - get the timestamps of the integrations
218 set_unit - set the units to be used from this point on
219 set_freqframe - set the frame info for the Spectral Axis
220 (e.g. 'LSRK')
221 set_instrument - set the instrument name
222 set_fluxunit - set the brightness flux unit
223 create_mask - return an mask in the current unit
224 for the given region. The specified regions
225 are NOT masked
226 set_restfreqs - give a list of rest frequencies
227 flag_spectrum - flag a whole Beam/IF/Pol
228 save - save the scantable to disk as either 'ASAP'
229 or 'SDFITS'
230 nbeam,nif,nchan,npol - the number of beams/IFs/Pols/Chans
231 [Math]
232 average_time - return the (weighted) time average of a scan
233 or a list of scans
234 average_pol - average the polarisations together.
235 The dimension won't be reduced and
236 all polarisations will contain the
237 averaged spectrum.
238 quotient - return the on/off quotient
239 b_operate - simple mathematical operations on two scan tables
240 scale - returns a scan scaled by a given factor
241 add - returns a scan with given value added
242 bin - return a scan with binned channels
243 smooth - return the spectrally smoothed scan
244 poly_baseline - fit a polynomial baseline to all Beams/IFs/Pols
245 gain_el - apply gain-elevation correction
246 opacity - apply opacity correction
247 convert_flux - convert to and from Jy and Kelvin brightness units
248
249 fitter
250 auto_fit - return a scan where the function is
251 applied to all Beams/IFs/Pols.
252 commit - return a new scan where the fits have been
253 commited.
254 fit - execute the actual fitting process
255 get_chi2 - get the Chi^2
256 set_scan - set the scantable to be fit
257 set_function - set the fitting function
258 set_parameters - set the parameters for the function(s), and
259 set if they should be held fixed during fitting
260 get_parameters - get the fitted parameters
261 [Plotter]
262 asapplotter - a plotter for asap, default plotter is
263 called 'plotter'
264 plot - plot a (list of) scantable
265 set_mode - set the state of the plotter, i.e.
266 what is to be plotted 'colour stacked'
267 and what 'panelled'
268 set_range - set the abcissa 'zoom' range
269 set_legend_map - specify user labels for the legend indeces
270
271 [Reading files]
272 reader - access rpfits/sdfits files
273 read - read in integrations
274 summary - list info about all integrations
275
276 [General]
277 commands - this command
278 print - print details about a variable
279 list_scans - list all scantables created bt the user
280 del - delete the given variable from memory
281 range - create a list of values, e.g.
282 range(3) = [0,1,2], range(2,5) = [2,3,4]
283 help - print help for one of the listed functions
284 execfile - execute an asap script, e.g. execfile('myscript')
285 Note:
286 How to use this with help:
287 # function 'summary'
288 [xxx] is just a category
289 Every 'sub-level' in this list should be replaces by a '.' Period when
290 using help
291 Example:
292 ASAP> help scantable # to get info on ths scantable
293 ASAP> help scantable.summary # to get help on the scantable's
294 ASAP> help average_time
295
296 """
297 print x
298 return
299
300print """Welcome to ASAP - the ATNF Single Dish Analysis Package
301This is a testing pre-release v0.1a
302
303Please report any bugs to:
304Malte.Marquarding@csiro.au
305
306[NOTE: ASAP is 0-based]
307Type commands() to get a list of all available ASAP commands.
308"""
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