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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

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