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Revision 1 as of 2011-09-14 10:23:27
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Revision 2 as of 2011-09-14 12:28:41
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||MARS||<)> 15:22:07.4042 ||<)> -18:57:44.888 ||<)> 4.06 * 4.04 ||<)> 106.6 Jy ||<)> 40.09 Jy ||
||URANUS ||<)> 23:52:22.9081 ||<)> -01:40:36.585 ||<)> 3.65 * 3.64 ||<)> 54.76 Jy ||<)> 20.71 Jy ||
||NEPTUNE ||<)> 21:53:45.7179 ||<)> -13:18:12.851 ||<)> 2.27 * 2.21 ||<)> 19.53 Jy ||<)> 7.39 Jy ||
||MARS||<)> 09:27:52.1030 ||<)> 16:28:10.206||<)> 5.62 * 5.59||<)> 201.1 Jy||<)> 75.6 Jy ||
||URANUS ||<)> 00:07:04.4071||<)> -00:04:03.960||<)> 3.65 * 3.54 ||<)> 53.25 Jy ||<)> 20.14 Jy ||
||NEPTUNE ||<)> 22:02:24.0220||<)> -12:36:20.471||<)> 2.27 * 2.21 ||<)> 19.53 Jy ||<)> 7.39 Jy ||
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Here are the ephemerids for planets [[attachment:Planethorizon.pdf]] Here are the ephemerids for planets [[attachment:Planethorizon2011.pdf]]
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[[attachment:NIKA2011Stronghorizon.pdf| Strong sources]]
[[attachment:NIKA2011Weakhorizon2.pdf| Weak sources]]
[[attachment:NIKA2011Stronghorizon2011.pdf| Strong sources]]
[[attachment:NIKA2011Weakhorizon2011.pdf| Weak sources]]

List of Astronomical Target for Nika Oct 2011 run3

FXD: first version before run

  • WORK IN PROGRESS (to be updated soon)

1. Planets Mars, Venus (too big, 57 arcsec), Uranus, Neptune for photometric calibration (primary calibrators)

Name

Right Ascention

Declination

Size (arcsecond diameter)

Flux @ 1.25 mm

Flux @ 2.05 mm

MARS

09:27:52.1030

16:28:10.206

5.62 * 5.59

201.1 Jy

75.6 Jy

URANUS

00:07:04.4071

-00:04:03.960

3.65 * 3.54

53.25 Jy

20.14 Jy

NEPTUNE

22:02:24.0220

-12:36:20.471

2.27 * 2.21

19.53 Jy

7.39 Jy

Here are the ephemerids for planets Planethorizon2011.pdf

and the other objects LST Strong sources Weak sources

2. Usual bright quasars

  • for image quality and linearity checks

3. List of bright ultracompact HII regions

  • for photometric calibration checks (secondary calibrators)

4. Extended emission from

  • Herschel new sources
  • Archeops bright cores
  • bright galaxies M87 (again), M82, others
  • less bright NGC1068 22mJy at 1.3mm rising to 36 at 3mm
  • --> Need fast speed scanning to reduce 1/f residual noise

5. Faint quasars in the 10 mJy range at 1mm (use Omont&Cox list pcox_IiAHPe_dec03_p5.pdf):

  • test detectability in faint source mode: e.g.
  • J075618.14+410408.6 z= 5.09 20.15 1.3 mm 5.5 ± 0.5 Wang et al 2008, ApJ, 135, 1201
  • J092721.82+200123.7 z= 5.77 19.87g 1.3 mm 5.0 ± 0.8 mJy 3.5 mm: 0.12 ± 0.03 mJy
  • IRAS F10214+4724 = SDSS J102434.56+470909.5 1.3mm: 10 mJy
  • H1413+517 14h15m46.240s +11d29m43.40s z=2.558 1.3mm 18+-2 mJy

6 Cluster of galaxies: RXJ1347-1145 (maybe too close to the sun), A665, A2163 and CL0016+16

  • If sensitivity allows demonstrate the ability to map clusters (one of the main scientific goals of this camera).

Here is the full detailed formatted list Source_list_fmt2011v1.txt with fluxes

Here is the catalog for Pako NIKAv8.sou.txt has been RENAMED to NIKA.sou on the pako computer

Here is a short manual on useful "Pako for Nika" commands Pako_helpv2.txt

ListAstroTargetNika3 (last edited 2011-10-24 01:14:59 by NikaBolometer)