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casa
$Rev:20696$
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casa
$Rev:20696$
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Public Member Functions | |
| def | __init__ |
| def | release |
| def | saveastable |
| def | loadfromtable |
| def | summarizevps |
| def | setcannedpb |
| def | setpbairy |
| def | setpbcospoly |
| def | setpbgauss |
| def | setpbinvpoly |
| def | setpbnumeric |
| def | setpbimage |
| def | setpbpoly |
| def | setpbantresptable |
| def | reset |
| def | setuserdefault |
| def | getuserdefault |
| def | getanttypes |
| def | numvps |
| def | getvp |
| def | createantresp |
| def | getrespimagename |
Public Attributes | |
| this | |
Static Private Attributes | |
| dictionary | __swig_setmethods__ |
| tuple | __setattr__ |
| dictionary | __swig_getmethods__ |
| tuple | __getattr__ |
| __repr__ | |
| __swig_destroy__ | |
| __del__ | |
Proxy of C++ casac::vpmanager class
Definition at line 70 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.__init__ | ( | self | ) |
__init__(self) -> vpmanager
Definition at line 77 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.createantresp | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
createantresp(self, imdir=string(""), starttime=string(""), bandnames=std::vector< string >(1, ""), bandminfreq=std::vector< string >(1, ""),
bandmaxfreq=std::vector< string >(1, "")) -> bool
Summary
Create a standard-format AntennaResponses table
Input Parameters:
imdir Path to the directory containing the response images
starttime Time from which onwards the response is valid, format YYYY/MM/DD/hh:mm:ss
bandnames List containing the names of the observatory's frequency bands
bandminfreq List containing the lower edges of the observatory's frequency bands, e.g. ['80GHz','120GHz']
bandmaxfreq List containing the upper edges of the observatory's frequency bands, e.g. ['120GHz','180GHz']
--------------------------------------------------------------------------------Definition at line 484 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.getanttypes | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
getanttypes(self, telescope=string(""), obstime=initialize_variant(""), freq=initialize_variant(""),
obsdirection=initialize_variant("AZEL 0deg 90deg")) -> std::vector< std::string >
Summary
Return the list of available antenna types for the given parameters
Input Parameters:
telescope Telescope name
obstime Time of the observation (for versioning and reference frame calculations)
freq Frequency of the observation (may include reference frame, default: LSRK)
obsdirection Direction of the observation (may include reference frame, default: J2000). default: Zenith AZEL 0deg 90deg
--------------------------------------------------------------------------------Definition at line 426 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.getrespimagename | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
getrespimagename(self, telescope=string(""), starttime=string(""), frequency=string(""), functype=string("ANY"),
anttype=string(""), azimuth=string("0deg"), elevation=string("45deg"),
rectype=string(""), beamnumber=0) -> string
Summary
Get the image name for the given parameters from the given responses table
Input Parameters:
telescope Which telescope is described by this response?
starttime Time at which the response has to be valid, format YYYY/MM/DD/hh:mm:ss
frequency The frequency at which the response has to be valid, e.g. '100GHz'
functype Type of the responsefunction requested, e.g. 'EFP' ANY
anttype Antenna type (observatory-dependent)
azimuth Azimuth of the observation (at the location of the observatory, 0 is North), e.g. '5deg' 0deg
elevation Elevation of the observation (at the location of the observatory, 0 is North), e.g. '60deg' 45deg
rectype Receiver type (observatory-dependent)
beamnumber Beam number (for the case of multiple beams per receiver) 0
--------------------------------------------------------------------------------Definition at line 504 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.getuserdefault | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
getuserdefault(self, telescope=string(""), anttype=string("")) -> int
Summary
Get the vp list number of the present default VP/PB for the given parameters (-1 = internal PB, -2 = none)
Input Parameters:
telescope Which telescope in the MS will use this vp/pb?
anttype Which antennatype will use this vp/pb? Default: '' = all
--------------------------------------------------------------------------------Definition at line 410 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.getvp | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
getvp(self, telescope=string(""), antennatype=string(""), obstime=initialize_variant(""), freq=initialize_variant(""),
obsdirection=initialize_variant("AZEL 0deg 90deg")) -> record *
Summary
Return the default vps/pbs record for the given parameters
Input Parameters:
telescope Telescope name
antennatype The antenna type as a string, e.g. 'DV'
obstime Time of the observation (for versioning and reference frame calculations), e.g. 2011/12/12T00:00:00
freq Frequency of the observation (may include reference frame, default: LSRK)
obsdirection Direction of the observation (may include reference frame, default: J2000), default: AZEL 0deg 90deg
--------------------------------------------------------------------------------Definition at line 464 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.loadfromtable | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
loadfromtable(self, tablename=string("")) -> bool
Summary
Load the vp or pb descriptions from a table (deleting all previous definitions)
Input Parameters:
tablename Name of table to load vp descriptions from
--------------------------------------------------------------------------------Definition at line 110 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.numvps | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
numvps(self, telescope=string(""), obstime=initialize_variant(""), freq=initialize_variant(""),
obsdirection=initialize_variant("AZEL 0deg 90deg")) -> int
Summary
Return the number of vps/pbs available for the given parameters
Input Parameters:
telescope Telescope name
obstime Time of the observation (for versioning and reference frame calculations)
freq Frequency of the observation (may include reference frame, default: LSRK)
obsdirection Direction of the observation (may include reference frame, default: J2000). default: Zenith AZEL 0deg 90deg
--------------------------------------------------------------------------------Definition at line 445 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.release | ( | self | ) |
release(self) Summary Release the VPManager for use by others. --------------------------------------------------------------------------------
Definition at line 84 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.reset | ( | self | ) |
reset(self) -> bool Summary Reinitialize the VPManager (will erase all VPs and defaults defined on the command line) --------------------------------------------------------------------------------
Definition at line 382 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.saveastable | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
saveastable(self, tablename=string("")) -> bool
Summary
Save the vp or pb descriptions as a table
Input Parameters:
tablename Name of table to save vp descriptions in
--------------------------------------------------------------------------------Definition at line 95 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setcannedpb | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setcannedpb(self, telescope=string("VLA"), othertelescope=string(""), dopb=True, commonpb=string("DEFAULT"),
dosquint=False, paincrement=initialize_variant("720deg"), usesymmetricbeam=False) -> record *
Summary
Select a vp/pb from our library of common pb models
Input Parameters:
telescope Which telescope in the MS will use this vp/pb? VLA
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
commonpb List of common vp/pb models: DEFAULT code figures it out DEFAULT
dosquint Enable the natural beam squint found in the common vp model false
paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application 720deg
usesymmetricbeam Not currently used false
--------------------------------------------------------------------------------Definition at line 140 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setpbairy | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setpbairy(self, telescope=string("VLA"), othertelescope=string(""), dopb=True, dishdiam=initialize_variant("25.0m"),
blockagediam=initialize_variant("2.5m"), maxrad=initialize_variant("0.8deg"),
reffreq=initialize_variant("1.0GHz"), squintdir=initialize_variant(""),
squintreffreq=initialize_variant("1.0GHz"), dosquint=False,
paincrement=initialize_variant("720deg"), usesymmetricbeam=False) -> record *
Summary
Make an airy disk vp
Input Parameters:
telescope Which telescope in the MS will use this vp/pb? VLA
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
dishdiam Effective diameter of dish 25.0m
blockagediam Effective diameter of subreflector blockage 2.5m
maxrad Maximum radial extent of the vp/pb (scales with 1/freq) 0.8deg
reffreq Frequency at which maxrad is specified 1.0GHz
squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
squintreffreq Frequency at which the squint is specified 1.0GHz
dosquint Enable the natural beam squint found in the common vp model false
paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application 720deg
usesymmetricbeam Not currently used false
--------------------------------------------------------------------------------Definition at line 162 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setpbantresptable | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setpbantresptable(self, telescope=string(""), othertelescope=string(""), dopb=True, antresppath=string("")) -> bool
Summary
Declare a reference to an antenna responses table
Input Parameters:
telescope Which telescope in the MS will use this vp/pb?
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
antresppath The path to the antenna responses table (absolute or relative to CASA data dir.)
--------------------------------------------------------------------------------Definition at line 364 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setpbcospoly | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setpbcospoly(self, telescope=string("VLA"), othertelescope=string(""), dopb=True, coeff=initialize_vector(1, (double)-1),
scale=initialize_vector(1, (double)-1), maxrad=initialize_variant("0.8deg"),
reffreq=initialize_variant("1.0GHz"), isthispb=string("PB"),
squintdir=initialize_variant(""), squintreffreq=initialize_variant("1.0GHz"),
dosquint=False, paincrement=initialize_variant("720deg"), usesymmetricbeam=False) -> record *
Summary
Make a vp/pb from a polynomial of scaled cosines
Input Parameters:
telescope Which telescope in the MS will use this vp/pb? VLA
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
coeff Vector of coefficients of cosines -1
scale Vector of scale factors of cosines -1
maxrad Maximum radial extent of the vp/pb (scales with 1/freq) 0.8deg
reffreq Frequency at which maxrad is specified 1.0GHz
isthispb Do these parameters describe a PB or a VP? PB
squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
squintreffreq Frequency at which the squint is specified 1.0GHz
dosquint Enable the natural beam squint found in the common vp model false
paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application 720deg
usesymmetricbeam Not currently used false
--------------------------------------------------------------------------------Definition at line 192 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setpbgauss | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setpbgauss(self, telescope=string("VLA"), othertelescope=string(""), dopb=True, halfwidth=initialize_variant("0.5deg"),
maxrad=initialize_variant("1.0deg"), reffreq=initialize_variant("1.0GHz"),
isthispb=string("PB"), squintdir=initialize_variant(""),
squintreffreq=initialize_variant("1.0GHz"), dosquint=False, paincrement=initialize_variant("720deg"),
usesymmetricbeam=False) -> record *
Summary
Make a Gaussian vp/pb
Input Parameters:
telescope Which telescope in the MS will use this vp/pb? VLA
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
halfwidth Half power half width of the Gaussian at the reffreq 0.5deg
maxrad Maximum radial extent of the vp/pb (scales with 1/freq) 1.0deg
reffreq Frequency at which maxrad is specified 1.0GHz
isthispb Do these parameters describe a PB or a VP? PB
squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
squintreffreq Frequency at which the squint is specified 1.0GHz
dosquint Enable the natural beam squint found in the common vp model false
paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application 720deg
usesymmetricbeam Not currently used false
--------------------------------------------------------------------------------Definition at line 223 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setpbimage | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setpbimage(self, telescope=string("VLA"), othertelescope=string(""), dopb=True, realimage=string(""),
imagimage=string(""), compleximage=string("")) -> record *
Summary
Make a vp/pb from a user-supplied image
Input Parameters:
telescope Which telescope in the MS will use this vp/pb? VLA
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
realimage Real part of vp as an image
imagimage Imaginary part of vp as an image
compleximage complex vp as an image of complex numbers; if specified realimage and imagimage are ignored
--------------------------------------------------------------------------------Definition at line 313 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setpbinvpoly | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setpbinvpoly(self, telescope=string("VLA"), othertelescope=string(""), dopb=True, coeff=initialize_vector(1, (double)-1),
maxrad=initialize_variant("0.8deg"), reffreq=initialize_variant("1.0GHz"),
isthispb=string("PB"), squintdir=initialize_variant(""),
squintreffreq=initialize_variant("1.0"), dosquint=False, paincrement=initialize_variant("720deg"),
usesymmetricbeam=False) -> record *
Summary
Make a vp/pb as an inverse polynomial
Input Parameters:
telescope Which telescope in the MS will use this vp/pb? VLA
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
coeff Coefficients of even powered terms -1
maxrad Maximum radial extent of the vp/pb (scales with 1/freq) 0.8deg
reffreq Frequency at which maxrad is specified 1.0GHz
isthispb Do these parameters describe a PB or a VP? PB
squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
squintreffreq Frequency at which the squint is specified 1.0
dosquint Enable the natural beam squint found in the common vp model false
paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application 720deg
usesymmetricbeam Not currently used false
--------------------------------------------------------------------------------Definition at line 253 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setpbnumeric | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setpbnumeric(self, telescope=string("VLA"), othertelescope=string(""), dopb=True, vect=initialize_vector(1, (double)-1),
maxrad=initialize_variant("0.8deg"), reffreq=initialize_variant("1.0GHz"),
isthispb=string("PB"), squintdir=initialize_variant(""),
squintreffreq=initialize_variant("1.0GHz"), dosquint=False, paincrement=initialize_variant("720deg"),
usesymmetricbeam=False) -> record *
Summary
Make a vp/pb from a user-supplied vector
Input Parameters:
telescope Which telescope in the MS will use this vp/pb? VLA
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
vect Vector of vp/pb samples uniformly spaced from 0 to maxrad -1
maxrad Maximum radial extent of the vp/pb (scales with 1/freq) 0.8deg
reffreq Frequency at which maxrad is specified 1.0GHz
isthispb Do these parameters describe a PB or a VP? PB
squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
squintreffreq Frequency at which the squint is specified 1.0GHz
dosquint Enable the natural beam squint found in the common vp model false
paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application 720deg
usesymmetricbeam Not currently used false
--------------------------------------------------------------------------------Definition at line 283 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setpbpoly | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setpbpoly(self, telescope=string("VLA"), othertelescope=string(""), dopb=True, coeff=initialize_vector(1, (double)-1),
maxrad=initialize_variant("0.8deg"), reffreq=initialize_variant("1.0GHz"),
isthispb=string("PB"), squintdir=initialize_variant(""),
squintreffreq=initialize_variant("1.0GHz"), dosquint=False, paincrement=initialize_variant("720"),
usesymmetricbeam=False) -> record *
Summary
Make a vp/pb from a polynomial
Input Parameters:
telescope Which telescope in the MS will use this vp/pb? VLA
othertelescope If telescope=='OTHER', specify name here
dopb Should we apply the vp/pb to this telescope's data? true
coeff Coefficients of even powered terms -1
maxrad Maximum radial extent of the vp/pb (scales with 1/freq) 0.8deg
reffreq Frequency at which maxrad is specified 1.0GHz
isthispb Do these parameters describe a PB or a VP? PB
squintdir Offset (Measure) of RR beam from pointing center, azel frame (scales with 1/freq)
squintreffreq Frequency at which the squint is specified 1.0GHz
dosquint Enable the natural beam squint found in the common vp model false
paincrement Increment in Parallactic Angle for asymmetric (ie, squinted) vp application 720
usesymmetricbeam Not currently used false
--------------------------------------------------------------------------------Definition at line 334 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.setuserdefault | ( | self, | |
| args, | |||
| kwargs | |||
| ) |
setuserdefault(self, vplistnum=-1, telescope=string(""), anttype=string("")) -> bool
Summary
Select the VP which is to be used by the imager for the given telescope and antenna type
Input Parameters:
vplistnum The number of the vp as displayed by summarizevps(), or -1 for internal default, or -2 for unset -1
telescope Which telescope in the MS will use this vp/pb?
anttype Which antennatype will use this vp/pb? Default: '' = all
--------------------------------------------------------------------------------Definition at line 393 of file vpmanager.py.
| def __casac__.vpmanager.vpmanager.summarizevps | ( | self, | |
verbose = False |
|||
| ) |
summarizevps(self, verbose=False) -> bool Summary Summarize the currently accumulated VP descriptions Input Parameters: verbose Print out full record? Otherwise, print summary. false --------------------------------------------------------------------------------
Definition at line 125 of file vpmanager.py.
__casac__.vpmanager.vpmanager.__del__ [static, private] |
Definition at line 83 of file vpmanager.py.
tuple __casac__.vpmanager.vpmanager.__getattr__ [static, private] |
Definition at line 75 of file vpmanager.py.
__casac__.vpmanager.vpmanager.__repr__ [static, private] |
Definition at line 76 of file vpmanager.py.
tuple __casac__.vpmanager.vpmanager.__setattr__ [static, private] |
Definition at line 73 of file vpmanager.py.
__casac__.vpmanager.vpmanager.__swig_destroy__ [static, private] |
Definition at line 82 of file vpmanager.py.
dictionary __casac__.vpmanager.vpmanager.__swig_getmethods__ [static, private] |
Definition at line 74 of file vpmanager.py.
dictionary __casac__.vpmanager.vpmanager.__swig_setmethods__ [static, private] |
Definition at line 72 of file vpmanager.py.
Definition at line 81 of file vpmanager.py.
1.8.0