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1# This file was automatically generated by SWIG (http://www.swig.org).
2# Version 3.0.12
3#
4# Do not make changes to this file unless you know what you are doing--modify
5# the SWIG interface file instead.
7from sys import version_info as _swig_python_version_info
8if _swig_python_version_info >= (2, 7, 0):
9 def swig_import_helper():
10 import importlib
11 pkg = __name__.rpartition('.')[0]
12 mname = '.'.join((pkg, '_vpmanager')).lstrip('.')
13 try:
14 return importlib.import_module(mname)
15 except ImportError:
16 return importlib.import_module('_vpmanager')
17 _vpmanager = swig_import_helper()
18 del swig_import_helper
19elif _swig_python_version_info >= (2, 6, 0):
20 def swig_import_helper():
21 from os.path import dirname
22 import imp
23 fp = None
24 try:
25 fp, pathname, description = imp.find_module('_vpmanager', [dirname(__file__)])
26 except ImportError:
27 import _vpmanager
28 return _vpmanager
29 try:
30 _mod = imp.load_module('_vpmanager', fp, pathname, description)
31 finally:
32 if fp is not None:
33 fp.close()
34 return _mod
35 _vpmanager = swig_import_helper()
36 del swig_import_helper
37else:
38 import _vpmanager
39del _swig_python_version_info
41try:
42 _swig_property = property
43except NameError:
44 pass # Python < 2.2 doesn't have 'property'.
46try:
47 import builtins as __builtin__
48except ImportError:
49 import __builtin__
51def _swig_setattr_nondynamic(self, class_type, name, value, static=1):
52 if (name == "thisown"):
53 return self.this.own(value)
54 if (name == "this"):
55 if type(value).__name__ == 'SwigPyObject':
56 self.__dict__[name] = value
57 return
58 method = class_type.__swig_setmethods__.get(name, None)
59 if method:
60 return method(self, value)
61 if (not static):
62 if _newclass:
63 object.__setattr__(self, name, value)
64 else:
65 self.__dict__[name] = value
66 else:
67 raise AttributeError("You cannot add attributes to %s" % self)
70def _swig_setattr(self, class_type, name, value):
71 return _swig_setattr_nondynamic(self, class_type, name, value, 0)
74def _swig_getattr(self, class_type, name):
75 if (name == "thisown"):
76 return self.this.own()
77 method = class_type.__swig_getmethods__.get(name, None)
78 if method:
79 return method(self)
80 raise AttributeError("'%s' object has no attribute '%s'" % (class_type.__name__, name))
83def _swig_repr(self):
84 try:
85 strthis = "proxy of " + self.this.__repr__()
86 except __builtin__.Exception:
87 strthis = ""
88 return "<%s.%s; %s >" % (self.__class__.__module__, self.__class__.__name__, strthis,)
90try:
91 _object = object
92 _newclass = 1
93except __builtin__.Exception:
94 class _object:
95 pass
96 _newclass = 0
98class vpmanager(_object):
99 """Proxy of C++ casac::vpmanager class."""
101 __swig_setmethods__ = {}
102 __setattr__ = lambda self, name, value: _swig_setattr(self, vpmanager, name, value)
103 __swig_getmethods__ = {}
104 __getattr__ = lambda self, name: _swig_getattr(self, vpmanager, name)
105 __repr__ = _swig_repr
107 def __init__(self):
108 """__init__(self) -> vpmanager"""
109 this = _vpmanager.new_vpmanager()
110 try:
111 self.this.append(this)
112 except __builtin__.Exception:
113 self.this = this
115 def saveastable(self, *args, **kwargs):
116 """
117 saveastable(self, _tablename) -> bool
121 Summary:
122 Save the vp or pb descriptions as a table
124 Description:
127 Save the vp or pb descriptions as a table. Each description is in a different
128 row of the table.
130 Input Parameters:
131 tablename Name of table to save vp descriptions in
133 --------------------------------------------------------------------------------
135 """
136 return _vpmanager.vpmanager_saveastable(self, *args, **kwargs)
139 def loadfromtable(self, *args, **kwargs):
140 """
141 loadfromtable(self, _tablename) -> bool
145 Summary:
146 Load the vp or pb descriptions from a table (deleting all previous definitions)
148 Description:
151 Load the vp or pb descriptions from a table created, e.g., with saveastable().
153 Input Parameters:
154 tablename Name of table to load vp descriptions from
156 --------------------------------------------------------------------------------
158 """
159 return _vpmanager.vpmanager_loadfromtable(self, *args, **kwargs)
162 def summarizevps(self, *args, **kwargs):
163 """
164 summarizevps(self, _verbose) -> bool
168 Summary:
169 Summarize the currently accumulated VP descriptions
171 Description:
174 Summarize the currently accumulated VP descriptions to the logger.
176 Input Parameters:
177 verbose Print out full record? Otherwise, print summary.
179 --------------------------------------------------------------------------------
181 """
182 return _vpmanager.vpmanager_summarizevps(self, *args, **kwargs)
185 def setcannedpb(self, *args, **kwargs):
186 """
187 setcannedpb(self, _telescope, _othertelescope, _dopb, _commonpb, _dosquint, _paincrement, _usesymmetricbeam) -> record *
191 Summary:
192 Select a vp/pb from our library of common pb models
194 Description:
197 We have many vp/pb models ready to go for a variety of telescopes. If 'DEFAULT' isselected, the system default for that telescope and frequency is used.
199 Input Parameters:
200 telescope Which telescope in the MS will use this vp/pb?
201 othertelescope If telescope=='OTHER', specify name here
202 dopb Should we apply the vp/pb to this telescope's data?
203 commonpb List of common vp/pb models: DEFAULT code figures it out
204 dosquint Enable the natural beam squint found in the common vp model
205 paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application
206 usesymmetricbeam Not currently used
208 --------------------------------------------------------------------------------
210 """
211 return _vpmanager.vpmanager_setcannedpb(self, *args, **kwargs)
214 def setpbairy(self, *args, **kwargs):
215 """
216 setpbairy(self, _telescope, _othertelescope, _dopb, _dishdiam, _blockagediam, _maxrad, _reffreq, _squintdir, _squintreffreq, _dosquint, _paincrement, _usesymmetricbeam) -> record *
220 Summary:
221 Make an airy disk vp
223 Description:
226 Information sufficient to create a portion of the Airy disk voltage pattern.
227 The Airy disk pattern is formed by Fourier transforming a uniformly illuminated
228 aperture and is given by
229 begin{equation}
230 vp_p(i) = ( areaRatio * 2.0 * j_{1}(x)/x
231 - 2.0 * j_{1}(x*lengthRatio)/(x*lengthRatio) )/ areaNorm,
232 end{equation}
233 where areaRatio is the dish area divided by the blockage area, lengthRatio
234 is the dish diameter divided by the blockage diameter, and
235 begin{equation}
236 x = frac{i * maxrad * 7.016 * dishdiam/24.5m}{N_{samples} * 1.566 * 60}.
237 end{equation}
239 Input Parameters:
240 telescope Which telescope in the MS will use this vp/pb?
241 othertelescope If telescope=='OTHER', specify name here
242 dopb Should we apply the vp/pb to this telescope's data?
243 dishdiam Effective diameter of dish
244 blockagediam Effective diameter of subreflector blockage
245 maxrad Maximum radial extent of the vp/pb (scales with 1/freq)
246 reffreq Frequency at which maxrad is specified
247 squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
248 squintreffreq Frequency at which the squint is specified
249 dosquint Enable the natural beam squint found in the common vp model
250 paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application
251 usesymmetricbeam Not currently used
253 --------------------------------------------------------------------------------
255 """
256 return _vpmanager.vpmanager_setpbairy(self, *args, **kwargs)
259 def setpbcospoly(self, *args, **kwargs):
260 """
261 setpbcospoly(self, _telescope, _othertelescope, _dopb, _coeff, _scale, _maxrad, _reffreq, _isthispb, _squintdir, _squintreffreq, _dosquint, _paincrement, _usesymmetricbeam) -> record *
265 Summary:
266 Make a vp/pb from a polynomial of scaled cosines
268 Description:
271 A voltage pattern or primary beam of the form
272 begin{equation}
273 VP(x) = sum_{i} ( coeff_{i} cos^{2i}( scale_{i} x).
274 end{equation}
275 This is a generalization of the WSRT primary beam model.
277 Input Parameters:
278 telescope Which telescope in the MS will use this vp/pb?
279 othertelescope If telescope=='OTHER', specify name here
280 dopb Should we apply the vp/pb to this telescope's data?
281 coeff Vector of coefficients of cosines
282 scale Vector of scale factors of cosines
283 maxrad Maximum radial extent of the vp/pb (scales with 1/freq)
284 reffreq Frequency at which maxrad is specified
285 isthispb Do these parameters describe a PB or a VP?
286 squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
287 squintreffreq Frequency at which the squint is specified
288 dosquint Enable the natural beam squint found in the common vp model
289 paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application
290 usesymmetricbeam Not currently used
292 --------------------------------------------------------------------------------
294 """
295 return _vpmanager.vpmanager_setpbcospoly(self, *args, **kwargs)
298 def setpbgauss(self, *args, **kwargs):
299 """
300 setpbgauss(self, _telescope, _othertelescope, _dopb, _halfwidth, _maxrad, _reffreq, _isthispb, _squintdir, _squintreffreq, _dosquint, _paincrement, _usesymmetricbeam) -> record *
304 Summary:
305 Make a Gaussian vp/pb
307 Description:
310 Make a Gaussian primary beam given by
311 begin{equation}
312 PB(x) = e^{- (x/(halfwidth*sqrt{1/log(2)})) }.
313 end{equation}
315 Input Parameters:
316 telescope Which telescope in the MS will use this vp/pb?
317 othertelescope If telescope=='OTHER', specify name here
318 dopb Should we apply the vp/pb to this telescope's data?
319 halfwidth Half power half width of the Gaussian at the reffreq
320 maxrad Maximum radial extent of the vp/pb (scales with 1/freq)
321 reffreq Frequency at which maxrad is specified
322 isthispb Do these parameters describe a PB or a VP?
323 squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
324 squintreffreq Frequency at which the squint is specified
325 dosquint Enable the natural beam squint found in the common vp model
326 paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application
327 usesymmetricbeam Not currently used
329 --------------------------------------------------------------------------------
331 """
332 return _vpmanager.vpmanager_setpbgauss(self, *args, **kwargs)
335 def setpbinvpoly(self, *args, **kwargs):
336 """
337 setpbinvpoly(self, _telescope, _othertelescope, _dopb, _coeff, _maxrad, _reffreq, _isthispb, _squintdir, _squintreffreq, _dosquint, _paincrement, _usesymmetricbeam) -> record *
341 Summary:
342 Make a vp/pb as an inverse polynomial
344 Description:
347 The inverse polynomial describes the inverse of the VP or PB
348 as a polynomial of even powers:
349 begin{equation}
350 1/VP(x) = sum_{i} coeff_{i} * x^{2i}.
351 end{equation}
353 Input Parameters:
354 telescope Which telescope in the MS will use this vp/pb?
355 othertelescope If telescope=='OTHER', specify name here
356 dopb Should we apply the vp/pb to this telescope's data?
357 coeff Coefficients of even powered terms
358 maxrad Maximum radial extent of the vp/pb (scales with 1/freq)
359 reffreq Frequency at which maxrad is specified
360 isthispb Do these parameters describe a PB or a VP?
361 squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
362 squintreffreq Frequency at which the squint is specified
363 dosquint Enable the natural beam squint found in the common vp model
364 paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application
365 usesymmetricbeam Not currently used
367 --------------------------------------------------------------------------------
369 """
370 return _vpmanager.vpmanager_setpbinvpoly(self, *args, **kwargs)
373 def setpbnumeric(self, *args, **kwargs):
374 """
375 setpbnumeric(self, _telescope, _othertelescope, _dopb, _vect, _maxrad, _reffreq, _isthispb, _squintdir, _squintreffreq, _dosquint, _paincrement, _usesymmetricbeam) -> record *
379 Summary:
380 Make a vp/pb from a user-supplied vector
382 Description:
385 Supply a vector of vp/pb sample values taken on a regular grid between x=0 and
386 x=maxrad. We perform sinc interpolation to fill in the lookup table.
388 Input Parameters:
389 telescope Which telescope in the MS will use this vp/pb?
390 othertelescope If telescope=='OTHER', specify name here
391 dopb Should we apply the vp/pb to this telescope's data?
392 vect Vector of vp/pb samples uniformly spaced from 0 to maxrad
393 maxrad Maximum radial extent of the vp/pb (scales with 1/freq)
394 reffreq Frequency at which maxrad is specified
395 isthispb Do these parameters describe a PB or a VP?
396 squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
397 squintreffreq Frequency at which the squint is specified
398 dosquint Enable the natural beam squint found in the common vp model
399 paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application
400 usesymmetricbeam Not currently used
402 --------------------------------------------------------------------------------
404 """
405 return _vpmanager.vpmanager_setpbnumeric(self, *args, **kwargs)
408 def setpbimage(self, *args, **kwargs):
409 """
410 setpbimage(self, _telescope, _othertelescope, _dopb, _realimage, _imagimage, _compleximage, _antnames) -> record *
414 Summary:
415 Make a vp/pb from a user-supplied image
417 Description:
420 Experimental: Supply an image of the E Jones elements. The format of the
421 image is:
422 begin{description}
423 item[Shape] nx by ny by 4 complex polarizations (RR, RL, LR, LL or
424 XX, XY, YX, YY) by 1 channel.
425 item[Direction coordinate] Az, El
426 item[Stokes coordinate] All four ``stokes'' parameters must be present
427 in the sequence RR, RL, LR, LL or XX, XY, YX, YY.
428 item[Frequency] Only one channel is currently needed - frequency
429 dependence beyond that is ignored.
430 end{description}
432 If a compleximage is specified the real and imaginary images is to be left empty.
434 The other option is to provide the real and imaginary part of the E-Jones as seperale {tt float} images
435 On that case
436 one or two images may be specified - the real (must be present) and
437 imaginary parts (optional).
439 Note that beamsquint must be intrinsic to the images themselves.
440 This will be accounted for correctly by regridding of the images
441 from Az-El to Ra-Dec according to the parallactic angle.
443 antnames is the Vector of names for which this response pattern apply '*' is for all
444 The name has to match exactly the name of the Antennas in the ANTENNA table of the MS with which
445 you want to use this VPManager table or object.
447 Input Parameters:
448 telescope Which telescope in the MS will use this vp/pb?
449 othertelescope If telescope=='OTHER', specify name here
450 dopb Should we apply the vp/pb to this telescope's data?
451 realimage Real part of vp as an image
452 imagimage Imaginary part of vp as an image
453 compleximage complex vp as an image of complex numbers; if specified realimage and imagimage are ignored
454 antnames antenna names for which this pattern is valid; default is all antennas
456 --------------------------------------------------------------------------------
458 """
459 return _vpmanager.vpmanager_setpbimage(self, *args, **kwargs)
462 def setpbpoly(self, *args, **kwargs):
463 """
464 setpbpoly(self, _telescope, _othertelescope, _dopb, _coeff, _maxrad, _reffreq, _isthispb, _squintdir, _squintreffreq, _dosquint, _paincrement, _usesymmetricbeam) -> record *
468 Summary:
469 Make a vp/pb from a polynomial
471 Description:
474 The VP or PB is described as a polynomial of even powers:
475 begin{equation}
476 VP(x) = sum_{i} coeff_{i} * x^{2i}.
477 end{equation}
479 Input Parameters:
480 telescope Which telescope in the MS will use this vp/pb?
481 othertelescope If telescope=='OTHER', specify name here
482 dopb Should we apply the vp/pb to this telescope's data?
483 coeff Coefficients of even powered terms
484 maxrad Maximum radial extent of the vp/pb (scales with 1/freq)
485 reffreq Frequency at which maxrad is specified
486 isthispb Do these parameters describe a PB or a VP?
487 squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
488 squintreffreq Frequency at which the squint is specified
489 dosquint Enable the natural beam squint found in the common vp model
490 paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application
491 usesymmetricbeam Not currently used
493 --------------------------------------------------------------------------------
495 """
496 return _vpmanager.vpmanager_setpbpoly(self, *args, **kwargs)
499 def setpbantresptable(self, *args, **kwargs):
500 """
501 setpbantresptable(self, _telescope, _othertelescope, _dopb, _antresppath) -> bool
505 Summary:
506 Declare a reference to an antenna responses table
508 Description:
511 Declare a reference to an antenna responses table containing a set of VP/PB definitions.
513 Input Parameters:
514 telescope Which telescope in the MS will use this vp/pb?
515 othertelescope If telescope=='OTHER', specify name here
516 dopb Should we apply the vp/pb to this telescope's data?
517 antresppath The path to the antenna responses table (absolute or relative to CASA data dir.)
519 --------------------------------------------------------------------------------
521 """
522 return _vpmanager.vpmanager_setpbantresptable(self, *args, **kwargs)
525 def reset(self):
526 """
527 reset(self) -> bool
531 Summary:
532 Reinitialize the VPManager (will erase all VPs and defaults defined on the command line)
534 Description:
537 Reinitialize the VPManager database.
538 Erase all VPs and defaults defined on the command line.
540 --------------------------------------------------------------------------------
542 """
543 return _vpmanager.vpmanager_reset(self)
546 def setuserdefault(self, *args, **kwargs):
547 """
548 setuserdefault(self, _vplistnum, _telescope, _anttype) -> bool
552 Summary:
553 Select the VP which is to be used by the imager for the given telescope and antenna type
555 Description:
558 Selects the VP which is to be used by the imager for the given telescope and antenna type.
559 Overwrites a previous default. Returns True if successful.
561 Input Parameters:
562 vplistnum The number of the vp as displayed by summarizevps(), or -1 for internal default, or -2 for unset
563 telescope Which telescope in the MS will use this vp/pb?
564 anttype Which antennatype will use this vp/pb? Default: '' = all
566 --------------------------------------------------------------------------------
568 """
569 return _vpmanager.vpmanager_setuserdefault(self, *args, **kwargs)
572 def getuserdefault(self, *args, **kwargs):
573 """
574 getuserdefault(self, _telescope, _anttype) -> long
578 Summary:
579 Get the vp list number of the present default VP/PB for the given parameters (-1 = internal PB, -2 = none)
581 Description:
584 Get the vp list number of the present default VP/PB for the given parameters.
586 Input Parameters:
587 telescope Which telescope in the MS will use this vp/pb?
588 anttype Which antennatype will use this vp/pb? Default: '' = all
590 --------------------------------------------------------------------------------
592 """
593 return _vpmanager.vpmanager_getuserdefault(self, *args, **kwargs)
596 def getanttypes(self, *args, **kwargs):
597 """
598 getanttypes(self, _telescope, _obstime, _freq, _obsdirection) -> std::vector< std::string >
602 Summary:
603 Return the list of available antenna types for the given parameters
605 Description:
608 Get a list of the available antenna types.
610 Input Parameters:
611 telescope Telescope name
612 obstime Time of the observation (for versioning and reference frame calculations)
613 freq Frequency of the observation (may include reference frame, default: LSRK)
614 obsdirection Direction of the observation (may include reference frame, default: J2000). default: Zenith
616 --------------------------------------------------------------------------------
618 """
619 return _vpmanager.vpmanager_getanttypes(self, *args, **kwargs)
622 def numvps(self, *args, **kwargs):
623 """
624 numvps(self, _telescope, _obstime, _freq, _obsdirection) -> long
628 Summary:
629 Return the number of vps/pbs available for the given parameters
631 Description:
634 Can be used to, e.g., determine the number of antenna types.
635 Note: if a global response is defined for the telescope, this will increase the count of
636 available vps/pbs by 1.
638 Input Parameters:
639 telescope Telescope name
640 obstime Time of the observation (for versioning and reference frame calculations)
641 freq Frequency of the observation (may include reference frame, default: LSRK)
642 obsdirection Direction of the observation (may include reference frame, default: J2000). default: Zenith
644 --------------------------------------------------------------------------------
646 """
647 return _vpmanager.vpmanager_numvps(self, *args, **kwargs)
650 def getvp(self, *args, **kwargs):
651 """
652 getvp(self, _telescope, _antennatype, _obstime, _freq, _obsdirection) -> record *
656 Summary:
657 Return the default vps/pbs record for the given parameters
659 Description:
662 Record is empty if no matching vp/pb could be found.
664 Input Parameters:
665 telescope Telescope name
666 antennatype The antenna type as a string, e.g. 'DV'
667 obstime Time of the observation (for versioning and reference frame calculations), e.g. 2011/12/12T00:00:00
668 freq Frequency of the observation (may include reference frame, default: LSRK)
669 obsdirection Direction of the observation (may include reference frame, default: J2000), default:
671 --------------------------------------------------------------------------------
673 """
674 return _vpmanager.vpmanager_getvp(self, *args, **kwargs)
677 def getvps(self, *args, **kwargs):
678 """
679 getvps(self, _telescope, _antennas, _obstimestart, _obstimeend, _minfreq, _maxfreq, _obsdirection) -> record *
683 Summary:
684 Return the default vps/pbs records for the given antenna list as subrecords in one record
686 Description:
689 Record is empty if no matching vp/pb could be found.
691 Input Parameters:
692 telescope Telescope name
693 antennas The antenna names, e.g., as taken from the MS ANTENNA table
694 obstimestart Time of the start of the observation (for versioning and reference frame calculations), e.g. 2011/12/12T00:00:00
695 obstimeend Time of the end of the observation (for versioning and reference frame calculations), e.g. 2011/12/12T00:00:00
696 minfreq Minimum frequency of the observation (may include reference frame, default: LSRK)
697 maxfreq Maximum frequency of the observation (may include reference frame, default: LSRK)
698 obsdirection Direction of the observation (may include reference frame, default: J2000), default:
700 --------------------------------------------------------------------------------
702 """
703 return _vpmanager.vpmanager_getvps(self, *args, **kwargs)
706 def createantresp(self, *args, **kwargs):
707 """
708 createantresp(self, _imdir, _starttime, _bandnames, _bandminfreq, _bandmaxfreq) -> bool
712 Summary:
713 Create a standard-format AntennaResponses table
715 Description:
718 The AntennaResponses table serves CASA to look up the location of images describing the
719 response of observatory antennas. Three types of images are supported: 'VP' - real voltage patterns,
720 'AIF' - complex aperture illumination patterns, 'EFP' - complex electric field patterns.
721 For each image, a validity range can be defined in Azimuth, Elevation, and Frequency.
722 Furthermore, an antenna type (for heterogeneous arrays), a receiver type (for the case of
723 several receivers on the same antenna having overlapping frequency bands), and a beam number
724 (for the case of multiple beams per antenna) are associated with each response image.
726 The images need to be stored in a single directory DIR of arbitrary name and need to
727 have file names following the pattern
728 begin{verbatim}
729 obsname_beamnum_anttype_rectype_azmin_aznom_azmax_elmin_elnom_elmax_freqmin_freqnom_freqmax_frequnit_comment_functype.im
730 end{verbatim}
731 where the individual name elements mean the following (none of the elements may contain
732 the space character, but they may be empty strings if they are not numerical values):
733 begin{description}
734 item[obsname] - name of the observatory as in the Observatories table, e.g. 'ALMA'
735 item[beamnum] - the numerical beam number (integer) for the case of multiple beams, e.g. 0
736 item[anttype] - name of the antenna type, e.g. 'DV'
737 item[rectype] - name of the receiver type, e.g. ''
738 item[azmin, aznom, azmax] - numerical value (degrees) of the minimal, the nominal, and
739 the maximal Azimuth where this response is valid, e.g. '-10.5_0._10.5'
740 item[elmin, elnom, elmax] - numerical value (degrees) of the minimal, the nominal, and
741 the maximal Elevation where this response is valid, e.g. '10._45._80.'
742 item[freqmin, freqnom, freqmax] - numerical value (degrees) of the minimal, the nominal, and
743 the maximal Frequency (in units of frequnit) where this response is valid, e.g. '84._100._116.'
744 item[frequnit] - the unit of the previous three frequencies, e.g. 'GHz'
745 item[comment] - any string containing only characters permitted in file names and not empty space
746 item[functype] - the type of the image as defined above ('VP', 'AIF', or 'EFP')
747 end{description}
749 The createantresp method will then extract the parameters from all the images in DIR
750 and create the lookup table in the same directory.
752 Input Parameters:
753 imdir Path to the directory containing the response images
754 starttime Time from which onwards the response is valid, format YYYY/MM/DD/hh:mm:ss
755 bandnames List containing the names of the observatory's frequency bands
756 bandminfreq List containing the lower edges of the observatory's frequency bands, e.g. ['80GHz','120GHz']
757 bandmaxfreq List containing the upper edges of the observatory's frequency bands, e.g. ['120GHz','180GHz']
759 --------------------------------------------------------------------------------
761 """
762 return _vpmanager.vpmanager_createantresp(self, *args, **kwargs)
765 def getrespimagename(self, *args, **kwargs):
766 """
767 getrespimagename(self, _telescope, _starttime, _frequency, _functype, _anttype, _azimuth, _elevation, _rectype, _beamnumber) -> string
771 Summary:
772 Get the image name for the given parameters from the given responses table
774 Description:
777 Given the observatory name, the antenna type, the receiver type, the observing frequency, the
778 observing direction, and the beam number, find the applicable response image and return its name.
780 Input Parameters:
781 telescope Which telescope is described by this response?
782 starttime Time at which the response has to be valid, format YYYY/MM/DD/hh:mm:ss
783 frequency The frequency at which the response has to be valid, e.g. '100GHz'
784 functype Type of the responsefunction requested, e.g. 'EFP'
785 anttype Antenna type (observatory-dependent)
786 azimuth Azimuth of the observation (at the location of the observatory, 0 is North), e.g. '5deg'
787 elevation Elevation of the observation (at the location of the observatory, 0 is North), e.g. '60deg'
788 rectype Receiver type (observatory-dependent)
789 beamnumber Beam number (for the case of multiple beams per receiver)
791 --------------------------------------------------------------------------------
793 """
794 return _vpmanager.vpmanager_getrespimagename(self, *args, **kwargs)
796 __swig_destroy__ = _vpmanager.delete_vpmanager
797 __del__ = lambda self: None
798vpmanager_swigregister = _vpmanager.vpmanager_swigregister
799vpmanager_swigregister(vpmanager)
801# This file is compatible with both classic and new-style classes.