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  • 0 0 Direction Right Ascension SIN 300 60 09:47:57.382 150.00 -4. 1 0 Direction Declination SIN 300 60 +13.16.40.660 150.00 4.
    3 KB (383 words) - 18:16, 9 November 2010
  • ...and a tilde denotes a range. NOTE: all index numbering in CASA begins with 0, not 1! spw = '0~3' # Spectral windows 0, 1, 2, and 3
    2 KB (296 words) - 15:42, 20 August 2012
  • xrange=[0, 0], yrange=[0, 0], figfile='', help=False, antenna: can be ID or name; single value, or list: 0,'0','0,1','DV04,DV05'.
    2 KB (343 words) - 09:51, 6 April 2017
  • for element in range (0,64): fldNames[0] = '3C147'
    1 KB (242 words) - 16:23, 29 July 2013
  • ...9; border: 1px solid #aaaaaa; margin: 0.2em 10px 10px; padding:0.2em 0.4em; text-align: center; font-size: 125%"> {| role="presentation" style="border:0; margin: 0; width: 100%; border-spacing: 10px;"
    4 KB (447 words) - 18:34, 7 March 2017
  • ...Simulating Observations in CASA v3.0.1 | Simulating Observations in CASA 3.0]] ...ting_Observations_in_CASA_3.1#ALMA_Early_Science_Configurations ALMA Cycle 0 Configurations]
    269 bytes (31 words) - 12:17, 2 May 2011
  • ...Simulating Observations in CASA v3.0.1 | Simulating Observations in CASA 3.0]] ...ting_Observations_in_CASA_3.1#ALMA_Early_Science_Configurations ALMA Cycle 0 Configurations]
    300 bytes (33 words) - 17:35, 26 April 2011
  • In the ALMA archive for Cycle 0 data, the packaged calibration script found in the ''scripts'' directory is step_title = {0: 'Import of the ASDM',
    6 KB (878 words) - 16:46, 29 March 2017
  • File:604px-Antennae galaxies xl.jpg
    ...clusters are formed. The contours show the molecular gas as traced by CO(1-0). Credit: NASA, ESA, and the Hubble Heritage Team STScI/AURA - ESA/Hubble C
    (881 × 879 (152 KB)) - 10:21, 5 August 2011
  • | startrowin: First row to take from input table 0 | startrowin = 0
    28 KB (3,381 words) - 16:35, 18 May 2015
  • Ignoring spectral window [0, 25, 26, 27, 28, 29, 30, 31, 32, 33] because it is WVR related Latency removed: Total time = 60.0 min, science time = 40.1 min
    5 KB (603 words) - 17:10, 11 July 2013
  • ...um data (from the dirty image) and for spectral line data (from the moment 0 map of the dirty line cube). ...e a spectral line and/or continuum "dirty map" by calling CLEAN with niter=0. This is the starting point for CLEAN, and the starting point for defining
    3 KB (544 words) - 11:41, 9 July 2015
  • ...6:32 INFO listsdm 12:27:08.17 - 12:28:05.36 1 0 J2038+5119 [0, 1] CALIBRATE_PHASE 2011-01-02 02:26:32 INFO listsdm 12:28:05.36 - 12:29:05.20 2 0 J2038+5119 [2, 3] CALIBRATE_PHASE
    9 KB (771 words) - 01:46, 16 March 2012
  • box = '0,0,299,299'
    2 KB (267 words) - 16:41, 29 March 2017
  • Antenna 0 = DV04 on pad J505, lat/long offset (m) = -7.2138/ -488.2036 Antenna 2 = DV07 on pad J510, lat/long offset (m) = -0.3652/ -512.3043
    3 KB (499 words) - 16:45, 4 January 2012
  • ..., CASA does it in one step. If you want a dirty image, just set ''niter''=0 so that [[clean]] doesn't actually do any...cleaning. minpb=0.2,pbcor=True,
    5 KB (806 words) - 13:38, 29 April 2010

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