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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]] |
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Tuesday/thursday 25th october 2017 : 40 position sources across the sky observed. Current model is found reasonable but Albreicht improves on it and implements modifications of P7, P10 and P11. |
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| 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]] || || === 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'''|| || 20171025s42 || FR, LP || Uranus, focus=best central - 0.2mm, v2 using CM_ONE_BLOCK || v0: FR, v2: LP || || 20171025s41 || FR, LP || Uranus, 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 || ||Mars, focus=best central - 0.3mm || || || 20171023s101 || LP || Mars, fair noise decorrelation at the first iteration || 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
Day to day observation logbook
Tuesday/thursday 25th october 2017 :
- 40 position sources across the sky observed. Current model is found reasonable but Albreicht improves on it and implements modifications of P7, P10 and P11.
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 |
20171025s42 |
FR, LP |
Uranus, focus=best central - 0.2mm, v2 using CM_ONE_BLOCK |
v0: FR, v2: LP |
20171025s41 |
FR, LP |
Uranus, 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 |
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Mars, focus=best central - 0.3mm |
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20171023s101 |
LP |
Mars, fair noise decorrelation at the first iteration |
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 |