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| [[Nika2Run11|Back to the NIKA2 run 12]] | [[http://www.iram.es/IRAMES/mainWiki/Continuum/NIKA2/Main#s17_pool:_24-31_October_2017|Back to the NIKA2 1st Science pool]] New frequency sweep done at beginning of the run on A2 => new KID numbering, the ref pix is now 824 (it's the same as in previous run, but its number was 823). No new freq sweep on A1 & A3; but several KIDs that were not usable previously are now usable (thanks to relatively low stable tau). Pointing array: A2 (pix 824). Focus array: A1. |
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'''Table for gain curve task (3C84, i.e. 0316+413 in nikas-17)''' || Dates || UT || scan # || elevation || comment || || 25-10-2017 || 4:00 || 50 || 58d || otf 8x4 || || 25-10-2017 || 5:36 || 70 || 40d || otf ?? || || 26-10-2017 || 19:56 || 254 || 31d || otf 8x5 || || 26-10-2017 || 22:51 || 316 || 63d || otf 8x5 || '''Thursday 27th october 2017''' Beammap on Uranus s49 elev=40deg tau=0.25 stable Gain curve task : 3C84 (0316+413) see table above. '''Tuesday/wednesday 25/26th october 2017''' 40 position sources across the sky observed. Current model is found reasonable but Albrecht improves on it and implements modifications of P7, P10 and P11. |
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| Gain curve task : 3C84 (0316+413) see table above. Use [[https://tapas.iram.es/tapas/ | TAPAS]] login with the project account nikas-17 by default. |
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| || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171021.html|Pipeline logbook 2017/10/21]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171022.html|Pipeline logbook 2017/10/22]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171023.html|Pipeline logbook 2017/10/23]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171024.html|Pipeline logbook 2017/10/24]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171025.html|Pipeline logbook 2017/10/25]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171026.html|Pipeline logbook 2017/10/26]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171027.html|Pipeline logbook 2017/10/27]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171028.html|Pipeline logbook 2017/10/28]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171029.html|Pipeline logbook 2017/10/29]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171030.html|Pipeline logbook 2017/10/30]] || || || [[https://www.iram.es/mrt-lx1/mrt/ncs/monitor/Nika2Logbook/logbook_20171031.html|Pipeline logbook 2017/10/31]] || || === Beammap analysis status === The table below gathers the beammap scan ID, comments related either to the observing condition or to the reduced beammap quality and the analysis status Status "done" means the analysis is completed, namely the kidpar file is produced using a 2-step iteration analysis, and uploaded in SVN. || '''Scan ID''' || '''analyser initials''' || '''comments''' || '''status''' || || 20171030s268 || || Uranus, obs. date is 11:15 p. m., elev about 60 deg, finished 30 min. before a crash of the main pump || || || 20171029s266 || LP || Uranus, obs. date about midnight, elev below 60 deg, v0 done || || || 20171028s310 || LP || Uranus, obs. date about 11:30 p. m., elev about 60 degrees. Analysis: fwhm ok, meyckey's ears visible || done || || 20171028s58 || LP || Uranus, obs. date about 3 a. m., elev. starting at 33 deg (setting), focus stable, analysis v0: some instabilities on A1, beams larger and more elliptical wrt the ref. kidpar. Large beam confirmed for v2 || done || || 20171027s49 || LP || Uranus, obs. date = 3 a.m., elev about 30 deg, focus stable, v0: sizeable amount of 'double' found || done || || 20171025s42 || FR, LP || Uranus, obs. date about 3 a.m., elev. from 32 deg., focus=best central - 0.2mm, v2 using CM_ONE_BLOCK || v0: FR, v2: LP || || 20171025s41 || FR, LP || Uranus, obs. date about 2:30 a.m., elev. from 37 deg., focus=best central - 0.3mm, v2 using CM_ONE_BLOCK || v0: FR, v2: LP || || 20171024s106 || ||Mars, focus=best central - 0.2mm, observed during the sunrise, large focus drift || || || 20171024s105 || LP ||Mars, focus=best central - 0.3mm, beams a bit large at 1mm (>12arcsec) || done || || 20171023s101 || LP || Mars, fair noise decorrelation at the first iteration, v2 also done || done || || 20171022s158 || LP || Mars, should be the best ever ! :), fair noise decorrelation at the first iteration, hint of a focus drift (due to sunrise) || done || || 20171021s218 || || Mars, || || || 20171021s167 || || Mars, || || || 20171020s93 || NP || Mars, should be well focused, used for kidpar_N2R12_v0.fits || done || |
Back to the NIKA2 1st Science pool
New frequency sweep done at beginning of the run on A2 => new KID numbering, the ref pix is now 824 (it's the same as in previous run, but its number was 823). No new freq sweep on A1 & A3; but several KIDs that were not usable previously are now usable (thanks to relatively low stable tau).
Pointing array: A2 (pix 824). Focus array: A1.
Day to day observation logbook
Table for gain curve task (3C84, i.e. 0316+413 in nikas-17)
Dates |
UT |
scan # |
elevation |
comment |
25-10-2017 |
4:00 |
50 |
58d |
otf 8x4 |
25-10-2017 |
5:36 |
70 |
40d |
otf ?? |
26-10-2017 |
19:56 |
254 |
31d |
otf 8x5 |
26-10-2017 |
22:51 |
316 |
63d |
otf 8x5 |
Thursday 27th october 2017
Beammap on Uranus s49 elev=40deg tau=0.25 stable
Gain curve task : 3C84 (0316+413) see table above.
Tuesday/wednesday 25/26th october 2017
40 position sources across the sky observed. Current model is found reasonable but Albrecht improves on it and implements modifications of P7, P10 and P11.
Gain curve task : 3C84 (0316+413) see table above.
Use TAPAS login with the project account nikas-17 by default.
Link to daily pipeline logbook |
Link to manual logbook |
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Beammap analysis status
The table below gathers the beammap scan ID, comments related either to the observing condition or to the reduced beammap quality and the analysis status
Status "done" means the analysis is completed, namely the kidpar file is produced using a 2-step iteration analysis, and uploaded in SVN.
Scan ID |
analyser initials |
comments |
status |
20171030s268 |
|
Uranus, obs. date is 11:15 p. m., elev about 60 deg, finished 30 min. before a crash of the main pump |
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20171029s266 |
LP |
Uranus, obs. date about midnight, elev below 60 deg, v0 done |
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20171028s310 |
LP |
Uranus, obs. date about 11:30 p. m., elev about 60 degrees. Analysis: fwhm ok, meyckey's ears visible |
done |
20171028s58 |
LP |
Uranus, obs. date about 3 a. m., elev. starting at 33 deg (setting), focus stable, analysis v0: some instabilities on A1, beams larger and more elliptical wrt the ref. kidpar. Large beam confirmed for v2 |
done |
20171027s49 |
LP |
Uranus, obs. date = 3 a.m., elev about 30 deg, focus stable, v0: sizeable amount of 'double' found |
done |
20171025s42 |
FR, LP |
Uranus, obs. date about 3 a.m., elev. from 32 deg., focus=best central - 0.2mm, v2 using CM_ONE_BLOCK |
v0: FR, v2: LP |
20171025s41 |
FR, LP |
Uranus, obs. date about 2:30 a.m., elev. from 37 deg., focus=best central - 0.3mm, v2 using CM_ONE_BLOCK |
v0: FR, v2: LP |
20171024s106 |
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Mars, focus=best central - 0.2mm, observed during the sunrise, large focus drift |
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20171024s105 |
LP |
Mars, focus=best central - 0.3mm, beams a bit large at 1mm (>12arcsec) |
done |
20171023s101 |
LP |
Mars, fair noise decorrelation at the first iteration, v2 also done |
done |
20171022s158 |
LP |
Mars, should be the best ever ! :), fair noise decorrelation at the first iteration, hint of a focus drift (due to sunrise) |
done |
20171021s218 |
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Mars, |
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20171021s167 |
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Mars, |
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20171020s93 |
NP |
Mars, should be well focused, used for kidpar_N2R12_v0.fits |
done |