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  • ...se, scan=True, baseband=True, clip=True, autocorr=True, hm_tbuff='1.5int', template=False, online=True, tbuff=0.0, fracspw=0.05, shadow=True, quack=True, edges In Fig. 17, we show some of gain amplitude plot examples. Antenna ea03 shows credible solutions (the colors represent different spec
    84 KB (12,632 words) - 17:59, 29 March 2017
  • ...rences between clean and tclean, please see the guide: [[TCLEAN_and_ALMA | Examples for using the new tclean CASA task for ALMA Imaging]]. '' * [[ALMA_Imaging_Pipeline_Reprocessing | Examples for ALMA Imaging Pipeline Reprocessing]]
    9 KB (1,222 words) - 16:52, 18 October 2019
  • ...data. In that case, look at the data itself in {{plotms}} (see below for examples) to decide whether or not to apply all flags. ...libration for our 8-bit data, but if one is following this CASA Guide as a template for 3-bit data, this step is needed to account for the small gain changes (
    115 KB (15,378 words) - 19:52, 4 February 2014
  • ...e to a 5km/s channel, so we will forgo the the continuum subtraction step. Examples of how to do this if you are so inclined are located in various other ALMA template='M100_Intcombo_0.193_cube.image',
    37 KB (5,642 words) - 19:30, 19 May 2015
  • ...data. In that case, look at the data itself in {{plotms}} (see below for examples) to decide whether or not to apply all flags. ...libration for our 8-bit data, but if one is following this CASA Guide as a template for 3-bit data, this step is needed to account for the small gain changes (
    117 KB (15,635 words) - 13:17, 6 February 2014
  • ...data. In that case, look at the data itself in {{plotms}} (see below for examples) to decide whether or not to apply all flags. ...libration for our 8-bit data, but if one is following this CASA Guide as a template for 3-bit data, this step is needed to account for the small gain changes (
    115 KB (15,378 words) - 19:51, 4 February 2014
  • ...data. In that case, look at the data itself in {{plotms}} (see below for examples) to decide whether or not to apply all flags. ...libration for our 8-bit data, but if one is following this CASA Guide as a template for 3-bit data, this step is needed to account for the small gain changes (
    117 KB (15,635 words) - 13:53, 16 December 2014
  • ...e to a 5km/s channel, so we will forgo the the continuum subtraction step. Examples of how to do this if you are so inclined are located in various other ALMA The TP image is resampled onto the same grid as that of the "template" 7m+12m image along the first two axes of the cube (i.e., RA and Dec; it is
    41 KB (6,356 words) - 12:20, 29 March 2018
  • ...e to a 5km/s channel, so we will forgo the the continuum subtraction step. Examples of how to do this if you are so inclined are located in various other ALMA The TP image is resampled onto the same grid as that of the "template" 7m+12m image along the first two axes of the cube (i.e., RA and Dec; it is
    44 KB (6,778 words) - 09:53, 8 May 2018
  • ...data. In that case, look at the data itself in {{plotms}} (see below for examples) to decide whether or not to apply all flags. ...libration for our 8-bit data, but if one is following this CASA Guide as a template for 3-bit data, this step is needed to account for the small gain changes (
    125 KB (15,910 words) - 23:10, 4 June 2015
  • ...data. In that case, look at the data itself in {{plotms}} (see below for examples) to decide whether or not to apply all flags. ...libration for our 8-bit data, but if one is following this CASA Guide as a template for 3-bit data, this step is needed to account for the small gain changes (
    127 KB (16,188 words) - 17:52, 13 July 2015
  • ...e to a 5km/s channel, so we will forgo the the continuum subtraction step. Examples of how to do this if you are so inclined are located in various other ALMA The TP image is resampled onto the same grid as that of the "template" 7m+12m image along the first two axes of the cube (i.e., RA and Dec; it is
    37 KB (5,732 words) - 09:33, 10 April 2017
  • ...se, scan=True, baseband=True, clip=True, autocorr=True, hm_tbuff='1.5int', template=False, online=True, tbuff=0.0, fracspw=0.05, shadow=True, quack=True, edges In Fig. 17, we show some of gain amplitude plot examples. Antenna ea03 shows credible solutions (the colors represent different spec
    83 KB (12,631 words) - 16:13, 10 October 2016
  • '''This guide describes some examples for perfecting the interferometric imaging products from the ALMA Cycle 4 P ...EADME file. The details of the various imaging pipeline stages, as well as examples of weblog output can be found in the [http://almascience.org/documents-and-
    18 KB (2,654 words) - 15:57, 26 July 2019
  • ...edu/index.php/TWHydraBand7_Calibration_4.3 TW Hydra guide] gives some nice examples showing how to use these tasks. This guide is continued at '''[[Image_Continuum | Image the Continuum Template]]'''.
    22 KB (2,926 words) - 18:22, 24 January 2019
  • A flagging template can also be provided to the pipeline which applies known flags to the data ...are also listed and the entire MS is flagged on a 8.84% level. No flagging template was applied.
    50 KB (7,973 words) - 18:32, 2 February 2018
  • ...se, scan=True, baseband=True, clip=True, autocorr=True, hm_tbuff='1.5int', template=True, online=True, tbuff=0.0, fracspw=0.05, shadow=True, quack=True, edgesp A flagging template can also be provided to the pipeline which applies known flags to the data
    85 KB (13,006 words) - 18:57, 19 May 2017
  • '''This guide describes some examples for perfecting the interferometric imaging products from the ALMA Cycle 5 P ...QA2 report. The details of the various imaging pipeline stages, as well as examples of weblog output can be found in the [https://almascience.nrao.edu/processi
    36 KB (5,210 words) - 15:55, 26 July 2019
  • ...rences between clean and tclean, please see the guide: [[TCLEAN_and_ALMA | Examples for using the new tclean CASA task for ALMA Imaging]]. '' * [[ALMA_Imaging_Pipeline_Reprocessing | Examples for ALMA Imaging Pipeline Reprocessing]]
    8 KB (1,075 words) - 21:06, 14 December 2017
  • <font size = 3>'''[[ALMA_Imaging_Pipeline_Reprocessing | Examples for ALMA Imaging Pipeline Reprocessing]]'''</font size> * <font size = 3>'''[[ALMA_Cycle_4_Imaging_Pipeline_Reprocessing | Cycle 4 Examples]]'''</font size>
    6 KB (859 words) - 16:29, 8 January 2018
  • A flagging template can also be provided to the pipeline which applies known flags to the data ...are also listed and the entire MS is flagged on a 8.84% level. No flagging template was applied.
    52 KB (8,196 words) - 14:51, 13 February 2018
  • '''This guide describes some examples for creating the interferometric imaging products using the ALMA Cycle 5 Pi ...or manual ALMA imaging, ms.split.cal files CANNOT BE DIRECTLY USED IN THE EXAMPLES GIVEN IN THIS GUIDE.
    7 KB (962 words) - 10:56, 29 May 2018
  • '''This guide describes some examples for perfecting the interferometric imaging products from the ALMA Cycle 6 P ...for manual ALMA imaging, ms.split.cal files CANNOT BE DIRECTLY USED IN THE EXAMPLES GIVEN IN THIS GUIDE.
    35 KB (5,047 words) - 15:26, 26 July 2019
  • A flagging template can also be provided to the pipeline which applies known flags to the data ...are also listed and the entire MS is flagged on a 8.84% level. No flagging template was applied.
    59 KB (9,223 words) - 19:22, 18 June 2019
  • ...e to a 5km/s channel, so we will forgo the the continuum subtraction step. Examples of how to do this if you are so inclined are located in various other ALMA The TP image is resampled onto the same grid as that of the "template" 7m+12m image along the first two axes of the cube (i.e., RA and Dec; it is
    39 KB (6,001 words) - 12:51, 25 January 2019
  • ..., shadow=True, quack=True, edgespw=True, autocorr=True, hm_tbuff='1.5int', template=True, online=True) ...b of modeling the image than the classic clean delta function. For broader examples of many {{tclean}} options, please see the [https://casaguides.nrao.edu/ind
    130 KB (17,843 words) - 15:22, 27 September 2019