source: trunk/python/__init__.py@ 1727

Last change on this file since 1727 was 1725, checked in by Malte Marquarding, 15 years ago

Finishing touches to opacity calculations, docs, plotting and model

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[100]1"""
2This is the ATNF Single Dish Analysis package.
3
4"""
[1080]5import os,sys,shutil, platform
[1691]6try:
7 from functools import wraps as wraps_dec
8except ImportError:
9 from asap.compatibility import wraps as wraps_dec
[226]10
[1080]11# Set up AIPSPATH and first time use of asap i.e. ~/.asap/*
12plf = None
13if sys.platform == "linux2":
14 if platform.architecture()[0] == '64bit':
15 plf = 'linux_64b'
16 else:
17 plf = 'linux_gnu'
18elif sys.platform == 'darwin':
19 plf = 'darwin'
20else:
21 # Shouldn't happen - default to linux
22 plf = 'linux'
23asapdata = __path__[-1]
[1171]24# Allow user defined data location
25if os.environ.has_key("ASAPDATA"):
26 if os.path.exists(os.environ["ASAPDATA"]):
27 asapdata = os.environ["ASAPDATA"]
[1371]28# use AIPSPATH if defined and "data" dir present
29if not os.environ.has_key("AIPSPATH") or \
30 not os.path.exists(os.environ["AIPSPATH"].split()[0]+"/data"):
[1316]31 os.environ["AIPSPATH"] = "%s %s somwhere" % ( asapdata, plf)
[1171]32# set up user space
[1080]33userdir = os.environ["HOME"]+"/.asap"
34if not os.path.exists(userdir):
35 print 'First time ASAP use. Setting up ~/.asap'
36 os.mkdir(userdir)
37 shutil.copyfile(asapdata+"/data/ipythonrc-asap", userdir+"/ipythonrc-asap")
[1588]38 shutil.copyfile(asapdata+"/data/ipy_user_conf.py",
[1434]39 userdir+"/ipy_user_conf.py")
[1080]40 f = file(userdir+"/asapuserfuncs.py", "w")
41 f.close()
42 f = file(userdir+"/ipythonrc", "w")
43 f.close()
[1472]44else:
45 # upgrade to support later ipython versions
46 if not os.path.exists(userdir+"/ipy_user_conf.py"):
[1588]47 shutil.copyfile(asapdata+"/data/ipy_user_conf.py",
[1472]48 userdir+"/ipy_user_conf.py")
49
[1171]50# remove from namespace
[1080]51del asapdata, userdir, shutil, platform
52
[513]53def _validate_bool(b):
[226]54 'Convert b to a boolean or raise'
55 bl = b.lower()
56 if bl in ('f', 'no', 'false', '0', 0): return False
57 elif bl in ('t', 'yes', 'true', '1', 1): return True
58 else:
59 raise ValueError('Could not convert "%s" to boolean' % b)
60
[513]61def _validate_int(s):
[226]62 'convert s to int or raise'
63 try: return int(s)
64 except ValueError:
65 raise ValueError('Could not convert "%s" to int' % s)
66
[513]67def _asap_fname():
[226]68 """
69 Return the path to the rc file
70
71 Search order:
72
73 * current working dir
74 * environ var ASAPRC
[274]75 * HOME/.asaprc
[706]76
[226]77 """
78
79 fname = os.path.join( os.getcwd(), '.asaprc')
80 if os.path.exists(fname): return fname
81
82 if os.environ.has_key('ASAPRC'):
83 path = os.environ['ASAPRC']
84 if os.path.exists(path):
85 fname = os.path.join(path, '.asaprc')
86 if os.path.exists(fname):
87 return fname
88
89 if os.environ.has_key('HOME'):
90 home = os.environ['HOME']
91 fname = os.path.join(home, '.asaprc')
92 if os.path.exists(fname):
93 return fname
94 return None
95
[706]96
[226]97defaultParams = {
98 # general
[513]99 'verbose' : [True, _validate_bool],
100 'useplotter' : [True, _validate_bool],
[542]101 'insitu' : [True, _validate_bool],
[706]102
[226]103 # plotting
[706]104 'plotter.gui' : [True, _validate_bool],
[226]105 'plotter.stacking' : ['p', str],
106 'plotter.panelling' : ['s', str],
[700]107 'plotter.colours' : ['', str],
108 'plotter.linestyles' : ['', str],
[710]109 'plotter.decimate' : [False, _validate_bool],
110 'plotter.ganged' : [True, _validate_bool],
[1022]111 'plotter.histogram' : [False, _validate_bool],
[1097]112 'plotter.papertype' : ['A4', str],
[1560]113 'plotter.axesformatting' : ['mpl', str],
[710]114
[226]115 # scantable
116 'scantable.save' : ['ASAP', str],
[513]117 'scantable.autoaverage' : [True, _validate_bool],
[226]118 'scantable.freqframe' : ['LSRK', str], #default frequency frame
[1076]119 'scantable.verbosesummary' : [False, _validate_bool],
[1422]120 'scantable.storage' : ['memory', str],
[1504]121 'scantable.history' : [True, _validate_bool],
[1586]122 'scantable.reference' : ['.*(e|w|_R)$', str],
123 'scantable.parallactify' : [False, _validate_bool]
[226]124 # fitter
125 }
126
[255]127def list_rcparameters():
[706]128
[255]129 print """
[737]130# general
131# print verbose output
132verbose : True
[255]133
[737]134# preload a default plotter
135useplotter : True
[255]136
[737]137# apply operations on the input scantable or return new one
138insitu : True
[706]139
[737]140# plotting
[710]141
[737]142# do we want a GUI or plot to a file
143plotter.gui : True
[710]144
[737]145# default mode for colour stacking
146plotter.stacking : Pol
[255]147
[737]148# default mode for panelling
149plotter.panelling : scan
[255]150
[1560]151# push panels together, to share axis labels
[737]152plotter.ganged : True
[710]153
[1513]154# decimate the number of points plotted by a factor of
[737]155# nchan/1024
156plotter.decimate : False
[733]157
[737]158# default colours/linestyles
159plotter.colours :
160plotter.linestyles :
[700]161
[1022]162# enable/disable histogram plotting
163plotter.histogram : False
164
[1097]165# ps paper type
166plotter.papertype : A4
167
[1513]168# The formatting style of the xaxis
[1560]169plotter.axesformatting : 'mpl' (default) or 'asap' (for old versions of matplotlib)
[1513]170
[737]171# scantable
[1076]172
[1259]173# default storage of scantable ('memory'/'disk')
[1076]174scantable.storage : memory
[1422]175
176# write history of each call to scantable
177scantable.history : True
178
[737]179# default ouput format when saving
180scantable.save : ASAP
[1422]181
[737]182# auto averaging on read
183scantable.autoaverage : True
[255]184
[737]185# default frequency frame to set when function
[1097]186# scantable.set_freqframe is called
[737]187scantable.freqframe : LSRK
[255]188
[737]189# Control the level of information printed by summary
190scantable.verbosesummary : False
[706]191
[1504]192# Control the identification of reference (off) scans
193# This is has to be a regular expression
[1595]194scantable.reference : .*(e|w|_R)$
[1560]195
[1595]196# Indicate whether the data was parallactified (total phase offest == 0.0)
197scantable.parallactify : False
198
[737]199# Fitter
200"""
[706]201
[226]202def rc_params():
203 'Return the default params updated from the values in the rc file'
[706]204
[513]205 fname = _asap_fname()
[706]206
[226]207 if fname is None or not os.path.exists(fname):
208 message = 'could not find rc file; returning defaults'
209 ret = dict([ (key, tup[0]) for key, tup in defaultParams.items()])
210 #print message
211 return ret
[706]212
[226]213 cnt = 0
214 for line in file(fname):
215 cnt +=1
216 line = line.strip()
217 if not len(line): continue
218 if line.startswith('#'): continue
219 tup = line.split(':',1)
220 if len(tup) !=2:
221 print ('Illegal line #%d\n\t%s\n\tin file "%s"' % (cnt, line, fname))
222 continue
[706]223
[226]224 key, val = tup
225 key = key.strip()
226 if not defaultParams.has_key(key):
227 print ('Bad key "%s" on line %d in %s' % (key, cnt, fname))
228 continue
[706]229
[226]230 default, converter = defaultParams[key]
231
232 ind = val.find('#')
233 if ind>=0: val = val[:ind] # ignore trailing comments
234 val = val.strip()
235 try: cval = converter(val) # try to convert to proper type or raise
[1080]236 except ValueError, msg:
[226]237 print ('Bad val "%s" on line #%d\n\t"%s"\n\tin file "%s"\n\t%s' % (val, cnt, line, fname, msg))
238 continue
239 else:
240 # Alles Klar, update dict
241 defaultParams[key][0] = cval
242
243 # strip the conveter funcs and return
244 ret = dict([ (key, tup[0]) for key, tup in defaultParams.items()])
[466]245 print ('loaded rc file %s'%fname)
[226]246
247 return ret
248
249
250# this is the instance used by the asap classes
[706]251rcParams = rc_params()
[226]252
253rcParamsDefault = dict(rcParams.items()) # a copy
254
255def rc(group, **kwargs):
256 """
257 Set the current rc params. Group is the grouping for the rc, eg
[379]258 for scantable.save the group is 'scantable', for plotter.stacking, the
259 group is 'plotter', and so on. kwargs is a list of attribute
[226]260 name/value pairs, eg
261
[379]262 rc('scantable', save='SDFITS')
[226]263
264 sets the current rc params and is equivalent to
[706]265
[379]266 rcParams['scantable.save'] = 'SDFITS'
[226]267
268 Use rcdefaults to restore the default rc params after changes.
269 """
270
[379]271 aliases = {}
[706]272
[226]273 for k,v in kwargs.items():
274 name = aliases.get(k) or k
[1422]275 if len(group):
276 key = '%s.%s' % (group, name)
277 else:
278 key = name
[226]279 if not rcParams.has_key(key):
280 raise KeyError('Unrecognized key "%s" for group "%s" and name "%s"' % (key, group, name))
[706]281
[226]282 rcParams[key] = v
283
284
285def rcdefaults():
286 """
287 Restore the default rc params - the ones that were created at
288 asap load time
289 """
290 rcParams.update(rcParamsDefault)
291
[1295]292def _n_bools(n, val):
[1588]293 return [ val for i in xrange(n) ]
[513]294
295def _is_sequence_or_number(param, ptype=int):
296 if isinstance(param,tuple) or isinstance(param,list):
[928]297 if len(param) == 0: return True # empty list
[513]298 out = True
299 for p in param:
300 out &= isinstance(p,ptype)
301 return out
302 elif isinstance(param, ptype):
303 return True
304 return False
305
[928]306def _to_list(param, ptype=int):
307 if isinstance(param, ptype):
308 if ptype is str: return param.split()
309 else: return [param]
310 if _is_sequence_or_number(param, ptype):
311 return param
312 return None
[715]313
[944]314def unique(x):
[992]315 """
316 Return the unique values in a list
317 Parameters:
318 x: the list to reduce
319 Examples:
320 x = [1,2,3,3,4]
321 print unique(x)
322 [1,2,3,4]
323 """
[944]324 return dict([ (val, 1) for val in x]).keys()
325
[992]326def list_files(path=".",suffix="rpf"):
327 """
328 Return a list files readable by asap, such as rpf, sdfits, mbf, asap
329 Parameters:
330 path: The directory to list (default '.')
331 suffix: The file extension (default rpf)
332 Example:
333 files = list_files("data/","sdfits")
334 print files
335 ['data/2001-09-01_0332_P363.sdfits',
336 'data/2003-04-04_131152_t0002.sdfits',
337 'data/Sgr_86p262_best_SPC.sdfits']
338 """
339 if not os.path.isdir(path):
340 return None
[1295]341 valid = "rpf rpf.1 rpf.2 sdf sdfits mbf asap".split()
[992]342 if not suffix in valid:
343 return None
344 files = [os.path.expanduser(os.path.expandvars(path+"/"+f)) for f in os.listdir(path)]
345 return filter(lambda x: x.endswith(suffix),files)
346
[715]347# workaround for ipython, which redirects this if banner=0 in ipythonrc
348sys.stdout = sys.__stdout__
349sys.stderr = sys.__stderr__
350
351# Logging
352from asap._asap import Log as _asaplog
353global asaplog
[710]354asaplog=_asaplog()
[715]355if rcParams['verbose']:
356 asaplog.enable()
357else:
358 asaplog.disable()
359
[1589]360
361def print_log_dec(f):
[1691]362 @wraps_dec(f)
[1589]363 def wrap_it(*args, **kw):
364 val = f(*args, **kw)
365 print_log()
366 return val
367 return wrap_it
368
[715]369def print_log():
[1589]370 log = asaplog.pop().strip()
[715]371 if len(log) and rcParams['verbose']: print log
372 return
373
[1295]374def mask_and(a, b):
375 assert(len(a)==len(b))
376 return [ a[i] & b[i] for i in xrange(len(a)) ]
[1134]377
[1295]378def mask_or(a, b):
379 assert(len(a)==len(b))
380 return [ a[i] | b[i] for i in xrange(len(a)) ]
381
382def mask_not(a):
383 return [ not i for i in a ]
384
[1117]385from asapfitter import fitter
[895]386from asapreader import reader
[944]387from selector import selector
[710]388
[100]389from asapmath import *
[1080]390from scantable import scantable
[1097]391from asaplinefind import linefinder
[1645]392from simplelinefinder import simplelinefinder
[1134]393from linecatalog import linecatalog
[1689]394from opacity import skydip
[1725]395from opacity import model as opacity_model
[285]396
[928]397if rcParams['useplotter']:
[1295]398 try:
[1423]399 from asapplotter import asapplotter
400 gui = os.environ.has_key('DISPLAY') and rcParams['plotter.gui']
401 if gui:
[1422]402 import matplotlib
403 matplotlib.use("TkAgg")
[1691]404 from matplotlib import pylab
[1422]405 xyplotter = pylab
[1423]406 plotter = asapplotter(gui)
407 del gui
[1295]408 except ImportError:
[1423]409 print "Matplotlib not installed. No plotting available"
[285]410
[574]411__date__ = '$Date: 2010-04-27 05:48:24 +0000 (Tue, 27 Apr 2010) $'.split()[1]
[1560]412__version__ = '$Revision: 1725 $'
[100]413
[1193]414def is_ipython():
[1725]415 return 'IPython' in sys.modules.keys()
[1589]416
[1193]417if is_ipython():
[1014]418 def version(): print "ASAP %s(%s)"% (__version__, __date__)
[1588]419
420 def list_scans(t = scantable):
[1560]421 import inspect
422 print "The user created scantables are: ",
423 globs=inspect.currentframe().f_back.f_locals.copy()
424 out = [ k for k,v in globs.iteritems() \
425 if isinstance(v, scantable) and not k.startswith("_") ]
426 print out
427 return out
[100]428
[715]429 def commands():
430 x = """
[113]431 [The scan container]
432 scantable - a container for integrations/scans
[182]433 (can open asap/rpfits/sdfits and ms files)
[113]434 copy - returns a copy of a scan
435 get_scan - gets a specific scan out of a scantable
[984]436 (by name or number)
[1093]437 drop_scan - drops a specific scan out of a scantable
438 (by number)
[984]439 set_selection - set a new subselection of the data
440 get_selection - get the current selection object
[113]441 summary - print info about the scantable contents
[182]442 stats - get specified statistic of the spectra in
443 the scantable
444 stddev - get the standard deviation of the spectra
445 in the scantable
[113]446 get_tsys - get the TSys
447 get_time - get the timestamps of the integrations
[1351]448 get_inttime - get the integration time
[733]449 get_sourcename - get the source names of the scans
[794]450 get_azimuth - get the azimuth of the scans
451 get_elevation - get the elevation of the scans
452 get_parangle - get the parallactic angle of the scans
[1697]453 get_coordinate - get the spectral coordinate for the given row,
454 which can be used for coordinate conversions
[876]455 get_unit - get the current unit
[513]456 set_unit - set the abcissa unit to be used from this
457 point on
[255]458 get_abcissa - get the abcissa values and name for a given
459 row (time)
[1259]460 get_column_names - get the names of the columns in the scantable
461 for use with selector.set_query
[113]462 set_freqframe - set the frame info for the Spectral Axis
463 (e.g. 'LSRK')
[276]464 set_doppler - set the doppler to be used from this point on
[984]465 set_dirframe - set the frame for the direction on the sky
[240]466 set_instrument - set the instrument name
[1190]467 set_feedtype - set the feed type
[255]468 get_fluxunit - get the brightness flux unit
[240]469 set_fluxunit - set the brightness flux unit
[1508]470 set_sourcetype - set the type of the source - source or reference
[188]471 create_mask - return an mask in the current unit
472 for the given region. The specified regions
473 are NOT masked
[255]474 get_restfreqs - get the current list of rest frequencies
475 set_restfreqs - set a list of rest frequencies
[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
[1012]480 flag - flag selected channels in the data
[1192]481 lag_flag - flag specified frequency in the data
[1151]482 save - save the scantable to disk as either 'ASAP',
483 'SDFITS' or 'ASCII'
[486]484 nbeam,nif,nchan,npol - the number of beams/IFs/Pols/Chans
[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.
[1144]492 average_beam - average the beams together.
[992]493 convert_pol - convert to a different polarisation type
[690]494 auto_quotient - return the on/off quotient with
[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
[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]658def welcome():
659 return """Welcome to ASAP v%s (%s) - the ATNF Spectral Analysis Package
[100]660
[1035]661Please report any bugs via:
[1378]662http://svn.atnf.csiro.au/trac/asap/simpleticket
[100]663
[378]664[IMPORTANT: ASAP is 0-based]
[706]665Type commands() to get a list of all available ASAP commands.""" % (__version__, __date__)
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