Uploads by Bemonts

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File list
Date Name Thumbnail Size Description Versions
13:24, 14 March 2018 FITS list.alma.cycle5.1.skymodel.flat.png (file) 12 KB skymodel.flat image 2
15:47, 18 August 2017 Pband delaycal.png (file) 20 KB Fig.4. Delays for each antenna and each polarization. Plot made with ‘plotcal’ 1
13:33, 14 March 2018 Complist only.alma.cycle5.1.skymodel.png (file) 22 KB Skymodel component only 1
15:47, 18 August 2017 Spec Pband plot.pdf (file) 29 KB Fig. 9. Test-data of the redshifted HI 21cm absorption line on top of the radio continuum in MG 0414+0354; see More, Carilli & Mention 1999 (Apj, 510, 87) for the original detection. 1
15:40, 18 August 2017 Pband TECIM.png (file) 38 KB Figure for P-band spectral-line guide 1
17:47, 14 December 2018 Psim2-5.4.alma.out20.skymodel.png (file) 50 KB   1
17:48, 14 December 2018 Psim2-5.4.alma.out20.observe.png (file) 71 KB   1
15:50, 18 August 2017 Spec Pband plot.png (file) 73 KB Fig.9. Test-data of the redshifted HI 21cm absorption line on top of the radio continuum in MG 0414+0354; see More, Carilli & Mention 1999 (Apj, 510, 87) for the original detection. 1
14:37, 23 January 2018 M51.alma.cycle5.3.observe.png (file) 81 KB   1
14:09, 8 March 2021 M51.alma.cycle8.3.observe.png (file) 114 KB   1
14:06, 8 March 2021 M51.aca.cycle8.observe.png (file) 124 KB   1
13:36, 14 March 2018 Complist only.alma.cycle5.1.analysis.png (file) 130 KB Analysis components only 1
13:28, 14 March 2018 FITS list.alma.cycle5.1.analysis.png (file) 149 KB Analysis image simanalyze 1
16:37, 18 August 2017 Pband phasecal.png (file) 151 KB Fig.6. Effects of phase calibration. The corrections were applied using the task “applycal” (we do not need to do this until we obtained all remaining calibration tables -- see below for details). The various colors show the different baselines wit... 1
16:32, 18 August 2017 Pband hanning.png (file) 153 KB Fig.1. Reducing the effects of Gibbs ringing by Hanning smoothing the data. Shown is only a small fraction of the band, both before and after Hanning smooth. The amplitude scale is the same in both plots. 1
16:38, 18 August 2017 Pband ampcal.png (file) 197 KB Fig.7. Effects of amplitude and flux calibration. The corrections were applied using the task “applycal” (we do not need to do this until we obtained all remaining calibration tables -- see below for details). The various colors show the different... 1
16:41, 14 December 2018 M51c.aca.i.analysis.casa5.4.png (file) 198 KB   1
17:46, 14 December 2018 Psim2-5.4.alma.out20.image.png (file) 236 KB   1
14:39, 23 January 2018 M51.concat.cycle5.image.png (file) 260 KB   1
14:41, 23 January 2018 M51.combine.cycle5.png (file) 260 KB   1
17:46, 14 December 2018 Psim2-5.4.alma.out20.analysis.png (file) 286 KB   1
13:04, 23 January 2018 M51.alma.cycle1.3.skymodel.png (file) 290 KB Hexagonal mosaic overplotted on sky model 1
14:38, 23 January 2018 M51.aca.tp.cycle5.skymodel.png (file) 334 KB   1
15:06, 8 March 2021 M51.concat.cycle8.3.image.png (file) 344 KB   1
16:44, 14 December 2018 M51c.ALMA 0.5arcsec.analysis.casa5.4.png (file) 372 KB   1
14:38, 23 January 2018 M51.aca.cycle5.skymodel.png (file) 372 KB   1
15:08, 8 March 2021 M51.combine.cycle8.3.png (file) 382 KB   1
15:02, 8 March 2021 M51.alma.cycle8.3.skymodel.png (file) 440 KB   2
16:33, 18 August 2017 Pband flagchan.png (file) 497 KB Fig.2. Flagging of calibrator 3C48. Shown are the XX and YY polarization on antenna ea01, both before and after flagging the bad channels. The colors represent the different baselines with ea01. 1
16:38, 18 August 2017 Pband sc1.png (file) 523 KB Fig.8. Continuum image of MG0414+0354 before (left) and after (right) the first iteration of self-calibration, where we only calibrated the phases. Subsequent iterations may further improve the phases and amplitudes. This image was made in the VIEWER,... 2
15:06, 8 March 2021 M51.aca.tp.cycle8.3.skymodel.png (file) 534 KB   1
15:04, 8 March 2021 M51.aca.cycle8.3.skymodel.png (file) 624 KB   2
16:39, 18 August 2017 Pband BPcal final.png (file) 2.77 MB Fig.5. Effects of bandpass calibration on the frequency-dependent amplitudes (top) and phases (bottom) across the observing band. The corrections were applied using the task “applycal” (we do not need to do this until we obtained all remaining cali... 1