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← Revision 66 as of 2014-02-18 09:01:07 ⇥
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== NIKA people on call (Telephone number) == [[http://www.iram.fr/wiki/nika2/index.php/February_6th,_2013#General_information|Telephones]] |
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TBW | |
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== Real schedule == [[http://www.iram.fr/IRAMFR/PV/sche/14/s07v1.html|Real schedule]] |
== Observing slots: Real schedule == [[http://www.iram.fr/IRAMFR/PV/sche/14/s07v2.html|Real schedule 1st week New v2]] [[http://www.iram.fr/IRAMFR/PV/sche/14/s09v1.html|Real schedule 2nd week]] |
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The calibration time, 2 hours per day from Sat 15 to Monday 17, will be used to test the standard calibration sequences. The scientific time will be managed in a common NIKA pool. Details to be given later. |
The calibration time, 5/2 hours per day from Sat 15 to Monday 17, will be used to test the standard calibration sequences. * The run7 parameters were Nasmyth (-37,-30) set Pointing (-16,-2) and p11cor, p12cor=0,0 (NasInPointingModel) with Detector 494 being the reference * Tune kids on a quasar (Track). Cross on 6 quasars with Nas=0,0: find pointing corr. (Method suggested by Juan and Carsten 16/2/2014) * Update the pointing model, ie put in the right p11cor, p12cor values as well as the elevation offset p?cor * KID optimisation * Pointliss. Focus and Focusliss * otf_geometry * Liss 5min weak source * otf_geom again * Liss 5min weak source * skydip * Check all procedures ( bright and faint sources) * Observe at least one of the brightest asteroids. Check that orbital elements are ok and that fluxes are ok. The scientific time will be managed in a common NIKA pool. [[http://www.iram.es/IRAMES/mainWiki/Continuum/PoolOrganization/1stNIKApool|Official 1st NIKA IRAM observing pool here]]. Calibration periods will be interspersed at regular intervals. Guidelines for calibration scans: * (Observer responsibility) Pointing every 1h or less. Focus every 2/4 hours, more often at sunrise and sunset. * (NIKA team responsibility t21) otf_geom every 6 hours. Skydips every 12 hours. Planet tracks are [[attachment:NIKA2014R8Planethorizon.pdf|there]]: Uranus only is useful 36.45Jy, 15.277 Jy, Neptune is too close from the Sun and Mars is too bright (875, 295 Jy) and too large (~10"). Strong point sources for focus (TBC) [[attachment:NIKA2014R8StrongSource.pdf|there]] Almost point sources for pointing and calibration [[attachment:NIKA2014R8PointingSourceCalib.pdf|there]] == Travel plans == February presence at Pico (Dash (-) is for travel on 1stDay-1, !FinalDay+1, X is night at Pico, D is for day only presence not night) and Grenoble This table is the NIKA team input table. [[NIKA/1stPool/Rooms| Here is the official room occupancy plan for external pool and IRAM observers (maintained by Israel Hermelo)]]. || '''Name @PICO''' ||'''Thu 13'''||'''Fri 14'''||'''Sat 15'''||'''Sun 16'''||'''Mon 17'''||'''Tue 18'''||'''Wed 19'''||''' Thu 20'''||'''Fri 21'''||'''Sat 22'''||'''Sun 23'''||'''Mon 24'''|| ''' Tue 25'''||''' Wed 26'''||'''Thu 27'''||'''Fri 28'''|| || Nicolas P. || || || || - || X || X || X || X || D || - || || || || || || || || Martino C. || || || || || || || || - || X || X || X || X || X || X || X || D || || Alexandre || || || || || - || X || X || X || X || X || X || X || X || - || || || || Alessandro || - || X || X || X || X || X || X || X || D || - || || || || || || || || Barbara || || || || - || X || X || X || X || D || - || || || || || || || || Laurence || || || || || || || || || || || - || X || X || X || X || D || || Juan || || || || || || || || || || || - || X || X || X || X || D || || Remi || || || || || || || || - || X || X || X || X || X || X || X || D || || Xavier || - || X || X || X || X || X || X || D || - || || || || || || || || || Nello || || || || || || || - || X || X || X || X || X || X || X || X || D || || Frederic || || || || || || - || X || X || X || X || D || || || || || || || || || || || || || || || || || || || || || || || || || Number of people || 0 || 2 || 2 || 2 || 4 || 5 || 6 || 6 || 5 || 5 || 4 || 6 || 6 || 5 || 5 || 5 || || room requirement || 0 || 1 || 1 || 1 || 3 || 3 || 3 || 3 || 3 || 3 || 2 || 3 || 3 || 3 || 3 || 3 || || '''Name @Grenoble''' ||'''13'''||'''14'''||'''Sat 15'''||'''Sun 16'''||'''17'''||'''18'''||'''19'''||'''20'''||'''21'''||'''Sat 22'''||'''Sun 23'''||'''24'''|| '''25'''||'''26'''||'''27'''||'''Fri 28'''|| || Nicolas P. || || || x || || || || || || || || X || X || X || X || X || X || || Martino C. || || X || X || - || || || || || || || || || || || || || || Andrea || || || || || || || || || || || X || X || X || X || X || X || || Alain || || X || X || X || X || X || X || X || ? || || || || || || || || || Alessandro || || || || || || || || || || || X || X || X || X || X || X || || Barbara || || || || - || || || || || || || X || X || X || X || X || X || || Juan || X || X || X || X || X || X || X || X || X || || || || || || || || || Remi || || || X || X || X || X || X || || || || || || || || || || || Xavier || || || || || || || || || || X || X || X || X || X || X || X || || Frederic || || || X || X || X || X || X || || || || || || || || || || |
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== Travel plans == TBW |
* Min room requirement gives the minimal number of room required at the telescope, implying several persons can share room in case the occupancy at the telescope is such that single rooms can't be provided to all (according to Dec 5 2013's status of the telescope room schedule everybody can have a single room). February presence at Grenoble, for offline data analysis and Real Time Support |
NIKA run #8 February 2014
Goals of the run
Scientific run including Guaranteed time proposals and open time proposals in the same NIKA pool
NIKA people on call (Telephone number)
Preparation of the run
Observing slots: Real schedule
Real schedule 1st week New v2 Real schedule 2nd week
Program
The calibration time, 5/2 hours per day from Sat 15 to Monday 17, will be used to test the standard calibration sequences.
The run7 parameters were Nasmyth (-37,-30) set Pointing (-16,-2) and p11cor, p12cor=0,0 (NasInPointingModel) with Detector 494 being the reference
- Tune kids on a quasar (Track). Cross on 6 quasars with Nas=0,0: find pointing corr. (Method suggested by Juan and Carsten 16/2/2014)
- Update the pointing model, ie put in the right p11cor, p12cor values as well as the elevation offset p?cor
- KID optimisation
- Pointliss. Focus and Focusliss
- otf_geometry
- Liss 5min weak source
- otf_geom again
- Liss 5min weak source
- skydip
- Check all procedures ( bright and faint sources)
- Observe at least one of the brightest asteroids. Check that orbital elements are ok and that fluxes are ok.
The scientific time will be managed in a common NIKA pool. Official 1st NIKA IRAM observing pool here. Calibration periods will be interspersed at regular intervals.
Guidelines for calibration scans:
- (Observer responsibility) Pointing every 1h or less. Focus every 2/4 hours, more often at sunrise and sunset.
- (NIKA team responsibility t21) otf_geom every 6 hours. Skydips every 12 hours.
Planet tracks are there: Uranus only is useful 36.45Jy, 15.277 Jy, Neptune is too close from the Sun and Mars is too bright (875, 295 Jy) and too large (~10").
Strong point sources for focus (TBC) there
Almost point sources for pointing and calibration there
Travel plans
February presence at Pico (Dash (-) is for travel on 1stDay-1, FinalDay+1, X is night at Pico, D is for day only presence not night) and Grenoble This table is the NIKA team input table. Here is the official room occupancy plan for external pool and IRAM observers (maintained by Israel Hermelo).
Name @PICO |
Thu 13 |
Fri 14 |
Sat 15 |
Sun 16 |
Mon 17 |
Tue 18 |
Wed 19 |
Thu 20 |
Fri 21 |
Sat 22 |
Sun 23 |
Mon 24 |
Tue 25 |
Wed 26 |
Thu 27 |
Fri 28 |
Nicolas P. |
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D |
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Martino C. |
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Alexandre |
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X |
X |
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X |
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Alessandro |
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Barbara |
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Laurence |
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Juan |
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Remi |
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Xavier |
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Nello |
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Frederic |
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D |
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Number of people |
0 |
2 |
2 |
2 |
4 |
5 |
6 |
6 |
5 |
5 |
4 |
6 |
6 |
5 |
5 |
5 |
room requirement |
0 |
1 |
1 |
1 |
3 |
3 |
3 |
3 |
3 |
3 |
2 |
3 |
3 |
3 |
3 |
3 |
Name @Grenoble |
13 |
14 |
Sat 15 |
Sun 16 |
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18 |
19 |
20 |
21 |
Sat 22 |
Sun 23 |
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25 |
26 |
27 |
Fri 28 |
Nicolas P. |
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x |
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X |
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Martino C. |
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X |
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Andrea |
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Alain |
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? |
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Alessandro |
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Barbara |
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Juan |
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Remi |
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Xavier |
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Frederic |
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* Min room requirement gives the minimal number of room required at the telescope, implying several persons can share room in case the occupancy at the telescope is such that single rooms can't be provided to all (according to Dec 5 2013's status of the telescope room schedule everybody can have a single room).
February presence at Grenoble, for offline data analysis and Real Time Support