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| Deletions are marked like this. | Additions are marked like this. |
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| FXD, first draft | FXD, second expanded version |
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| Please feel free to add your own preference. This will be discussed in a teleconf at a later date. | Please feel free to add your own preference. Send me your comments. |
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| # Planets Mars, Venus for photometric calibration (primary calibrators) |
1. Planets Mars (4.06*4.04 arcsecond diameter, ), Venus (too big, 57 arcsec), Uranus ( 3.65 * 3.64), Neptune (2.27 * 2.21) for photometric calibration (primary calibrators) Typical coordinates and fluxes at 1.25 and 2.05 mm bands MARS RA 15:22:07.4042 Dec -18:57:44.888 106.6 40.09 Jy URANUS RA 23:52:22.9081 Dec -01:40:36.585 54.76 20.71 NEPTUNE RA 21:53:45.7179 Dec -13:18:12.851 19.53 7.39 |
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| # Usual bright quasars for image quality and linearity checks |
Here are the ephemerids for planets [[attachment:Planethorizon.pdf]] and the other objects LST [[attachment:NIKA2010horizon.pdf]] |
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| # List of bright ultracompact HII regions for photometric calibration checks (secondary calibrators) |
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| # 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 |
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 |
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| # Faint quasars in the 10 mJy range at 1mm (use Omont's list): 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 |
5. Faint quasars in the 10 mJy range at 1mm (use Omont&Cox list [[attachment: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 |
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| # Cluster of galaxies: RXJ1347-1145, A665, A2163 and CL0016+16 | 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 detailed formatted list [[attachment:Source_list_fmt2010v3.txt]] with fluxes Here is the catalog for Pako [[attachment:NIKAv3.sou.txt]] should be RENAMED to NIKA.sou Here is a short manual on useful Pako for Nika commands [[attachment:Pako.txt]] |
List of Astronomical Target for Nika v2 Oct 2010 run
FXD, second expanded version
Please feel free to add your own preference. Send me your comments.
1. Planets
- Mars (4.06*4.04 arcsecond diameter, ), Venus (too big, 57 arcsec),
Uranus ( 3.65 * 3.64), Neptune (2.27 * 2.21)
- for photometric calibration (primary calibrators)
Typical coordinates and fluxes at 1.25 and 2.05 mm bands MARS RA 15:22:07.4042 Dec -18:57:44.888 106.6 40.09 Jy URANUS RA 23:52:22.9081 Dec -01:40:36.585 54.76 20.71 NEPTUNE RA 21:53:45.7179 Dec -13:18:12.851 19.53 7.39
Here are the ephemerids for planets Planethorizon.pdf and the other objects LST NIKA2010horizon.pdf
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 detailed formatted list Source_list_fmt2010v3.txt with fluxes
Here is the catalog for Pako NIKAv3.sou.txt should be RENAMED to NIKA.sou
Here is a short manual on useful Pako for Nika commands Pako.txt