Imaging an EVLA OSRO HI data set: Difference between revisions

From CASA Guides
Jump to navigationJump to search
No edit summary
Line 18: Line 18:


== Doppler Track ==  
== Doppler Track ==  
<pre>
#  cvel :: regrid an MS to a new spectral window / channel structure or frame
vis                =  'leo1.ms'        #  Name of input measurement set
outputvis          = 'leob1.ms'        #  Name of output measurement set
passall            =      False        #  Pass through (write to output MS) non-selected data with no
                                        #  change
field              =        ''        #  Select field using field id(s) or field name(s)
spw                =        ''        #  Select spectral window/channels
selectdata          =      False        #  Other data selection parameters
mode                =  'channel'        #  Regridding mode
    nchan          =        -1        #  Number of channels in output spw (-1=all)
    start          =          0        #  first input channel to use
    width          =          1        #  Number of input channels to average
    interpolation  =  'nearest'        #  Spectral interpolation method


phasecenter        =        ''        #  Image phase center: position or field index
restfreq            = '1420405751.786Hz' #  rest frequency (see help)
outframe            =    'BARY'        #  Output frame (''=keep input frame)
veltype            =    'radio'        #  velocity definition
hanning            =      False        #  Turn on Hanning smoothing of spectral channels
async              =      False        #  If true the taskname must be started using cvel(...)
</pre>
output:
<pre>
2010-02-15 01:31:51 INFO cvel ##########################################
2010-02-15 01:31:51 INFO cvel ##### Begin Task: cvel              #####
2010-02-15 01:31:51 INFO  cvel::::casa
2010-02-15 01:31:51 INFO cvel vis="leo1.ms", outputvis="leob1.ms", passall="False", field="", spw=, antenna="", timerange="",
2010-02-15 01:31:51 INFO cvel mode=channel, nchan=-1, start=0, width=1, interpolation = nearest, outframe="BARY",
2010-02-15 01:31:51 INFO cvel phasecenter="", restfreq="1420405751.786Hz", veltype="radio", hanning="False"
2010-02-15 01:31:51 INFO cvel Creating SubMS with time-sorted main table ...
2010-02-15 01:31:54 INFO ms Sorted main table of /export/home/rso-lchomiuk/test/Leo/leo1.ms by TIME and stored it in leob1.ms .
2010-02-15 01:31:55 INFO cvel Using Leo-1 (original field 0, new field 0) as phase center.
2010-02-15 01:31:55 INFO ms Starting combination of spectral windows ...
2010-02-15 01:31:55 INFO SubMS Less than two SPWs selected. No combination necessary.
2010-02-15 01:31:55 INFO ms
2010-02-15 01:31:55 INFO ms Testing if spectral frame transformation/regridding is needed ...
2010-02-15 01:31:55 INFO SubMS Regridded spectral window 0 will be created for field 0 with parameters
2010-02-15 01:31:55 INFO SubMS input frame = TOPO, output frame = BARY
2010-02-15 01:31:55 INFO SubMS Channels equidistant in freq
2010-02-15 01:31:55 INFO SubMS Central frequency (in output frame) = 1.41632e+09 Hz
2010-02-15 01:31:55 INFO SubMS Width of central channel (in output frame) = 7811.76 Hz
2010-02-15 01:31:55 INFO SubMS Number of channels = 226
2010-02-15 01:31:55 INFO SubMS Total width of SPW (in output frame) = 1.76546e+06 Hz
2010-02-15 01:31:55 INFO SubMS Lower edge = 1.41543e+09 Hz, upper edge = 1.4172e+09 Hz
2010-02-15 01:31:55 INFO SubMS Interpolation Method = nearestNeighbour
2010-02-15 01:31:55 INFO SubMS Added 1 new rows to the DATA_DESCRIPTION table and deleted 1 old ones.
2010-02-15 01:31:55 INFO SubMS Added 1 rows to the SPECTRAL_WINDOW table and deleted 1 old ones.
2010-02-15 01:31:55 INFO SubMS Added 1 rows to the SOURCE table and deleted 1 old ones.
2010-02-15 01:31:55 INFO SubMS Main table data array columns will be rewritten ...
2010-02-15 01:32:34 INFO ms Spectral frame transformation/regridding completed.
2010-02-15 01:32:34 INFO ms Final spectral window has 226 channels of width 7.811764e+03 Hz
2010-02-15 01:32:34 INFO ms First channel center = 1.41544e+09 Hz, last channel center = 1.4172e+09 Hz
2010-02-15 01:32:35 INFO  cvel::::casa
2010-02-15 01:32:35 INFO cvel ##### End Task: cvel                #####
2010-02-15 01:32:35 INFO cvel ##########################################
</pre>




[[Main Page | &#8629; '''CASA Guides''']]
[[Main Page | &#8629; '''CASA Guides''']]

Revision as of 21:33, 14 February 2010

Overview

This tutorial explains how to image an HI dataset acquired with the WIDAR0 correlator. It assumes that you've already calibrated your data as described in the calibration tutorial, and that you now have a split dataset with a single source of interest in it. In this example, the source is called 'Leo-1'; see the calibration tutorial for more details on this data set.

Flag Your Split Data

Load the split dataset into plotms and/or viewer and flag any bad data.

Data flagging with viewer

Data flagging with plotms

For a spectral line dataset like this one, you'll probably want to average in various ways to spot bad data. Averaging channels together can make bad baselines pop up!

Continuum Subtraction

???

Doppler Track

#  cvel :: regrid an MS to a new spectral window / channel structure or frame
vis                 =  'leo1.ms'        #  Name of input measurement set
outputvis           = 'leob1.ms'        #  Name of output measurement set
passall             =      False        #  Pass through (write to output MS) non-selected data with no
                                        #   change
field               =         ''        #  Select field using field id(s) or field name(s)
spw                 =         ''        #  Select spectral window/channels
selectdata          =      False        #  Other data selection parameters
mode                =  'channel'        #   Regridding mode
     nchan          =         -1        #  Number of channels in output spw (-1=all)
     start          =          0        #  first input channel to use
     width          =          1        #  Number of input channels to average
     interpolation  =  'nearest'        #  Spectral interpolation method

phasecenter         =         ''        #  Image phase center: position or field index
restfreq            = '1420405751.786Hz' #  rest frequency (see help)
outframe            =     'BARY'        #  Output frame (''=keep input frame)
veltype             =    'radio'        #  velocity definition
hanning             =      False        #  Turn on Hanning smoothing of spectral channels
async               =      False        #  If true the taskname must be started using cvel(...)

output:

2010-02-15 01:31:51 INFO cvel	##########################################
2010-02-15 01:31:51 INFO cvel	##### Begin Task: cvel               #####
2010-02-15 01:31:51 INFO  	cvel::::casa
2010-02-15 01:31:51 INFO cvel	vis="leo1.ms", outputvis="leob1.ms", passall="False", field="", spw=, antenna="", timerange="",
2010-02-15 01:31:51 INFO cvel	mode=channel, nchan=-1, start=0, width=1, interpolation = nearest, outframe="BARY",
2010-02-15 01:31:51 INFO cvel	phasecenter="", restfreq="1420405751.786Hz", veltype="radio", hanning="False"
2010-02-15 01:31:51 INFO cvel	Creating SubMS with time-sorted main table ...
2010-02-15 01:31:54 INFO ms	Sorted main table of /export/home/rso-lchomiuk/test/Leo/leo1.ms by TIME and stored it in leob1.ms .
2010-02-15 01:31:55 INFO cvel	Using Leo-1 (original field 0, new field 0) as phase center.
2010-02-15 01:31:55 INFO ms	Starting combination of spectral windows ...
2010-02-15 01:31:55 INFO SubMS	Less than two SPWs selected. No combination necessary.
2010-02-15 01:31:55 INFO ms	 
2010-02-15 01:31:55 INFO ms	Testing if spectral frame transformation/regridding is needed ...
2010-02-15 01:31:55 INFO SubMS	Regridded spectral window 0 will be created for field 0 with parameters 
2010-02-15 01:31:55 INFO SubMS	input frame = TOPO, output frame = BARY
2010-02-15 01:31:55 INFO SubMS	 Channels equidistant in freq
2010-02-15 01:31:55 INFO SubMS	 Central frequency (in output frame) = 1.41632e+09 Hz
2010-02-15 01:31:55 INFO SubMS	 Width of central channel (in output frame) = 7811.76 Hz
2010-02-15 01:31:55 INFO SubMS	 Number of channels = 226
2010-02-15 01:31:55 INFO SubMS	 Total width of SPW (in output frame) = 1.76546e+06 Hz
2010-02-15 01:31:55 INFO SubMS	 Lower edge = 1.41543e+09 Hz, upper edge = 1.4172e+09 Hz
2010-02-15 01:31:55 INFO SubMS	 Interpolation Method = nearestNeighbour
2010-02-15 01:31:55 INFO SubMS	Added 1 new rows to the DATA_DESCRIPTION table and deleted 1 old ones.
2010-02-15 01:31:55 INFO SubMS	Added 1 rows to the SPECTRAL_WINDOW table and deleted 1 old ones.
2010-02-15 01:31:55 INFO SubMS	Added 1 rows to the SOURCE table and deleted 1 old ones.
2010-02-15 01:31:55 INFO SubMS	Main table data array columns will be rewritten ...
2010-02-15 01:32:34 INFO ms	Spectral frame transformation/regridding completed.
2010-02-15 01:32:34 INFO ms	Final spectral window has 226 channels of width 7.811764e+03 Hz
2010-02-15 01:32:34 INFO ms	First channel center = 1.41544e+09 Hz, last channel center = 1.4172e+09 Hz
2010-02-15 01:32:35 INFO  	cvel::::casa
2010-02-15 01:32:35 INFO cvel	##### End Task: cvel                 #####
2010-02-15 01:32:35 INFO cvel	##########################################


CASA Guides