oldsplit – Create a visibility subset from an existing visibility set – manipulation task

Description

T H I S T A S K I S D E P R E C A T E D I T W I L L B E R E M O V E D S O O N

Oldsplit is the general purpose program to make a new data set that is a subset or averaged form of an existing data set. General selection parameters are included, and one or all of the various data columns (DATA, LAG_DATA and/or FLOAT_DATA, and possibly MODEL_DATA and/or CORRECTED_DATA) can be selected.

Oldsplit is often used after the initial calibration of the data to make a smaller measurement set with only the data that will be used in further flagging, imaging and/or self-calibration. Oldsplit can average over frequency (channels) and time (integrations).

Parameters

Title

Parameter

Default

Description

vis

''

outputvis

''

datacolumn

'corrected'

field

''

spw

''

width

int(1)

antenna

''

timebin

'0s'

timerange

''

scan

''

intent

''

array

''

uvrange

''

correlation

''

observation

''

combine

''

keepflags

True

keepmms

False

Parameter Explanations

vis

''

Name of input measurement set

outputvis

''

Name of output measurement set

datacolumn

'corrected'

Which data column(s) to Oldsplit out

field

''

Select field using ID(s) or name(s)

spw

''

Select spectral window/channels

width

int(1)

Number of channels to average to form one output channel

antenna

''

Select data based on antenna/baseline

timebin

'0s'

Bin width for time averaging

timerange

''

Select data by time range

scan

''

Select data by scan numbers

intent

''

Select data by scan intents

array

''

Select (sub)array(s) by array ID number

uvrange

''

Select data by baseline length

correlation

''

Select correlations

observation

''

Select by observation ID(s)

combine

''

Let time bins span changes in scan and/or state

keepflags

True

If practical, keep completely flagged rows instead of dropping them.

keepmms

False

If the input is a multi-MS, make the output one, too. (experimental)