pipeline.hifv.cli.gotasks.hifv_fluxboot2

pipeline.hifv.cli.gotasks.hifv_fluxboot2 = <pipeline.hifv.cli.gotasks.hifv_fluxboot2._hifv_fluxboot2 object>

hifv_fluxboot2 —- Fluxboot2

——— parameter descriptions ———————————————

vis List of visibility data files. These may be ASDMs, tar files of ASDMs,

MSes, or tar files of MSes, If ASDM files are specified, they will be converted to MS format. example: vis=[‘X227.ms’, ‘asdms.tar.gz’]

caltable String name of the flagged caltable fitorder Polynomial order of the spectral fitting for valid flux densities

with multiple spws. The default value of -1 means that the heuristics determine the fit order based on fractional bandwidth and receiver bands present in the observation. An override value of 0,1,2,3 or 4 may be specified by the user. Spectral index (1) and, if applicable, curvature (2) are reported in the weblog. If no determination can be made by the heuristics, a fitorder of 1 will be used.

pipelinemode The pipeline operating mode. In ‘automatic’ mode the pipeline

determines the values of all context defined pipeline inputs automatically. In ‘interactive’ mode the user can set the pipeline context defined parameters manually. In ‘getinputs’ mode the user can check the settings of all pipeline parameters without running the task.

dryrun Run the commands (True) or generate the commands to be run but

do not execute (False). This is a pipeline task execution mode.

acceptresults Add the results of the task to the pipeline context (True) or

reject them (False). This is a pipeline task execution mode.

refantignore String list of antennas to ignore

Example: refantignore=’ea02,ea03’

——— examples ———————————————————–

Output:

results – If pipeline mode is ‘getinputs’ then None is returned. Otherwise the results object for the pipeline task is returned.

Examples

1. VLA CASA pipeline flux density bootstrapping.

hifv_fluxboot2()