Uploads by Estarr
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This special page shows all uploaded files.
Date | Name | Thumbnail | Size | Description | Versions |
---|---|---|---|---|---|
15:52, 25 August 2022 | Finalampfreqcal0 S 4terms.png (file) | 14 KB | gain amp vs freq cal table when 4 spix terms are used | 1 | |
13:34, 25 August 2022 | Finalampfreqcal0 S updated.png (file) | 14 KB | amp vs freq cal table when 4 spix terms are used | 1 | |
13:34, 25 August 2022 | Finalampfreqcal0 S.png (file) | 14 KB | amp vs freq cal table when only 2 spix terms are used | 1 | |
15:51, 25 August 2022 | Finalampfreqcal0 S 2terms.png (file) | 14 KB | gain amp vs freq cal table when only 2 spix terms are used | 1 | |
16:30, 4 August 2022 | Reverse BD listobs.png (file) | 15 KB | 1 | ||
15:53, 25 August 2022 | Finalamptimecal0 S 4terms.png (file) | 17 KB | gain amp vs time cal table when 4 spix terms are used | 1 | |
13:33, 25 August 2022 | Coefficients.png (file) | 18 KB | Pipeline 6.2.1, multi-band data using 4 spectral index coefficients | 1 | |
16:44, 5 August 2022 | C ramp 1.png (file) | 18 KB | flux cal models are made with narrow band data in A band, causing amp ramps in phase cal solutions | 1 | |
00:53, 1 August 2021 | 3C129 pband delays.png (file) | 19 KB | 1 | ||
15:32, 25 August 2022 | Finalamptimecal0 S.png (file) | 21 KB | 2 | ||
15:53, 25 August 2022 | Finalamptimecal0 S 2terms.png (file) | 21 KB | gain amp vs time cal table when only 2 spix terms are used | 1 | |
13:35, 25 August 2022 | Finalamptimecal0 S updated.png (file) | 21 KB | amp vs time cal table when 4 spix terms are used | 1 | |
19:32, 4 August 2022 | Compression freq.png (file) | 22 KB | VLA Pipeline 6.2.1<br /> finalcals > final amp freq cal<br /> C band compression from known 6.2 GHz microwave emitter | 1 | |
19:23, 4 August 2022 | Compression BP.png (file) | 22 KB | finalcals > BP amp solution C band compression from known 6.2 GHz microwave emitter | 1 | |
05:35, 29 December 2023 | South selfchan model 6.5.4.png (file) | 22 KB | 1 | ||
03:30, 29 December 2023 | North selfchan model 6.5.4.png (file) | 23 KB | 1 | ||
16:58, 31 July 2021 | Prebp hanning casa 5.5.0.png (file) | 25 KB | Reverted to version as of 15:23, 11 July 2019 (EDT) | 3 | |
21:03, 4 August 2022 | Spectral index fit.png (file) | 26 KB | A poor spectral index fit in S band causing discontinuous spws in amp vs freq. | 1 | |
19:32, 4 August 2022 | Compression time.png (file) | 29 KB | VLA Pipeline 6.2.1<br /> finalcals > final amp time cal<br /> C band compression from known 6.2 GHz microwave emitter | 1 | |
00:18, 1 August 2021 | 3C147 postbandpass rflag.png (file) | 31 KB | 1 | ||
01:51, 1 August 2021 | 3C129 initial bp phase.png (file) | 32 KB | 1 | ||
20:38, 31 July 2021 | 3C129 pband 3C147 prebp hanning automatic.png (file) | 32 KB | 1 | ||
01:51, 1 August 2021 | 3C129 initial bp amp.png (file) | 33 KB | 1 | ||
03:29, 1 August 2021 | 3C129 gain phase.png (file) | 33 KB | 1 | ||
19:34, 4 August 2022 | Compression SP no.png (file) | 35 KB | VLA Pipeline 6.2.1<br /> finalcals > priorcals switched power<br /> C band compression from known 6.2 GHz microwave emitter<br /> antenna with no compression for comparison | 1 | |
16:43, 4 August 2022 | Reverse BD plotsummary.png (file) | 42 KB | 1 | ||
16:59, 31 July 2021 | 3C129 pband 3C147 prebp hanning.png (file) | 43 KB | 2 | ||
17:12, 5 August 2022 | 3C286 model issue.png (file) | 49 KB | flux cal models in A config do not represent structure very well, resulting in amp vs uvwave spikes. | 1 | |
15:57, 31 July 2021 | 3C129 pband 3C147 prebp.png (file) | 53 KB | 2 | ||
20:32, 4 August 2022 | Omt reflection.png (file) | 54 KB | Standing wave between feed horn window and OMT causes sinusoidal pattern across corrected amp vs freq. | 1 | |
03:29, 1 August 2021 | 3C129 gain amp.png (file) | 54 KB | 1 | ||
16:54, 1 March 2024 | Uid A002 X215db8 X392.bpphase.6.5.4.png (file) | 57 KB | 1 | ||
17:13, 5 August 2022 | 3C286 model improved.png (file) | 58 KB | An improved flux cal model removes the amp spikes seen in amp vs uvwave. | 1 | |
20:18, 5 October 2023 | Xb.Tsys vs time.page2 6.5.4.png (file) | 65 KB | 1 | ||
16:45, 5 August 2022 | C ramp uvwave.png (file) | 72 KB | flux cal models are made with narrow band data in A band, causing amp spikes in uvwave | 1 | |
19:34, 4 August 2022 | Compression SP.png (file) | 81 KB | VLA Pipeline 6.2.1<br /> finalcals > priorcals switched power<br /> C band compression from known 6.2 GHz microwave emitter | 1 | |
18:50, 13 November 2023 | Antennae North.Cont.Dirty.image.File.Info.png (file) | 106 KB | 1 | ||
16:02, 25 August 2022 | Model 4terms.png (file) | 126 KB | gain calibrator model when 4 spix terms are used | 1 | |
22:10, 19 December 2020 | Ngc5921-gaincal.png (file) | 133 KB | 2 | ||
20:18, 5 October 2023 | Xb.Tsys vs time.page1 6.5.4.png (file) | 137 KB | 1 | ||
19:48, 9 October 2023 | Uid A002 X207fe4 X3a.wvrtsys NGC ampfreq 6.5.4.png (file) | 138 KB | 1 | ||
16:01, 25 August 2022 | Model 2terms.jpg (file) | 138 KB | gain calibrator model when only 2 spix terms are used | 1 | |
21:03, 4 August 2022 | Discontinuous spws.png (file) | 144 KB | Discontinuous spws in corrected amp vs frequency due to poor spectral index fitting. | 1 | |
19:47, 9 October 2023 | Uid A002 X207fe4 X3a.wvrtsys Titan ampfreq 6.5.4.png (file) | 152 KB | 1 | ||
19:43, 9 October 2023 | Uid A002 X1ff7b0 Xb.wvrtsys 3c279 ampuvdist 6.5.4.png (file) | 165 KB | 1 | ||
12:33, 22 March 2024 | M51c.ALMA 0.5arcsec.analysis.casa6.5.4.png (file) | 167 KB | 1 | ||
19:14, 13 October 2023 | Xb 3c279 corrected phase time 6.5.4.png (file) | 177 KB | 1 | ||
19:39, 13 October 2023 | Xb NGC corrected amp uvdist 6.5.4.png (file) | 187 KB | 1 | ||
18:36, 9 October 2023 | Uid A002 X1ff7b0 Xb ampfreq DV11 data 6.5.4.png (file) | 199 KB | 1 | ||
18:36, 9 October 2023 | Uid A002 X1ff7b0 Xb ampfreq DV11 corrected 6.5.4.png (file) | 207 KB | 1 |