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NRAO Home > CASA > CASA Toolkit Reference Manual |
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ms.cvel - Function
1.3.1 transform spectral data to different reference frame and/or regrid the frequency
channels
Description
This function permits you to transform the spectral data of your measurement
set to a given reference frame and/or regrid it. It will combine all spectral
windows of the MS into one.
Arguments
Inputs |
| ||
mode |
| ”channel”, ”velocity”, ”frequency”, or ”channel_b”,
default = ”channel” | |
| allowed: | string |
|
| Default: | channel | |
nchan |
| number of channels, default = -1 = all
| |
| allowed: | int | |
| Default: | -1 |
|
start |
| start channel, default = 0
| |
| allowed: | any |
|
| Default: | variant 0 | |
width |
| new channel width, default = 1
| |
| allowed: | any |
|
| Default: | variant 1 | |
interp |
| interpolation method ”nearest”, ”linear”, ”spline”,
”cubic”, ”fftshift”, default = linear
| |
| allowed: | string |
|
| Default: | linear | |
phasec |
| phase center, default = first field
| |
| allowed: | any |
|
| Default: | variant
|
|
restfreq |
| rest frequency, default = 1.4GHz
| |
| allowed: | any |
|
| Default: | variant 1.4GHz |
|
outframe |
| LSRK, LSRD, BARY, GALACTO, LGROUP, CMB,
GEO, TOPO, or SOURCE default = ”” = keep reference
frame.
| |
| allowed: | string |
|
| Default: |
|
|
veltype |
| radio or optical, default = radio
| |
| allowed: | string |
|
| Default: | radio |
|
hanning |
| If true, perform hanning smoothing before regridding.
| |
| allowed: | bool |
|
| Default: | true |
|
bool
Example
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Copyright © 2016 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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