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Variables
ngc4826_demo Namespace Reference

Variables

tuple pathname
 miriad: source Vlsr = 408; delta is 20 km/s
string datapath
string prefix
string msfile
tuple startTime
tuple startProc
string copystring16apr
 16 APR Calibration
tuple copy2time
tuple setjy2time
 List contents of MS.
tuple flagdata2time
 Flag end channels.
string gcaltable
 Derive gain calibration solutions, try VLA-like calibration:
string field
 Correct the calibrater/target source data: Use new parm spwmap to apply gain solutions derived from spwid1 to all other spwids...
float minsnr
string refant
tuple gaincal2time
string fcaltable
 Transfer the flux density scale:
 fluxtable
string reference
tuple fluxscale2time
float gaincurve
tuple correct2time
string calsplitms
 Split out calibrated target source and calibrater data:
string srcsplitms
string datacolumn
tuple split2time
string antenna
 Extra flagging.
string clipexpr
list clipminmax
 clipoutside
string timerange
 unflag
string calimage
 Image the calibrater data:
list cell
string psfmode
string calclnimage
tuple imagecal2time
string srcimage
 Image the target source mosaic:
int nchan
string spw
string stokes
string srcclnimage
string momfile
 Do first and second moments.
string momzeroimage
string momoneimage
int moments
string planes
tuple endProc
tuple endTime
tuple thistest_cal_16apr
 Regression 16 APR.
tuple thistest_src_16apr
tuple calstat
list im_calmax16
tuple srcstat
list im_srcmax16
string offbox
tuple offstat
list im_offrms16
tuple momzerostat
list thistest_immax
list thistest_imrms
float calmean16
 Previous regression values.
float srcmean16
float srcmax16
float calmax16
float immax
float imrms
float offrms16
tuple diff_cal16apr
tuple diff_src16apr
tuple diff_calmax16
tuple diff_srcmax16
tuple diff_immax
tuple diff_imrms
tuple diff_offrms16
string calvis_status
string srcvis_status
string calmax_status
string srcmax_status
string mom0max_status
string mom0rms_status
string offrms_status
tuple datestring
string outfile
tuple logfile
 regstate

Variable Documentation

Extra flagging.

Definition at line 215 of file ngc4826_demo.py.

Definition at line 238 of file ngc4826_demo.py.

Image the calibrater data:

Definition at line 231 of file ngc4826_demo.py.

Definition at line 345 of file ngc4826_demo.py.

Definition at line 381 of file ngc4826_demo.py.

Previous regression values.

Definition at line 342 of file ngc4826_demo.py.

Split out calibrated target source and calibrater data:

Definition at line 191 of file ngc4826_demo.py.

Definition at line 308 of file ngc4826_demo.py.

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Definition at line 89 of file ngc4826_demo.py.

16 APR Calibration

Concatenate the separate sources

Definition at line 81 of file ngc4826_demo.py.

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Definition at line 286 of file ngc4826_demo.py.

Definition at line 287 of file ngc4826_demo.py.

Transfer the flux density scale:

Definition at line 150 of file ngc4826_demo.py.

Correct the calibrater/target source data: Use new parm spwmap to apply gain solutions derived from spwid1 to all other spwids...

Definition at line 134 of file ngc4826_demo.py.

Flag end channels.

Definition at line 121 of file ngc4826_demo.py.

Definition at line 156 of file ngc4826_demo.py.

Definition at line 153 of file ngc4826_demo.py.

Definition at line 138 of file ngc4826_demo.py.

Definition at line 175 of file ngc4826_demo.py.

Derive gain calibration solutions, try VLA-like calibration:

Definition at line 131 of file ngc4826_demo.py.

Definition at line 310 of file ngc4826_demo.py.

Definition at line 319 of file ngc4826_demo.py.

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Definition at line 390 of file ngc4826_demo.py.

Definition at line 279 of file ngc4826_demo.py.

Do first and second moments.

miriad:source velocity is 408; delta is 20 km/s; 24 maps

Definition at line 274 of file ngc4826_demo.py.

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Definition at line 402 of file ngc4826_demo.py.

miriad: source Vlsr = 408; delta is 20 km/s

     Mosaic field spacing looks like:

     F3 (fieldid 4)         F2 (fieldid 3)

F4 (fieldid 5) F0 (fieldid 1) F1 (fieldid 2)

   F5 (fieldid 6)         F6 (fieldid 7)

4x64 channels = 256 channels

Primary Beam should be about 1.6' FWHM (7m dishes, 2.7mm wavelength) Resolution should be about 5-8"

                                                                   #

Set up some variables for control

Definition at line 53 of file ngc4826_demo.py.

Definition at line 280 of file ngc4826_demo.py.

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Definition at line 154 of file ngc4826_demo.py.

Definition at line 436 of file ngc4826_demo.py.

List contents of MS.

Set the flux density of 3C273 to 23 Jy

Definition at line 109 of file ngc4826_demo.py.

Definition at line 204 of file ngc4826_demo.py.

Definition at line 257 of file ngc4826_demo.py.

Definition at line 262 of file ngc4826_demo.py.

Image the target source mosaic:

mosaic data ...Sault weighting implies a noise unform image hence flux scale across image needed to be corrected to get right value

Definition at line 253 of file ngc4826_demo.py.

Definition at line 344 of file ngc4826_demo.py.

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Definition at line 259 of file ngc4826_demo.py.

Regression 16 APR.

Definition at line 299 of file ngc4826_demo.py.

Definition at line 326 of file ngc4826_demo.py.

Definition at line 327 of file ngc4826_demo.py.

Definition at line 302 of file ngc4826_demo.py.

Definition at line 219 of file ngc4826_demo.py.

Definition at line 220 of file ngc4826_demo.py.