User contributions for Ekeller
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5 April 2017
- 11:4211:42, 5 April 2017 diff hist 0 N File:Imaging Prep Flow.png No edit summary
- 11:3711:37, 5 April 2017 diff hist +114 Imaging Prep No edit summary
- 11:3611:36, 5 April 2017 diff hist +35 Imaging Prep No edit summary
- 11:3511:35, 5 April 2017 diff hist +36 N File:Imaging Prep WorkFlow.pdf Workflow for the Imaging Prep guide. current
- 11:2611:26, 5 April 2017 diff hist +137 Self-Calibration Template CASA 6.1.1 No edit summary
- 11:2511:25, 5 April 2017 diff hist +42 N File:Plotcal image.png First round of self-cal solutions plotted. current
- 11:1111:11, 5 April 2017 diff hist +109 Self-Calibration Template CASA 6.1.1 →Self-Calibration on the Continuum (optional)
- 11:1111:11, 5 April 2017 diff hist +49 N File:Apcal.png Continuum image after amplitude self-calibration. current
- 11:0611:06, 5 April 2017 diff hist 0 Self-Calibration Template CASA 6.1.1 →Self-Calibration on the Continuum (optional)
- 11:0511:05, 5 April 2017 diff hist +128 Self-Calibration Template CASA 6.1.1 →Self-Calibration on the Continuum (optional)
- 11:0311:03, 5 April 2017 diff hist +54 N File:Pcal1.png Continuum image after first round of self-calibration. current
- 10:5410:54, 5 April 2017 diff hist +185 Image Line CASA 6.1.1 →Create Diagnostic PNGs
- 10:5310:53, 5 April 2017 diff hist +25 N File:TWHydra CO 3 2.image.mom8.png Moment 8 map of CO (3-2). current
- 10:5010:50, 5 April 2017 diff hist 0 Image Line CASA 6.1.1 →Image line emission (repeat as necessary)
- 10:4810:48, 5 April 2017 diff hist +412 Image Line CASA 6.1.1 →Image line emission (repeat as necessary)
- 10:4710:47, 5 April 2017 diff hist +36 N File:CO initial image.png Channel 54 of the dirty cube TW Hya. current
- 10:4510:45, 5 April 2017 diff hist +56 N File:TWHydra CO3 2 plotms.png Amp vs velocity plot to identify line channels to image. current
- 10:4310:43, 5 April 2017 diff hist +752 Image Continuum CASA 6.1.1 →Imaging the Continuum
- 10:4110:41, 5 April 2017 diff hist 0 N File:Final Cont residual.png No edit summary current
- 10:4010:40, 5 April 2017 diff hist 0 N File:Final Continuum Image.png No edit summary current
- 10:3710:37, 5 April 2017 diff hist +35 N File:Cont before clean mask.png Continuum image with mask overlaid. current
- 10:3410:34, 5 April 2017 diff hist +32 N File:Cont before clean.png Dirty continuum image of TW Hya. current
- 10:2910:29, 5 April 2017 diff hist 0 Imaging Prep →Regridding spectral window (optional)
- 10:2610:26, 5 April 2017 diff hist +4 Imaging Prep →Combining measurement sets from multiple executions
- 10:2410:24, 5 April 2017 diff hist +11 Imaging Prep →Flux Equalization (optional)
- 10:2310:23, 5 April 2017 diff hist +12 Image Continuum CASA 6.1.1 →Imaging the Continuum
- 10:2210:22, 5 April 2017 diff hist +2,806 Image Continuum CASA 6.1.1 No edit summary
- 09:3809:38, 5 April 2017 diff hist +427 Image Line CASA 6.1.1 →Apply a primary beam correction
- 09:3709:37, 5 April 2017 diff hist +138 N File:TW Hya Calibrated final.pbcor.png TW Hydra image after a primary beam correction is applied to correct the lower rms found at the edges of the images from the primary beam. current
- 09:3609:36, 5 April 2017 diff hist +24 N File:TW Hya Calibrated final cont.image.png TW Hydra continuum image current
- 09:2909:29, 5 April 2017 diff hist 0 File:Calibrated final AmpVsUVWave.png Ekeller uploaded a new version of "File:Calibrated final AmpVsUVWave.png" current
- 09:2909:29, 5 April 2017 diff hist 0 File:Calibrated final AmpVsUVWave.png Ekeller uploaded a new version of "File:Calibrated final AmpVsUVWave.png"
- 09:2009:20, 5 April 2017 diff hist +248 Image Continuum CASA 6.1.1 →Create an Averaged Continuum MS
- 09:1809:18, 5 April 2017 diff hist +69 N File:Calibrated final field0 spw0 LineChannelFlagged.png Line is flagged out in spw 0 in order to create continuum only image. current
- 09:1609:16, 5 April 2017 diff hist +1 Image Continuum CASA 6.1.1 →Create an Averaged Continuum MS
- 09:1509:15, 5 April 2017 diff hist +398 Image Continuum CASA 6.1.1 →Create an Averaged Continuum MS
- 09:1309:13, 5 April 2017 diff hist +53 N File:Calibrated final Field0 Spw3.png Spw 3 is a continuum window and no lines are present. current
- 09:1009:10, 5 April 2017 diff hist +78 N File:Calibrated final Field0 Spw0.png TW Hydra spw 0 amp vs channel plot can be used to identify continuum channels. current
- 09:0209:02, 5 April 2017 diff hist −240 Image Continuum CASA 6.1.1 →Image Parameters
- 09:0109:01, 5 April 2017 diff hist +234 Image Continuum CASA 6.1.1 →Image Parameters
- 08:5908:59, 5 April 2017 diff hist −12 Image Continuum CASA 6.1.1 →Image Parameters
- 08:5808:58, 5 April 2017 diff hist +62 Image Continuum CASA 6.1.1 →Image Parameters
- 08:5808:58, 5 April 2017 diff hist +432 Image Continuum CASA 6.1.1 →Image Parameters
- 08:5708:57, 5 April 2017 diff hist +26 N File:Antennae North.Cont.Dirty.smallIMSize.image.png Mosaic under padded image. current
- 08:5408:54, 5 April 2017 diff hist +30 N File:Antennae Antennae North.Cont.Dirty.image.png Correctly padded mosaic image. current
- 08:5108:51, 5 April 2017 diff hist +84 Image Continuum CASA 6.1.1 →Image Parameters
- 08:5008:50, 5 April 2017 diff hist +194 Image Continuum CASA 6.1.1 →Image Parameters
4 April 2017
- 17:0017:00, 4 April 2017 diff hist +71 N File:Calibrated final AmpVsUVWave.png Use the Amp vs UVWave plot to find the longest baseline in wavelengths.
- 16:5516:55, 4 April 2017 diff hist +2 Image Continuum CASA 6.1.1 →Image Parameters
- 16:5316:53, 4 April 2017 diff hist −11 Imaging Prep →Flux Equalization (optional)