calibrater.setsolve2 - Function

2.2.1 Arrange to solve for calibration
Description

TBD.

Arguments





Inputs

type

Component type

allowed:

string

Default:

G T B D M MF

t

Solution interval (units optional)

allowed:

any

Default:

variant

table

Output calibration table name

allowed:

string

Default:

append

Append to existing table?

allowed:

bool

Default:

false

preavg

Pre-averaging interval (in sec)

allowed:

double

Default:

-1.0

phaseonly

Solve only for phase?

allowed:

bool

Default:

false

apmode

Solve for ’AP’, ’A’ (amp-only) or ’P’ (phase-only)

allowed:

string

Default:

AP

refant

Reference antenna. Default is none.

allowed:

any

Default:

variant

solnorm

Normalize solution after solve

allowed:

bool

Default:

false

minsnr

SNR threshold for accepting solutions

allowed:

float

Default:

0.0

combine

Data axes on which to combine solving (scan, spw, and/or field)

allowed:

string

Default:

cfcache

Name of the directory to be used for convolution function disk cache. This is used when type=EP.

allowed:

string

Default:

painc

Parallactic Angle increment used to trigger computation of a new convolution function. This is used when type=EP. Default value implies that only one convolution function will be computed for the entire range of observation.

allowed:

float

Default:

360.0

Returns
bool

Example

TBD.

Please send any comments or questions about CASA or AIPS++ to aips2-requests@nrao.edu

Copyright © 2008 Associated Universities Inc., Washington, D.C.

This code is available under the terms of the GNU General Public Lincense


Home | Contact Us | Directories | Site Map | Help | Privacy Policy | Search

Updated daily during alpha development.