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  • au.plotPWV(ms, figfile='', plotrange=[0, 0, 0, 0], clip=True) plotrange: the ranges for the X and Y axes (default=[0,0,0,0] which is autorange)
    1 KB (208 words) - 13:17, 14 April 2014
  • {'blc': array([0, 0, 0, 0], dtype=int32), 'max': array([ 0.10524261]),
    2 KB (199 words) - 17:52, 7 June 2010
  • #REDIRECT [[Guide To Processing ALMA Data for Cycle 0]]
    55 bytes (8 words) - 18:26, 15 April 2014
  • #REDIRECT [[Guide To Redo Calibration For ALMA Cycle 0]]
    56 bytes (8 words) - 14:29, 21 April 2014
  • Summary 0 ( Zeros ) : Flagged : 274944.0 out of 549888.0 Summary 1 ( TFCrop ) : Flagged : 18633.0 out of 549888.0
    1 KB (146 words) - 10:19, 28 March 2012
  • Avoided 201 flagged channels on pol=0, spw=0, antenna=0 Avoided 201 flagged channels on pol=1, spw=0, antenna=0
    2 KB (354 words) - 17:25, 13 November 2012
  • 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
  • | 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
  • CASA <49>: print os.getenv('CASAPATH').split(' ')[0] + '/data/alma/simmos/' | alma.cycle0.compact.cfg || ALMA Cycle 0 compact config
    10 KB (1,677 words) - 13:14, 7 July 2015
  • == How To Redo ALMA Calibration for Cycle 0 Data Packages == ...a Concatenation]] in the [[Guide_To_Processing_ALMA_Data_for_Cycle_0|Cycle 0 Data Processing Guide]].
    8 KB (1,144 words) - 14:32, 21 April 2014
  • my_stats = imstat("sis14_twhya_n2hp.image", chans="0~4") imstat("sis14_twhya_n2hp.image", chans="0~4")
    5 KB (823 words) - 11:18, 5 March 2018
  • ObservationID = 0 ArrayID = 0 ...6480 [0,1,2,3,4,5,6,7] [0.001, 0.001, 0.001, 0.001, 0.001, 0.001, 0.001, 0.001] [CALIBRATE_ATMOSPHERE#AMBIENT,CALIBRATE_ATMOSPHERE#HOT,CALIBRATE_ATMOS
    9 KB (1,096 words) - 16:50, 12 April 2024
  • * Reducing a CARMA Spectral-Line mosaic of CO(1-0) in M99 (NGC4254) from the STING collaboration (Rahman et al. 2010) using t
    775 bytes (114 words) - 13:26, 5 October 2010
  • ...tunnel=False, maxrows=10, limit=1000, debug=False, server='', dateCriteria=0, * dateCriteria: -1, 0 or 1, meaning: before, on, after (currently, only 0 works!)
    4 KB (421 words) - 14:16, 18 April 2014
  • gain=0.1, threshold='3.0mJy', psfmode='clark', imagermode='csclean', interactive=T, npercycle=100, imsize=300, cell=['0.4arcsec', '0.4arcsec'],
    3 KB (398 words) - 17:46, 6 January 2012
  • sdcal(infile=sdmsd, calmode = 'ps,tsys,apply', spw='0,1,2,3') split(vis = sdmsd, spw = '0,1,2,3', outputvis = sdmsc, scan = '2', datacolumn = 'corrected', keepflags
    5 KB (769 words) - 16:33, 19 August 2021
  • ImageMetaData Restoring Beam : 0.789582 arcsec, 0.551785 arcsec, -58.4646 deg ImageMetaData 0 0 Direction Right Ascension SIN 256 256 11:01:51.796 128.00...
    9 KB (1,122 words) - 14:53, 29 May 2019
  • ...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
    11 KB (1,154 words) - 12:06, 10 May 2013
  • CASA <49>: print os.getenv('CASAPATH').split(' ')[0] + '/data/alma/simmos/' | alma.cycle0.compact.cfg || ALMA Cycle 0 compact config
    15 KB (2,527 words) - 17:29, 11 January 2018
  • Field IDs with matching source ID = [ 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23] Field IDs with matching source ID = [ 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23]
    3 KB (468 words) - 09:47, 12 April 2014
  • ImageMetaData Restoring Beam : 0.830341 arcsec, 0.683704 arcsec, -66.1199 deg ImageMetaData 0 0 Direction Right Ascension SIN 250 250 11:01:51.796 125.00...
    9 KB (1,200 words) - 17:18, 12 October 2023
  • ImageMetaData Restoring Beam : 0.830341 arcsec, 0.683704 arcsec, -66.1199 deg ImageMetaData 0 0 Direction Right Ascension SIN 250 250 11:01:51.796 125.00...
    10 KB (1,203 words) - 14:28, 6 April 2022
  • ImageMetaData Restoring Beam : 0.830341 arcsec, 0.683704 arcsec, -66.1199 deg ImageMetaData 0 0 Direction Right Ascension SIN 250 250 11:01:51.796 125.00...
    10 KB (1,203 words) - 14:46, 25 October 2022
  • ...nceFrame='TOPO', plaintext=False, lineNumbers=None, columns=None, yscale=1.0, plotunits='linear') </tt> ...maximum number of spws to select for the fit starting from the first one (0=no max)
    8 KB (1,058 words) - 12:56, 8 August 2013
  • CASA <49>: print os.getenv('CASAPATH').split(' ')[0] + '/data/alma/simmos/' | alma.cycle0.compact.cfg || ALMA Cycle 0 compact config
    15 KB (2,583 words) - 10:14, 14 December 2018
  • myspw = '0~7' myspwapcal = '0~7:20~100'
    6 KB (740 words) - 15:23, 24 April 2012
  • alma_cycle: 0 or 1 (will automatically fill in the configs offered) alma_cycle=0: configs=['alma.cycle0.compact.cfg',
    3 KB (477 words) - 12:36, 6 September 2013
  • ra = np.array([[0,1,2],[3,4,5]]) ra[0,0] = 5.75
    19 KB (3,193 words) - 18:51, 1 November 2011
  • fitspw='0:240~280' and then set excludechans=True to tell CASA that continuum by setting the fitorder to 0. We target only field '5',
    10 KB (1,580 words) - 11:13, 5 March 2018
  • {| style="width: 100%; valign: top; " cellpadding=0 ...idth: 100%; background-color:#FFFFFF;border:0px solid #EFF9FC; cellpadding=0"
    5 KB (620 words) - 16:24, 12 February 2024
  • ...one with a -4MHz offset. In this example, the spectral windows (spw), are 0, 1, and 2, respectively. For this example we use the bandpass calibrator 3c preavg = -1.0 # Pre-averaging interval (sec) (rarely needed)
    10 KB (1,205 words) - 15:47, 11 March 2021
  • ...aeBand7]]: Mosaic of the galaxy merger NGC 4038/4039 (Antennae) at Band 7 (0.87 mm) ...16293Band9]]: Mosaic of the protostellar cluster IRAS16293-2422 at Band 9 (0.45 mm)
    8 KB (1,075 words) - 21:06, 14 December 2017
  • {| style="width: 100%; valign: top; " cellpadding=0 ...idth: 100%; background-color:#FFFFFF;border:0px solid #EFF9FC; cellpadding=0"
    5 KB (621 words) - 11:22, 18 July 2017
  • ...dId numbers. In this example, the flux calibrator (MARS) is assigned FldId=0, the bandpass (and phase) calibrator (3C273) is assigned FldId=1, the mosai setjy(vis=msfile, field='3C273',fluxdensity=[17.8,0.,0.,0.], spw='0~2')
    12 KB (1,968 words) - 13:26, 29 April 2010
  • ...=&LONG_RANGE=&FRAME=Equatorial&CENTER_DEC=&LAT_RANGE=&EQUINOX=J2000&SRAD=1.0%27&MIN_EXPOSURE=&OBS_BANDS=L&TELESCOPE=VLA&OBS_MODE=ALL&CORR_MODE=ALL&TELES ...up of the data that remain. The ''y''-axis scale was reduced to the range (0, 100 Jy) by using the (Axes)'''Range''' controls.
    17 KB (2,443 words) - 18:10, 19 July 2017
  • {| style="width: 100%; valign: top; " cellpadding=0 ...idth: 100%; background-color:#FFFFFF;border:0px solid #EFF9FC; cellpadding=0"
    5 KB (635 words) - 10:44, 19 March 2018
  • {{Simulations Intro 4.0}} ; simutil.calc_pointings(spacing, imsize, cell, direction=None, relmargin=0.5)
    3 KB (481 words) - 15:53, 7 November 2012
  • ...a measurement set is handled separately during calibration. In ALMA Cycle 0 observations, each execution block contains four spectral windows. ...coordinate Ux, Vx) to the phase center in the Fourier plane (coordinates 0,0). The (u,v) distance of a visibility corresponds to the projected length of
    5 KB (781 words) - 10:11, 16 April 2014
  • {| style="width: 100%; valign: bottom; " cellpadding=0 {| style="width: 100%; valign: top; " cellpadding=0
    6 KB (854 words) - 18:09, 14 November 2012
  • equatorial (J2000.0) or galactic coordinates centered at a specific 'position'. setup_time = 8.0 # Initial setup time (min)
    9 KB (1,180 words) - 18:18, 5 February 2013
  • ...aeBand7]]: Mosaic of the galaxy merger NGC 4038/4039 (Antennae) at Band 7 (0.87 mm). Validated for CASA 6.5.4. ...16293Band9]]: Mosaic of the protostellar cluster IRAS16293-2422 at Band 9 (0.45 mm). Validated for CASA 6.5.4.
    8 KB (1,173 words) - 12:33, 22 April 2024
  • * Reducing a CARMA Spectral-Line mosaic of CO(1-0) in M99 (NGC4254) from the STING collaboration (Rahman et al. 2010) using t
    1 KB (164 words) - 17:01, 30 November 2017
  • 0 64 TOPO 36387.2295 125 8000 RR RL LR LL 0 J1008+0730 0 0.03639232 -0.026
    13 KB (1,853 words) - 13:35, 9 January 2012
  • 0 64 TOPO 36387.2295 125 8000 RR RL LR LL 0 J1008+0730 0 0.03639232 -0.026
    13 KB (1,838 words) - 17:57, 6 January 2012
  • freqSD = crval4S.values()[0] sbmajor = sbema.values()[0]
    8 KB (1,332 words) - 16:42, 19 August 2021
  • box = '0,0,299,299' incell = '0.043arcsec'
    5 KB (856 words) - 14:21, 29 April 2011
  • repodir=os.getenv("CASAPATH").split(' ')[0]+"/data/alma/simmos/" You can also simply set antennalist="alma;0.5arcsec" and simobserve will choose the closest configuration based on the
    4 KB (599 words) - 23:46, 28 December 2013
  • fitspw='0:0~239;281~383' and then set excludechans=False to tell CASA that continuum by setting the fitorder to 0. We target only field '5',
    12 KB (1,869 words) - 15:05, 29 May 2019
  • ...raBand7 | TWHydraBand7]]: The protoplanetary disk source TW Hya at Band 7 (0.87 mm) ...aeBand7]]: Mosaic of the galaxy merger NGC 4038/4039 (Antennae) at Band 7 (0.87 mm)
    6 KB (859 words) - 16:29, 8 January 2018
  • freqSD = crval4S.values()[0] sbmajor = sbema.values()[0]
    9 KB (1,473 words) - 09:42, 11 January 2018
  • au.editIntents('uid___A002_X142764_X24.ms', field=0, newintents='DELAY,PHASE,WVR')
    2 KB (220 words) - 18:26, 27 June 2013
  • ...ties are predicted using the task [https://casadocs.readthedocs.io/en/v6.4.0/api/tt/casatasks.imaging.setjy.html setjy]. The most current models availab [https://casadocs.readthedocs.io/en/v6.4.0/api/tt/casatasks.imaging.setjy.html setjy] are accessible using the flux-de
    14 KB (1,935 words) - 23:52, 10 November 2021
  • ImageMetaData::summary+ Restoring Beam : 0.609236 arcsec, 0.452453 arcsec, -51.5786 deg ImageMetaData::summary+ 0 0 Direction Right Ascension SIN 250 250 11:01:51.796 125.00...
    12 KB (1,674 words) - 10:15, 8 February 2024
  • field='0' sourcepar=[0.006,0.1,-0.05,0.4,0.3,0.0]
    5 KB (844 words) - 16:51, 29 July 2015
  • xaxis='chan', figfile='', plotrange=[0,0,0,0], help=False, caltable2='', solutionTimeThresholdSeconds=60.0, phase='', ms='', showtsky=False,
    14 KB (2,237 words) - 13:13, 17 April 2024
  • fitspw='0:0~239;281~383' and then set excludechans=False to tell CASA that continuum by setting the fitorder to 0. We target only field '5',
    12 KB (1,972 words) - 17:16, 12 October 2023
  • ...returns the apparent position but this will be changed to J2000 in casa 4.0. savefig="", showplot=False, antennalist="",frequency=345.0)
    8 KB (983 words) - 16:28, 6 September 2013
  • CASA <49>: print os.getenv('CASAPATH').split(' ')[0] + '/data/alma/simmos/' /home/casa/packages/RHEL7/release/casa-release-5.4.0-68/data/alma/simmos/
    23 KB (3,748 words) - 14:29, 2 November 2022
  • {| style="width: 100%; valign: top; " cellpadding=0 ...idth: 100%; background-color:#EFF9FC;border:0px solid #EFF9FC; cellpadding=0"
    6 KB (825 words) - 17:50, 15 November 2012
  • fitspw='0:0~239;281~383' and then set excludechans=False to tell CASA that continuum by setting the fitorder to 0. We target only field '5',
    13 KB (2,029 words) - 14:27, 6 April 2022
  • fitspw='0:0~239;281~383' and then set excludechans=False to tell CASA that continuum by setting the fitorder to 0. We target only field '5',
    13 KB (2,029 words) - 16:28, 24 October 2022
  • ...l window individually. You will find a strong CO(1-0) emission line in spw 0 in channels 55 to 69, and CN emission lines in spw 1 between channels 35~47 spw='0:20~53;71~120,1:70~120,2:20~120,3:20~120', psfmode='hogbom',
    24 KB (3,568 words) - 21:20, 12 January 2012
  • ...l window individually. You will find a strong CO(1-0) emission line in spw 0 in channels 55 to 69, and CN emission lines in spw 1 between channels 35~47 spw='0:20~53;71~120,1:70~120,2:20~120,3:20~120', psfmode='hogbom',
    24 KB (3,580 words) - 05:18, 11 May 2012
  • ...2012/07:36:57.0 - 07:39:13.1 4 0 J0522-364 5060 [0] [6.05] [CALIBRATE_BANDPASS#ON_SOURCE, CALIBRATE_PHASE#ON_SOURCE, CALIBRAT ...07:44:45.2 - 07:47:01.2 7 1 Ceres 5060 [0] [6.05] [CALIBRATE_AMPLI#ON_SOURCE, CALIBRATE_PHASE#ON_SOURCE, CALIBRATE_W
    20 KB (3,099 words) - 00:21, 7 March 2014
  • if (version < '5.1.0'): ...mosaic', mosweight = True, minpb=0.3, pbcor=False, threshold='1.0Jy', gain=0.1)
    6 KB (1,016 words) - 16:37, 19 August 2021
  • ...an older version of CASA please see [[NGC3256 Band3 Calibration for CASA 4.0]]. ...l window individually. You will find a strong CO(1-0) emission line in spw 0 in channels 55 to 69, and CN emission lines in spw 1 between channels 35~47
    24 KB (3,681 words) - 09:10, 19 April 2013
  • ...l window individually. You will find a strong CO(1-0) emission line in spw 0 in channels 55 to 69, and CN emission lines in spw 1 between channels 35~47 spw='0:20~53;71~120,1:70~120,2:20~120,3:20~120', psfmode='hogbom',
    24 KB (3,683 words) - 10:44, 1 June 2012
  • '''This guide is designed for CASA 4.0. If you are using an older version of CASA please see [[NGC3256 Band3 Cali ...line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.0]]''' section left off: right after running the CASA task {{split}} to split
    24 KB (3,681 words) - 13:14, 27 October 2012
  • ...l window individually. You will find a strong CO(1-0) emission line in spw 0 in channels 55 to 69, and CN emission lines in spw 1 between channels 35~47 spw='0:20~53;71~120,1:70~120,2:20~120,3:20~120', psfmode='hogbom',
    24 KB (3,712 words) - 11:47, 29 November 2013
  • cell=['0.08arcsec'], plotrange=[0,0,-30,30],
    12 KB (1,779 words) - 11:15, 5 March 2018
  • ...ig. 1.''' HST image of the Antennae. White contours correspond to the CO(1-0) intensity map in Wilson et al. (2000; see also Fig. 2). (Credit: NASA, ESA ...0.jpg|200px|thumb|right|'''Fig. 2.''' Caltech millimeter array (OVRO) CO(1-0) integrated intensity map from Wilson et al. (2000). ]]
    9 KB (1,381 words) - 10:20, 5 June 2012
  • vernum = str(version()[0])+'.'+str(version()[1]) plotms(vis=msc, field='0,3~150', xaxis='time', yaxis='field', coloraxis='scan', plotfile='field_vs_t
    7 KB (1,154 words) - 14:35, 16 April 2024
  • Observed from 25-Oct-2012/07:32:00.0 to 25-Oct-2012/19:16:29.9 (UTC) ObservationID = 0 ArrayID = 0
    29 KB (3,228 words) - 01:23, 1 September 2020
  • if (version < '4.7.0'): ...de='mosaic', mosweight = True, minpb=0.3, pbcor=F, threshold='1.0Jy', gain=0.1)
    7 KB (1,182 words) - 09:10, 11 January 2018
  • {{Simulations Intro 4.0}} * '''weighting''' selects natural, briggs (robust=0.5), or uniform weighting.
    2 KB (366 words) - 11:18, 2 November 2012
  • ...source name. In this example, the flux calibrator (MARS) is assigned FldId=0, the bandpass (and phase) calibrator (3C273) is assigned FldId=1, the mosai ...ith 63 channels each. Also remember that CASA and python start counting at 0, not 1.)
    20 KB (3,309 words) - 17:30, 16 March 2012
  • ...source name. In this example, the flux calibrator (MARS) is assigned FldId=0, the bandpass (and phase) calibrator (3C273) is assigned FldId=1, the mosai ...ith 63 channels each. Also remember that CASA and python start counting at 0, not 1.)
    20 KB (3,312 words) - 14:21, 6 October 2010
  • {| style="width: 100%; valign: top; " cellpadding=0 ...idth: 100%; background-color:#EFF9FC;border:0px solid #EFF9FC; cellpadding=0"
    6 KB (845 words) - 11:21, 18 July 2017
  • CASA <49>: print os.getenv('CASAPATH').split(' ')[0] + '/data/alma/simmos/' /home/casa/packages/RHEL7/release/casa-6.1.1-15-pipeline-2020.1.0.40/data/alma/simmos/
    31 KB (5,070 words) - 14:16, 3 November 2022
  • ...ig. 1.''' HST image of the Antennae. White contours correspond to the CO(1-0) intensity map in Wilson et al. (2000; see also Fig. 2). (Credit: NASA, ESA ...0.jpg|200px|thumb|right|'''Fig. 2.''' Caltech millimeter array (OVRO) CO(1-0) integrated intensity map from Wilson et al. (2000). ]]
    9 KB (1,443 words) - 12:08, 22 November 2011
  • CASA <49>: print os.getenv('CASAPATH').split(' ')[0] + '/data/alma/simmos/' /home/casa/packages/RHEL7/release/casa-release-5.4.0-68/data/alma/simmos/
    32 KB (5,174 words) - 10:20, 26 April 2023
  • window is centered on the CO(1-0) emission line in the galaxy NGC 3256 and is our ...observations of this galaxy exist. Casoli et al. (1990) observed the CO(1-0)
    8 KB (1,256 words) - 10:57, 26 April 2012
  • # specifically INCENTER +/- 0.5xINWIDTH should encompass all channels in the SPW of interest. spwid='0'
    12 KB (2,073 words) - 10:46, 15 March 2022
  • configdir = casa.values()[0]['data']+'/alma/simmos/' ...redshifts. The intrinsic model is based on the velocity field of the CO 1-0 emission from M51 presented in Helfer et al. (2003, ApJS, 145, 259), scale
    7 KB (1,189 words) - 18:34, 10 September 2019
  • ...Band 9. '''This guide requires CASA 3.4'''. Among other things, CASA 3.4.0 contains an improved antenna primary beam model for ALMA. In this casa guid This guide has been written for CASA release 3.4.0. Please confirm your version before proceeding.
    28 KB (4,108 words) - 16:24, 9 October 2012
  • # concatvis = vislist[0] ...file called calibrated_source.ms. Follow [https://casa.nrao.edu/Release4.1.0/doc/UserMan/UserMansu82.html this link] for more information regarding the
    22 KB (2,892 words) - 16:28, 28 February 2024
  • ...calibration and imaging of pre-upgrade VLA polarimetric data with CASA 5.5.0. If you are a beginning or novice user, please consult relevant [https://ca Observed from 15-Apr-1999/23:15:25.0 to 16-Apr-1999/22:54:21.6 (TAI)
    25 KB (3,544 words) - 13:00, 13 February 2023
  • ...the fully calibrated data see: [[IRAS16293_Band9_-_Calibration_for_CASA_4.0]]'''. ..._Band9_-_Calibration_for_CASA_4.0 IRAS16293_Band9_-_Calibration_for_CASA_4.0] . If you completed the calibration section, then you already have the fina
    29 KB (4,266 words) - 17:07, 20 November 2012
  • fieldlist = ['0'] # change to list of science data fields to inspect spwlist = ['0','1','2','3'] # change to list of science spws to inspect
    23 KB (2,951 words) - 13:49, 7 December 2023
  • avgtime='1e8',avgscan=T,spw='0~1:4~60',antenna='', coloraxis='spw') uvcontsub2(vis='IRC10216',fitspw='0~1:4~13;52~60',
    21 KB (3,516 words) - 16:03, 2 September 2011
  • ia.calcmask(mask='image.im > 0.0126', name='mymask1') ...rao.edu/aips2_docs/notes/223/index.shtml LEL syntax]. All values above the 0.0126 threshold are kept, the values below that threshold are blanked. This
    5 KB (810 words) - 10:54, 25 August 2021
  • cell=['0.1arcsec'], ...x,min) within mask : (0.0293485,-0.00934437) over full image : (0.0622498,-0.0327437)
    15 KB (2,072 words) - 14:42, 12 June 2019
  • ...set spwmap=[0,0,0] to map spw=0 to spw=0, spw=1 to spw=0, and spw=2 to spw=0. spwmap = [0,0,0] # mapping self-calibration solutions to individual spectral windows. Gener
    21 KB (3,082 words) - 16:54, 28 February 2024
  • This guide has been written for CASA release 4.2.0. Please confirm your version before proceeding. if (version < '4.2.0'):
    29 KB (4,388 words) - 11:43, 12 November 2014
  • fitspec='0:0~239;281~383'. continuum by setting the fitorder to 0. We target only field '5',
    13 KB (1,997 words) - 16:21, 12 October 2023
  • This guide has been written for CASA release 4.1.0. Please confirm your version before proceeding. if (version < '4.1.0'):
    30 KB (4,407 words) - 20:48, 10 December 2013
  • J2000 23h59m28.10 -019d52m12.35 10.0 os.getenv("CASAPATH").split()[0]+"/data/alma/simmos/"
    12 KB (1,706 words) - 11:53, 1 December 2010
  • ...l window individually. You will find a strong CO(1-0) emission line in spw 0 in channels 55 to 69, and CN emission lines in spw 1 between channels 35~47 spw='0:20~53;71~120,1:70~120,2:20~120,3:20~120', psfmode='hogbom',
    24 KB (3,714 words) - 14:51, 4 February 2016
  • ...l window individually. You will find a strong CO(1-0) emission line in spw 0 in channels 55 to 69, and CN emission lines in spw 1 between channels 35~47 spw='0:20~53;71~120,1:70~120,2:20~120,3:20~120', psfmode='hogbom',
    25 KB (3,722 words) - 14:57, 4 April 2017
  • ...l window individually. You will find a strong CO(1-0) emission line in spw 0 in channels 55 to 69, and CN emission lines in spw 1 between channels 35~47 spw='0:20~53;71~120,1:70~120,2:20~120,3:20~120', psfmode='hogbom',
    24 KB (3,722 words) - 15:37, 31 March 2017
  • window is centered on the CO(1-0) emission line in the galaxy NGC 3256 and is our ...observations of this galaxy exist. Casoli et al. (1990) observed the CO(1-0)
    9 KB (1,372 words) - 01:46, 19 January 2012
  • CASA <49>: print os.getenv('CASAPATH').split(' ')[0] + '/data/alma/simmos/' /home/casa/packages/RHEL7/release/casa-6.4.0-16/data/alma/simmos/
    39 KB (6,403 words) - 15:53, 2 November 2022
  • ...ig. 1.''' HST image of the Antennae. White contours correspond to the CO(1-0) intensity map in Wilson et al. (2000; see also Fig. 2). (Credit: NASA, ESA ...0.jpg|200px|thumb|right|'''Fig. 2.''' Caltech millimeter array (OVRO) CO(1-0) integrated intensity map from Wilson et al. (2000). ]]
    10 KB (1,605 words) - 11:54, 30 May 2012
  • ..._X9fddd8_Xc52_target.ms', field='', intent='', spw='17,19,21,23', antenna='0~35', gaintable='/lustre/naasc/sciops/comm/amcnicho/pipeline/root/2013.1.007 # For CASA 5.0 and 5.1, applycal() does not yet fully support
    8 KB (1,144 words) - 11:09, 29 September 2017
  • ...e [http://casa.nrao.edu/Memos/229.html MeasurementSet definition version 2.0]. ...48 but not to include dummy scans (the first two, which have a field ID of 0). We can have Python create a string of scan numbers that satisfy this req
    18 KB (2,494 words) - 10:53, 19 September 2019
  • spw = '0' # Select spectral window/channels start = 0 # first input channel to use
    26 KB (3,652 words) - 12:22, 25 May 2010
  • ...set spwmap=[0,0,0] to map spw=0 to spw=0, spw=1 to spw=0, and spw=2 to spw=0. spwmap = [0,0,0] # mapping self-calibration solutions to individual spectral windows. Gener
    22 KB (3,210 words) - 16:35, 11 October 2023
  • ...which are flagged have Flag = 1, whereas unflagged data are set to Flag = 0. Note that, to display flagged data, you will have to click on the '''Displ ...then FlagRow will be set to 1 for that row. Unflagged rows have FlagRow = 0. However, note that some tasks (like {{plotms}}) may flag a row, but ''not'
    5 KB (842 words) - 18:01, 7 June 2010
  • cell=['0.1arcsec'], ...the last major cycle. If it doesn't exist, please re-run tclean with niter=0,calcres=False,calcpsf=False in order to trigger a 'predict model' step that
    15 KB (2,227 words) - 17:06, 12 October 2023
  • This guide has been written for CASA release 4.5.0. Please confirm your version before proceeding. if (version < '4.5.0'):
    26 KB (3,752 words) - 09:31, 4 April 2017
  • This tutorial describes the data reduction for CO (1-0) data observed toward the galaxy M99 (NGC 4254) using CARMA. CO (1-0) observations are a standard method used by millimeter astronomers to estim
    37 KB (5,752 words) - 17:27, 26 May 2011
  • Ignoring spectral window [0, 25, 26, 27, 28, 29, 30, 31, 32, 33] because it is WVR related
    2 KB (265 words) - 11:50, 1 March 2012
  • *'''This guide requires CASA 4.1.0 and assumes that you have downloaded M100_Band3_SD_UncalibratedData.tgz fro '''This guide is designed for CASA 4.1.0.
    39 KB (4,942 words) - 10:56, 4 August 2014
  • ...ges] will return '1:0~259,1:501~3839'. The fitspw parameter should be '0,1:0~259,1:501~3839,2'. If you haven't installed Analysis Utilities, see [https: fitspw = '2:0~1200;1500~3839,3:0~1200;1500~3839' # line free channels. Use au.invertChannelRanges
    16 KB (2,477 words) - 16:36, 28 February 2024
  • This tutorial describes the data reduction for CO (1-0) data observed toward the galaxy M99 (NGC 4254) using CARMA. CO (1-0) observations are a standard method used by millimeter astronomers to estim
    39 KB (6,041 words) - 13:04, 5 July 2011
  • [[File:g19.3CO.png|thumb| Integrated intensity SMA 12CO 2-1 map of G19.3+0.07 overlaid on a Spitzer image]] ...ript works with CASA 3.1.0. For an updated script that works with CASA 3.2.0, please go to [[SMA CO Line Data 3.2]].'''
    41 KB (5,906 words) - 11:46, 18 May 2011
  • This guide has been written for CASA release 4.4.0. Please confirm your version before proceeding. if (version < '4.4.0'):
    29 KB (4,388 words) - 21:53, 6 July 2015
  • ...images, we typically employed ''robust=0.0'', though occasionally up to 1.0 was used. ...orded by the longest baselines is challenging. For example, at 89 GHz with 0.25 km/s channels, 30 antennas, 3.5 hours on-source, and an angular resoluti
    16 KB (2,452 words) - 10:11, 8 May 2018
  • This guide has been written for CASA release 4.3.0. Please confirm your version before proceeding. if (version < '4.3.0'):
    30 KB (4,388 words) - 11:03, 21 February 2018
  • [[File:g19.3CO.png|thumb| Integrated intensity SMA 12CO 2-1 map of G19.3+0.07 overlaid on a Spitzer image]] ...six-pointing mosaic of 12CO 2-1 emission in the infrared dark cloud G19.3+0.07. The CO line was placed in the USB. These data are from Brogan et al. in
    42 KB (6,040 words) - 13:25, 5 May 2011
  • ...ges] will return '1:0~259,1:501~3839'. The fitspw parameter should be '0,1:0~259,1:501~3839,2'. If you haven't installed Analysis Utilities, see [https: fitspw = '2:0~1200;1500~3839,3:0~1200;1500~3839' # line free channels. Use au.invertChannelRanges
    16 KB (2,499 words) - 15:03, 18 October 2023
  • if line[0] == '#': continue # Ignore anything that starts with a # plt.errorbar(z_array, mod_array, yerr=moderr_array, fmt='.', capsize=0,
    17 KB (2,938 words) - 18:54, 17 November 2011
  • window is centered on the CO(1-0) emission line in the galaxy NGC 3256 and is our ...observations of this galaxy exist. Casoli et al. (1990) observed the CO(1-0)
    9 KB (1,395 words) - 09:09, 7 September 2015
  • ''This tutorial was created and tested using CASA 6.2.0'' ...calibrated and the science target [https://casadocs.readthedocs.io/en/v6.2.0/api/tt/casatasks.manipulation.split.html split] out.
    28 KB (3,634 words) - 19:56, 5 October 2021
  • ...IRAM interferometer (Garcia-Burillo et al. 1998). In this CASAguide, CO (1-0) emission is mapped with ALMA using the main (12-m) array, the 7-m array, a ...488.281 kHz, or 1.27 km/s, and one of the windows is centered at the CO (1-0) line with a rest frequency of 115.271 GHz in ALMA Band 3. There are three
    11 KB (1,777 words) - 18:56, 26 March 2024
  • approximately 1/500000*206265 arcsec = 0.4 arcsec. We will use a '''cellsize=0.1''', to oversample the beam sufficiently. The FWHM of the primary beam of
    28 KB (4,145 words) - 09:41, 14 September 2017
  • This guide has been written for CASA release 3.4.0. Please confirm your version before proceeding. 3c279 is the bandpass calibrator (field id=0)
    49 KB (7,548 words) - 15:38, 9 May 2012
  • approximately 1/500000*206265 arcsec = 0.4 arcsec. We will use a '''cellsize=0.1''', to oversample the beam sufficiently. The FWHM of the primary beam of
    28 KB (4,149 words) - 09:48, 10 April 2017
  • ...ig. 1.''' HST image of the Antennae. White contours correspond to the CO(1-0) intensity map in Wilson et al. (2000; see also Fig. 2). (Credit: NASA, ESA ...0.jpg|300px|thumb|right|'''Fig. 2.''' Caltech millimeter array (OVRO) CO(1-0) integrated intensity map from Wilson et al. (2000). ]]
    11 KB (1,652 words) - 04:27, 31 December 2023
  • Observed from 03-Jan-2013/06:31:48.0 to 03-Jan-2013/07:47:51.0 (UTC) ObservationID = 0 ArrayID = 0
    26 KB (3,524 words) - 10:41, 14 June 2016
  • Observed from 03-Jan-2013/06:31:48.0 to 03-Jan-2013/07:47:51.0 (UTC) ObservationID = 0 ArrayID = 0
    26 KB (3,524 words) - 13:14, 20 April 2017
  • Observed from 03-Jan-2013/06:31:48.0 to 03-Jan-2013/07:47:51.0 (UTC) ObservationID = 0 ArrayID = 0
    26 KB (3,524 words) - 11:47, 18 November 2016
  • 0 64 TOPO 36387.2295 125 8000 36387.2295 RR RL L 0 J1008+0730 0 0.03639232 -0.026
    44 KB (6,777 words) - 12:19, 19 May 2010
  • ...', observation='', verbose=True, listfile='', listunfl=False, cachesize=50.0, overwrite=False ) Observed from 24-Jun-2015/07:32:30.0 to 24-Jun-2015/10:02:03.0 (UTC)
    30 KB (3,840 words) - 17:11, 22 February 2024
  • ...''mysteps'' index. Several steps may be listed together such as ''mysteps=[0,1,2]''. mysteps = [0]
    8 KB (1,236 words) - 16:50, 29 April 2024
  • ...', observation='', verbose=True, listfile='', listunfl=False, cachesize=50.0, overwrite=False ) Observed from 24-Jun-2015/07:32:30.0 to 24-Jun-2015/10:02:03.0 (UTC)
    30 KB (3,847 words) - 16:55, 22 February 2024
  • <b>This CASA Guide is for CASA version 5.0.0</b> Observed from 03-Jan-2013/06:31:48.0 to 03-Jan-2013/07:47:51.0 (UTC)
    27 KB (3,594 words) - 18:15, 20 July 2017
  • 0%....10....20....30....40....50....60....70....80....90....100%
    3 KB (510 words) - 16:33, 30 April 2010
  • ...ence-verification. The guide has been written for data reduced in CASA 4.3.0 or later and assumes that all calibration tables (Tsys and gain tables) hav This guide has been written for CASA release 4.3.0. Please confirm your version before proceeding.
    37 KB (5,642 words) - 19:30, 19 May 2015
  • ...erved frequency range, one may "overlap" EVLA basebands, offsetting one by 0.5 times the subband width. This way, the decreased sensitivity at subband 0 64 TOPO 4736 2000 128000 RR RL LR LL
    11 KB (1,530 words) - 21:09, 1 March 2012
  • <b>This CASA Guide is for CASA version 5.4.0</b> ...https://casaguides.nrao.edu/index.php/VLA_Continuum_Tutorial_3C391-CASA5.4.0 VLA 3C391 Continuum Tutorial] before proceeding with this tutorial.
    27 KB (3,654 words) - 14:39, 6 November 2018
  • ...w = '0'</tt>), while floats and integers never will (e.g., <tt>diameter=25.0</tt>). Boolean variables will be <tt>True</tt> or <tt>False</tt> with no qu ...xample, start at 0. The first field in a measurement set has <tt>FIELD_ID==0</tt>.
    15 KB (2,361 words) - 12:09, 14 December 2018
  • ...oment maps of the original BIMA SONG measurements of M51. ''Left'': Moment 0 (integrated intensity). ''Right'': Moment 1 (velocity field).]] ...but, in this simulation, we will model how it would appear at redshift z = 0.1 (luminosity distance = 460 Mpc).
    17 KB (2,562 words) - 19:00, 28 April 2011
  • ...ithresh algorithm is given in the [https://casa.nrao.edu/casadocs/casa-5.4.0/synthesis-imaging/masks-for-deconvolution CASA documentation] and [https:// ...i.e., ''negativethreshold''=5.0 will create a mask for values less than -5.0 sigma.
    42 KB (5,977 words) - 16:32, 8 March 2024
  • 0 none 1924-292 19:24:51.05600 -29.14.30.1280 J2000 0 169125 0 4 TOPO 184550 1500000 7500000 I
    48 KB (7,218 words) - 15:07, 23 May 2012
  • <b>This CASA Guide is for CASA version 5.5.0</b> ...https://casaguides.nrao.edu/index.php/VLA_Continuum_Tutorial_3C391-CASA5.4.0 VLA 3C391 Continuum Tutorial] before proceeding with this tutorial.
    28 KB (3,769 words) - 11:37, 10 July 2019
  • <b>This CASA Guide is for CASA version 5.7.0</b> ...https://casaguides.nrao.edu/index.php/VLA_Continuum_Tutorial_3C391-CASA5.4.0 VLA 3C391 Continuum Tutorial] before proceeding with this tutorial.
    28 KB (3,783 words) - 13:04, 13 November 2020
  • <b>This CASA Guide is for CASA version 6.2.0</b> ...https://casaguides.nrao.edu/index.php/VLA_Continuum_Tutorial_3C391-CASA6.2.0 VLA 3C391 Continuum Tutorial] before proceeding with this tutorial.
    29 KB (3,922 words) - 11:40, 2 May 2022
  • ...erved frequency range, one may "overlap" EVLA basebands, offsetting one by 0.5 times the subband width. This way, the decreased sensitivity at subband 0 64 TOPO 4736 2000 128000 RR RL LR LL
    11 KB (1,581 words) - 13:47, 1 May 2013
  • approximately 1/500000*206265 arcsec = 0.4 arcsec. We will use a '''cellsize=0.1''', to oversample the beam sufficiently. The FWHM of the primary beam of
    32 KB (4,524 words) - 16:03, 3 April 2018
  • approximately 1/500000*206265 arcsec = 0.4 arcsec. We will use a '''cellsize=0.1''', to oversample the beam sufficiently. The FWHM of the primary beam of
    31 KB (4,534 words) - 17:29, 11 March 2021
  • <table width="650" cellspacing="6" cellpadding="4" border="0"> ...D'Angelo 2005. It simulates a M_planet = 1 M_jup around a star of M_star = 0.5 Msun at a Distance = 50pc. A FITS [http://www.cv.nrao.edu/~awootten/mmaim
    4 KB (627 words) - 14:44, 7 November 2012
  • approximately 1/500000*206265 arcsec = 0.4 arcsec. We will use a '''cellsize=0.1''', to oversample the beam sufficiently. The FWHM of the primary beam of
    31 KB (4,537 words) - 17:31, 11 March 2021
  • approximately 1/500000*206265 arcsec = 0.4 arcsec. We will use a '''cellsize=0.1''', to oversample the beam sufficiently. The FWHM of the primary beam of
    31 KB (4,537 words) - 09:10, 13 October 2021
  • approximately 1/500000*206265 arcsec = 0.4 arcsec. We will use a '''cellsize=0.1''', to oversample the beam sufficiently. The FWHM of the primary beam of
    31 KB (4,537 words) - 10:20, 1 October 2021
  • avgtime='1e8',avgscan=T,spw='0~1:4~60',antenna='', coloraxis='spw') uvcontsub2(vis='IRC10216',fitspw='0~1:4~13;52~60',
    28 KB (4,647 words) - 20:37, 29 February 2012
  • 3c279 is the bandpass calibrator (field id=0) Observed from 22-Apr-2011/00:01:52.9 to 22-Apr-2011/01:43:42.0 (UTC)
    52 KB (7,967 words) - 17:18, 16 December 2011
  • avgtime='1e8',avgscan=T,spw='0~1:4~60',antenna='', coloraxis='spw') uvcontsub2(vis='IRC10216',fitspw='0~1:4~13;52~60',
    28 KB (4,648 words) - 12:31, 9 April 2012
  • approximately 1/500000*206265 arcsec = 0.4 arcsec. We will use a '''cellsize=0.1''', to oversample the beam sufficiently. The FWHM of the primary beam of
    30 KB (4,386 words) - 14:55, 23 October 2023
  • ''This tutorial was created and tested using CASA 6.2.0'' ...ted and had their science targets [https://casadocs.readthedocs.io/en/v6.2.0/api/tt/casatasks.manipulation.split.html split] out.
    27 KB (3,372 words) - 18:44, 27 October 2021
  • avgtime='1e8',avgscan=T,spw='0~1:4~60',antenna='', coloraxis='spw') uvcontsub2(vis='IRC10216',fitspw='0~1:4~13;52~60',
    28 KB (4,570 words) - 17:09, 11 January 2012
  • ...oment maps of the original BIMA SONG measurements of M51. ''Left'': Moment 0 (integrated intensity). ''Right'': Moment 1 (velocity field).]] ...but, in this simulation, we will model how it would appear at redshift z = 0.1 (luminosity distance = 460 Mpc).
    18 KB (2,660 words) - 16:01, 18 May 2010
  • 0 none IRAS16293-2422-a 16:32:22.992000 -24.28.36.00000 J2000 0 7812 1 none IRAS16293-2422-a 16:32:22.479253 -24.28.36.00000 J2000 0 7821
    36 KB (5,365 words) - 10:23, 28 September 2018
  • Found W08 in file: /usr/lib64/casapy/release/3.4.0/data/alma/simmos/vla.a.cfg Found E08 in file: /usr/lib64/casapy/release/3.4.0/data/alma/simmos/vla.a.cfg
    6 KB (1,030 words) - 16:45, 24 March 2013
  • ...und-color:#E0E0E0; border:1px solid #3366FF; text-align: left; cellpadding=0" ...und-color:#E0E0E0; border:1px solid #3366FF; text-align: left; cellpadding=0"
    11 KB (1,742 words) - 17:03, 22 March 2024
  • -- minpixpos: [244, 770, 0, 0] -- maxpixpos: [611, 520, 0, 0]
    14 KB (2,204 words) - 17:10, 17 April 2024
  • ...um and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 5.4.0'''. In this casa guide you will also need the [http://casaguides.nrao.edu/i This guide has been written for CASA release 5.4.0. Please confirm your version before proceeding.
    37 KB (5,453 words) - 16:43, 11 March 2021
  • ''A new version of this page exists for CASA 3.3: [[M51 at z = 0.1 and z = 0.3 (CASA 3.3)]].'' ...oment maps of the original BIMA SONG measurements of M51. ''Left'': Moment 0 (integrated intensity). ''Right'': Moment 1 (velocity field).]]
    18 KB (2,815 words) - 09:46, 24 October 2011
  • 3c279 is the bandpass calibrator (field id=0) Observed from 22-Apr-2011/00:01:52.9 to 22-Apr-2011/01:43:42.0 (UTC)
    57 KB (8,983 words) - 12:55, 31 May 2012
  • Image Statistics: Beam 0.652", 0.504", -65.889°, RMS = 12.9 mJy </caption>]] cell=['0.1arcsec'],
    22 KB (3,254 words) - 12:48, 27 September 2023
  • 0 none IRAS16293-2422-a 16:32:22.992000 -24.28.36.00000 J2000 0 7812 1 none IRAS16293-2422-a 16:32:22.479253 -24.28.36.00000 J2000 0 7821
    36 KB (5,329 words) - 11:03, 27 October 2020
  • 3c279 is the bandpass calibrator (field id=0) Observed from 22-Apr-2011/00:01:52.9 to 22-Apr-2011/01:43:42.0 (UTC)
    57 KB (9,025 words) - 15:30, 25 January 2012
  • ...um and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 5.7.0'''. In this casa guide you will also need the [http://casaguides.nrao.edu/i This guide has been written for CASA release 5.7.0. Please confirm your version before proceeding.
    37 KB (5,464 words) - 11:16, 10 June 2021
  • parameter=[-0.0072,0.0045,-0.0017, -0.0220,0.0040,-0.0190]) ...0.03 on the best days. We will use a zenith opacity of <math>\tau_z</math>=0.04. The zenith opacity is then corrected for
    45 KB (7,121 words) - 14:11, 21 May 2012
  • ...heric spectral lines in SS Objects, the models were updated for the CASA 4.0 release. The new models are called Butler-JPL- Horizons 2012 and represent |Venus || -0.01 || -0.01 || +0.00 || +0.38
    9 KB (1,396 words) - 17:09, 19 August 2021
  • 3c279 is the bandpass calibrator (field id=0) Observed from 22-Apr-2011/00:01:52.9 to 22-Apr-2011/01:43:42.0 (UTC)
    60 KB (9,450 words) - 16:45, 23 April 2012
  • if (version < '6.1.0'): 0 none IRAS16293-2422-a 16:32:22.992000 -24.28.36.00000 J2000 0 7812
    37 KB (5,482 words) - 16:40, 10 June 2021
  • if (version < '6.2.0'): 0 none IRAS16293-2422-a 16:32:22.992000 -24.28.36.00000 J2000 0 7812
    37 KB (5,511 words) - 10:16, 7 April 2022
  • if (version < '6.4.0'): 0 none IRAS16293-2422-a 16:32:22.992000 -24.28.36.00000 J2000 0 7812
    37 KB (5,507 words) - 14:15, 25 October 2022
  • if (version < '6.4.0'): 0 none IRAS16293-2422-a 16:32:22.992000 -24.28.36.00000 J2000 0 7812
    37 KB (5,511 words) - 14:16, 25 October 2022
  • ...t is the antenna: either an integer number (1..28, 29=PieTown, 30=all, and 0=mean) or a string name in the form of 'ea03'. The second argument is the b CASA <5>: getgain(3,'K',45.0)
    3 KB (409 words) - 16:16, 1 May 2013
  • {{Checked 5.5.0}} Note: IPython's (5.1.0) latest updates prevent copy/pasting several lines of code. To remedy this,
    31 KB (4,501 words) - 12:57, 13 February 2023
  • flagzero=True,cliplevel=1e-08,flagpol=True,shadow=True, diameter=28.0) ...data, regardless of source. To be conservative, we specify ''diameter=28.0'' to set the assumed antenna diameter for calculation of when antennas are
    7 KB (1,170 words) - 16:58, 8 May 2016
  • ...i.e., ''negativethreshold''=5.0 will create a mask for values less than -5.0 sigma. | 5.0
    54 KB (7,365 words) - 11:29, 3 April 2024
  • ...ed using a zero-based index. Scan 0 refers to the 1934-638 field (field ID 0) which we will use for bandpass and flux calibration. Field ID 1 is the 205 field=’0
    31 KB (4,564 words) - 02:04, 2 June 2015
  • 0 none IRAS16293-2422-a 16:32:22.992000 -24.28.36.00000 J2000 0 7812 1 none IRAS16293-2422-a 16:32:22.479253 -24.28.36.00000 J2000 0 7821
    38 KB (5,651 words) - 08:54, 23 October 2023
  • ...u/cgi-bin/ZXHLP2.PL?IMAGR IMAGR], [https://casadocs.readthedocs.io/en/v6.4.0/api/tt/casatasks.imaging.tclean.html tclean], etc.) are not provided. ...han on a network. Sometimes, it may be necessary to type "aips tv=local:0.0". Once AIPS starts, users may be asked to select a printer (this depends o
    63 KB (10,564 words) - 19:14, 1 June 2023
  • cl.addcomponent(dir=direction, flux=1.0, fluxunit='Jy', freq='230.0GHz', shape="Gaussian", majoraxis="0.1arcmin", minoraxis='0.05arcmin', positionangle='45.0deg')
    12 KB (1,923 words) - 13:13, 6 September 2017
  • The currently maintained combination CASAguide, written for CASA 4.3.0, can be found here: https://casaguides.nrao.edu/index.php/M100_Band3_Combin ...-verification. '''This guide has been written for data reduced in CASA 4.5.0''' and assumes that all calibration tables (Tsys and gain tables) have been
    37 KB (5,732 words) - 09:33, 10 April 2017
  • ...u/cgi-bin/ZXHLP2.PL?IMAGR IMAGR], [https://casadocs.readthedocs.io/en/v6.4.0/api/tt/casatasks.imaging.tclean.html tclean], etc.) are not provided. ...han on a network. Sometimes, it may be necessary to type "aips tv=local:0.0". Once AIPS starts, users may be asked to select a printer (this depends o
    63 KB (10,611 words) - 13:48, 18 December 2023
  • 2010-02-11 18:11:34 INFO listobs Observed from 18-Dec-2009/10:52:17.0 to 18-Dec-2009/14:00:01.5 (UTC) 2010-02-11 18:11:35 INFO listobs ObservationID = 0 ArrayID = 0
    51 KB (6,414 words) - 17:21, 4 May 2010
  • ...ASA version 3.3. For older versions of CASA, see [[M51 at z = 0.1 and z = 0.3 (CASA 3.2)]].'' ...oment maps of the original BIMA SONG measurements of M51. ''Left'': Moment 0 (integrated intensity). ''Right'': Moment 1 (velocity field).]]
    22 KB (3,487 words) - 11:15, 22 November 2011
  • ...see that the Northern mosaic '''imsize''' needs to be about 1 arcmin. With 0.2" pixels, this requires a '''imsize'''=300. ...0:1~50;120~164': To specify only the line-free channels of spectral window 0.
    41 KB (6,416 words) - 16:05, 16 May 2012
  • [https://carta.readthedocs.io/en/3.0/ https://carta.readthedocs.io/en/3.0/] ...ted and had their science targets [https://casadocs.readthedocs.io/en/v6.2.0/api/tt/casatasks.manipulation.split.html split] out.
    34 KB (4,087 words) - 10:49, 26 January 2023
  • This guide is designed for CASA 4.3.0. This guide has been written for CASA release 4.3.0. Please confirm your version before proceeding.
    49 KB (6,272 words) - 16:27, 26 August 2015
  • The ability to image ''flanking fields'' will be introduced in CASA v. 3.0.0. For the purposes of this tutorial, flanking fields are the locations of ne 'J2000 13h27m20.98 43d26m28.0',
    14 KB (1,990 words) - 16:55, 23 June 2017
  • spw='0~3:22~3820',width=100,datacolumn='data') plotms(vis='TWHydra_cont.ms',spw='0~3',xaxis='channel',yaxis='amp',
    41 KB (6,493 words) - 21:20, 23 April 2012
  • parameter=[-0.0072,0.0045,-0.0017, -0.0220,0.0040,-0.0190]) 0 : 36.387 : 0.041
    49 KB (7,632 words) - 21:16, 29 August 2011
  • spw='0~3:22~3820',width=100,datacolumn='data') plotms(vis='TWHydra_cont.ms',spw='0~3',xaxis='channel',yaxis='amp',
    41 KB (6,495 words) - 18:36, 12 January 2012
  • ObservationID = 0 ArrayID = 0 ...2011/19:38:05.8 - 19:50:22.8 11 1 M100 1500 [0,1,2,3] [6.05, 6.05, 6.05, 6.05] [CALIBRATE_WVR#ON_SOURCE,OBSERVE_TARGET#ON
    39 KB (5,971 words) - 14:39, 19 August 2021
  • *'''This guide requires CASA 5.1.0 and assumes that you have downloaded M100_Band3_TP_UncalibratedData.tgz as ...ocesses described below WILL NOT OPERATE in CASA versions earlier than 5.1.0'''
    39 KB (5,284 words) - 16:07, 19 August 2021
  • if (version < '5.1.0'): ...016, 0.016, 0.016, 0.016, 0.576, 0.576, 0.576, 0.576, 0.576, 0.576, 0.576, 0.576] [CALIBRATE_ATMOSPHERE#AMBIENT,CALIBRATE_ATMOSPHERE#HOT,CALIBRATE_ATMOS
    40 KB (4,408 words) - 16:31, 19 August 2021
  • * timerange = 2006/12/09/0:0:0~23:0:0. ...(vis='ag733.ms', antenna='VA15', timerange='2006/12/09/04:45:10.0~04:45:20.0')
    29 KB (4,241 words) - 17:16, 2 February 2023
  • <?xml version="1.0" encoding="UTF-8"?> xcoord = 0 # x pixel coordinate
    14 KB (2,217 words) - 20:53, 16 January 2012
  • ...-verification. '''This guide has been written for data reduced in CASA 5.4.0''' and assumes that all calibration tables (Tsys and gain tables) have been This guide has been written for CASA release 5.4.0. Please confirm your version before proceeding.
    40 KB (6,024 words) - 16:09, 19 August 2021
  • ...-verification. '''This guide has been written for data reduced in CASA 6.1.0''' and assumes that all calibration tables (Tsys and gain tables) have been This guide has been written for CASA release 6.1.0. Please confirm your version before proceeding.
    40 KB (6,039 words) - 14:44, 19 August 2021
  • ...ocesses described below WILL NOT OPERATE in CASA versions earlier than 6.2.0''' if (version < '6.2.0'):
    40 KB (5,491 words) - 11:39, 7 April 2022
  • if (version < '6.2.0'): ObservationID = 0 ArrayID = 0
    40 KB (6,067 words) - 11:49, 7 April 2022
  • ...ocesses described below WILL NOT OPERATE in CASA versions earlier than 5.1.0''' This guide has been written for CASA release 5.7.0. Please confirm your version before proceeding.
    39 KB (5,356 words) - 14:36, 19 August 2021
  • ...ocesses described below WILL NOT OPERATE in CASA versions earlier than 6.4.0''' if (version < '6.4.0'):
    40 KB (5,491 words) - 11:06, 12 October 2023
  • if (version < '6.5.0'): uid___A002_X85c183_X60b Observed from 2014-07-01T22:43:50.0 to 2014-07-01T23:32:39.6 (UTC) DA61, PM03, PM04
    40 KB (5,472 words) - 16:52, 2 February 2024
  • version = 1.0.8 CASA_PATH = /home/casa/release/casa-release-5.4.0-70 linux admit cpu-name
    15 KB (2,623 words) - 16:10, 28 February 2024
  • if (version < '4.7.0'): ...016, 0.016, 0.016, 0.016, 0.576, 0.576, 0.576, 0.576, 0.576, 0.576, 0.576, 0.576] [CALIBRATE_ATMOSPHERE#AMBIENT,CALIBRATE_ATMOSPHERE#HOT,CALIBRATE_ATMOS
    41 KB (4,534 words) - 08:50, 11 January 2018
  • ...ocesses described below WILL NOT OPERATE in CASA versions earlier than 6.1.0''' This guide is designed for CASA 6.1.0.
    40 KB (5,435 words) - 14:37, 19 August 2021
  • This guide is designed for CASA 4.5.0. This guide has been written for CASA release 4.5.0.,Please confirm your version before proceeding.
    39 KB (5,283 words) - 01:21, 23 August 2017
  • 0 none 1037-295 10:37:16.0790 -29.34.02.8130 J2000 0 38759 0 4 TOPO 184550 1500000 7500000 183300 I
    67 KB (10,305 words) - 09:50, 10 May 2012
  • [https://carta.readthedocs.io/en/3.0/ https://carta.readthedocs.io/en/3.0/] casa -r 6.5.4-9-pipeline-2023.1.0.124
    39 KB (4,613 words) - 17:21, 26 February 2024
  • ...&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES 6], but the reduction techniques could be applie opacity = 0.0
    35 KB (5,087 words) - 17:54, 8 February 2023
  • Image Statistics: Beam 0.560", 0.416", -55.974°, RMS = 6.6 mJy </caption>]] cell=['0.1arcsec'],
    23 KB (3,449 words) - 17:16, 13 October 2023
  • ...ce Verification data. Both contain several lines, including CO emission (1-0 for NGC 3256 and 3-2 for TW Hydra), and continuum emission. We will begin b ...out a subset of the spectral windows (thus changing the definition of spw 0). You might be able to get away with this depending on how you set things u
    9 KB (1,578 words) - 10:49, 27 February 2013
  • This guide has been written for CASA release 3.4.0. Please confirm your version before proceeding. spw='0~3:21~3820',width=100,datacolumn='data')
    45 KB (6,856 words) - 16:30, 12 June 2012
  • ...CASA version 4.0. For older versions of CASA see [[M51 at z = 0.1 and z = 0.3 (CASA 3.4)]].''' ...oment maps of the original BIMA SONG measurements of M51. ''Left'': Moment 0 (integrated intensity). ''Right'': Moment 1 (velocity field).]]
    22 KB (3,420 words) - 15:28, 26 October 2012
  • 0 none 1037-295 10:37:16.0790 -29.34.02.8130 J2000 0 38759 0 4 TOPO 184550 1500000 7500000 183300 I
    58 KB (8,691 words) - 11:04, 23 November 2011
  • [https://casaguides.nrao.edu/index.php?title=VLA_Data_Combination-CASA5.0.0] '''This tutorial was created and tested using CASA 4.6.0'''
    29 KB (3,669 words) - 18:03, 28 July 2017
  • 0 none 1037-295 10:37:16.0790 -29.34.02.8130 J2000 0 38759 0 4 TOPO 184550 1500000 7500000 183300 I
    58 KB (8,728 words) - 17:14, 25 January 2012
  • ...-verification. '''This guide has been written for data reduced in CASA 4.3.0''' and assumes that all calibration tables (Tsys and gain tables) have been This guide has been written for CASA release 4.3.0. Please confirm your version before proceeding.
    41 KB (6,318 words) - 16:11, 19 August 2021
  • ...te to data combination. If you are trying to combine ALMA data from Cycles 0, 1, and/or 2, you should be aware of the issues described here. Only data c ...erture efficiency depends on the rms antenna surface accuracy and is about 0.75 for ALMA dishes.
    33 KB (5,060 words) - 17:27, 29 April 2024
  • This guide has been written for CASA release 3.4.0. Please confirm your version before proceeding by pasting the following li Observed from 22-Apr-2011/00:01:52.9 to 22-Apr-2011/01:43:42.0 (UTC)
    64 KB (10,004 words) - 16:29, 31 May 2012
  • Example 2. Plot the antenna pad locations for the ALMA Cycle 0 compact configuration.
    4 KB (325 words) - 11:47, 3 July 2013
  • if (version < '6.5.0'): ObservationID = 0 ArrayID = 0
    42 KB (6,416 words) - 17:35, 22 April 2024
  • This guide has been written for CASA release 3.4.0. Please confirm your version before proceeding. 0 none 1037-295 10:37:16.0790 -29.34.02.8130 J2000 0 38759
    60 KB (9,062 words) - 13:47, 4 September 2012
  • spw='0~3:21~3820',width=100,datacolumn='data') plotms(vis='TWHydra_cont.ms',spw='0~3',xaxis='channel',yaxis='amp',
    47 KB (7,259 words) - 16:08, 31 May 2012

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