Coverage for /wheeldirectory/casa-6.7.0-12-py3.10.el8/lib/py/lib/python3.10/site-packages/casatasks/fluxscale.py: 56%
27 statements
« prev ^ index » next coverage.py v7.6.4, created at 2024-10-31 17:39 +0000
1##################### generated by xml-casa (v2) from fluxscale.xml #################
2##################### d755b0baa9e1470fc32bae479b20569e ##############################
3from __future__ import absolute_import
4import numpy
5from casatools.typecheck import CasaValidator as _val_ctor
6_pc = _val_ctor( )
7from casatools.coercetype import coerce as _coerce
8from casatools.errors import create_error_string
9from .private.task_fluxscale import fluxscale as _fluxscale_t
10from casatasks.private.task_logging import start_log as _start_log
11from casatasks.private.task_logging import end_log as _end_log
12from casatasks.private.task_logging import except_log as _except_log
14class _fluxscale:
15 """
16 fluxscale ---- Bootstrap the flux density scale from standard calibrators
19 Bootstrap the flux density scale from standard calibrators.
22 --------- parameter descriptions ---------------------------------------------
24 vis Name of input visibility file
25 Default: none
27 Example: vis='ngc5921.ms'
28 caltable Name of input calibration table
29 Default: none
31 Example: caltable='ngc5921.gcal'. This cal
32 table was obtained from task gaincal.=
33 fluxtable Name of output, flux-scaled calibration table (required)
34 Default: none
36 Example: fluxtable='ngc5921.gcal2'
38 The gains in this table have been adjusted by the
39 derived flux density each calibrator. The
40 MODEL_DATA column has NOT been updated for the
41 flux density of the calibrator. Use setjy to do
42 this if it is a point source.
43 reference Reference field name(s) (transfer flux scale FROM)
44 Default: none
46 Example: reference='1328+307'
48 The names of the fields with a known flux
49 densities or visibilities that have been placed
50 in the MODEL column by setjy or ft for a model
51 not in the CASA system. The syntax is similar to
52 field. Hence field index or names can be used.
53 transfer Transfer field name(s) (transfer flux scale TO)
54 Default: '' (all sources in caltable that are not
55 specified as reference sources. Do not include
56 unknown target sources)
58 The names of the fields with unknown flux
59 densities. These should be point-like calibrator
60 sources The syntax is similar to field. Hence
61 source index or names can be used.
63 Examples: transfer='1445+099, 3C84'; transfer
64 = '0,4'
66 NOTE: All fields in reference and transfer must
67 have solutions in the caltable.
68 listfile Name of listfile that contains the fit information.
69 Default: '' (no fit listfile will be created)
71 The list file contains the flux density, flux
72 density error, S/N, and number of solutions (all
73 antennas and feeds) for each spectral window.
74 NOTE: The nominal spectral window frequencies
75 will be included in the future.
76 append Append fluxscaled solutions to the fluxtable?
77 Default: False (the fluxtable must not exist)
78 Options: False|True
79 refspwmap Vector of spectral windows enabling scaling across
80 spectral windows
81 Default: [-1] (none)
83 Example with 4 spectral windows:
84 If the reference fields were observed only in
85 spw=1 and 3, and the transfer fields were
86 observed in all 4 spws (0,1,2,3), specify
87 refspwmap=[1,1,3,3]. This will ensure that
88 transfer fields observed in spws 0,1,2,3 will
89 be referenced to reference field solutions
90 only in spw 1 or 3.
91 gainthreshold Threshold in the input gain solutions to be used in fractional deviation from median values.
92 Default: -1 (no threshold)
94 Example: gainthreshold=0.15 (only used the
95 gain solutions within 15% (inclusive) of the
96 median gain value (per field and per spw).
97 antenna Select data based on antenna/baseline
98 Subparameter of antenna
99 Default: '' (all)
101 If antenna string is a non-negative integer, it
102 is assumed an antenna index, otherwise, it is
103 assumed as an antenna name
105 Examples:
106 antenna='5&6'; baseline between antenna
107 index 5 and index 6.
108 antenna='VA05&VA06'; baseline between VLA
109 antenna 5 and 6.
110 antenna='5&6;7&8'; baselines with
111 indices 5-6 and 7-8
112 antenna='5'; all baselines with antenna index
113 5
114 antenna='05'; all baselines with antenna
115 number 05 (VLA old name)
116 antenna='5,6,10'; all baselines with antennas
117 5,6,10 index numbers
118 timerange Select data based on time range
119 Subparameter of antenna
120 Default = '' (all)
122 Examples:
123 timerange =
124 'YYYY/MM/DD/hh:mm:ss~YYYY/MM/DD/hh:mm:ss'
125 (Note: if YYYY/MM/DD is missing date defaults
126 to first day in data set.)
127 timerange='09:14:0~09:54:0' picks 40 min on
128 first day
129 timerange= '25:00:00~27:30:00' picks 1 hr to 3
130 hr 30min on NEXT day
131 timerange='09:44:00' pick data within one
132 integration of time
133 timerange='>10:24:00' data after this time
134 scan Scan number range
135 Subparameter of antenna
136 Default: '' = all
137 incremental Create an incremental caltable containing only gain
138 correction factors ( flux density= 1/(gain correction factor)**2)?
139 Default: False
140 Options: False|True
142 Example: incremental=True (output a caltable
143 containing flux scale factors.)
145 NOTE: If you use the incremental option, note
146 that BOTH this incremental fluxscale table AND an
147 amplitude vs. time table should be supplied in
148 applycal.
149 fitorder Polynomial order of the spectral fitting for valid flux
150 densities
151 Default: 1
153 It falls back to a lower fitorder if there are
154 not enough solutions to fit with the requested
155 fitorder.
156 display Display statistics and/or spectral fitting results.
157 Default: False
158 Options: False|True
160 Currently only a histogram of the correction
161 factors to derive the final flux density for each
162 spectral window will be plotted.
164 --------- examples -----------------------------------------------------------
167 For more information, see the task pages of fluxscale in CASA Docs:
169 https://casa.nrao.edu/casadocs/
173 """
175 _info_group_ = """calibration"""
176 _info_desc_ = """Bootstrap the flux density scale from standard calibrators"""
178 def __call__( self, vis='', caltable='', fluxtable='', reference=[ ], transfer=[ ], listfile='', append=False, refspwmap=[ int(-1) ], gainthreshold=float(-1.0), antenna='', timerange='', scan='', incremental=False, fitorder=int(1), display=False ):
179 schema = {'vis': {'type': 'cReqPath', 'coerce': _coerce.expand_path}, 'caltable': {'type': 'cStr', 'coerce': _coerce.to_str}, 'fluxtable': {'type': 'cStr', 'coerce': _coerce.to_str}, 'reference': {'type': 'cStrVec', 'coerce': [_coerce.to_list,_coerce.to_strvec]}, 'transfer': {'type': 'cStrVec', 'coerce': [_coerce.to_list,_coerce.to_strvec]}, 'listfile': {'type': 'cStr', 'coerce': _coerce.to_str}, 'append': {'type': 'cBool'}, 'refspwmap': {'type': 'cIntVec', 'coerce': [_coerce.to_list,_coerce.to_intvec]}, 'gainthreshold': {'type': 'cFloat', 'coerce': _coerce.to_float}, 'antenna': {'type': 'cStr', 'coerce': _coerce.to_str}, 'timerange': {'type': 'cStr', 'coerce': _coerce.to_str}, 'scan': {'type': 'cStr', 'coerce': _coerce.to_str}, 'incremental': {'type': 'cBool'}, 'fitorder': {'type': 'cInt'}, 'display': {'type': 'cBool'}}
180 doc = {'vis': vis, 'caltable': caltable, 'fluxtable': fluxtable, 'reference': reference, 'transfer': transfer, 'listfile': listfile, 'append': append, 'refspwmap': refspwmap, 'gainthreshold': gainthreshold, 'antenna': antenna, 'timerange': timerange, 'scan': scan, 'incremental': incremental, 'fitorder': fitorder, 'display': display}
181 assert _pc.validate(doc,schema), create_error_string(_pc.errors)
182 _logging_state_ = _start_log( 'fluxscale', [ 'vis=' + repr(_pc.document['vis']), 'caltable=' + repr(_pc.document['caltable']), 'fluxtable=' + repr(_pc.document['fluxtable']), 'reference=' + repr(_pc.document['reference']), 'transfer=' + repr(_pc.document['transfer']), 'listfile=' + repr(_pc.document['listfile']), 'append=' + repr(_pc.document['append']), 'refspwmap=' + repr(_pc.document['refspwmap']), 'gainthreshold=' + repr(_pc.document['gainthreshold']), 'antenna=' + repr(_pc.document['antenna']), 'timerange=' + repr(_pc.document['timerange']), 'scan=' + repr(_pc.document['scan']), 'incremental=' + repr(_pc.document['incremental']), 'fitorder=' + repr(_pc.document['fitorder']), 'display=' + repr(_pc.document['display']) ] )
183 task_result = None
184 try:
185 task_result = _fluxscale_t( _pc.document['vis'], _pc.document['caltable'], _pc.document['fluxtable'], _pc.document['reference'], _pc.document['transfer'], _pc.document['listfile'], _pc.document['append'], _pc.document['refspwmap'], _pc.document['gainthreshold'], _pc.document['antenna'], _pc.document['timerange'], _pc.document['scan'], _pc.document['incremental'], _pc.document['fitorder'], _pc.document['display'] )
186 except Exception as exc:
187 _except_log('fluxscale', exc)
188 raise
189 finally:
190 task_result = _end_log( _logging_state_, 'fluxscale', task_result )
191 return task_result
193fluxscale = _fluxscale( )