|
Size: 1167
Comment:
|
Size: 2255
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 1: | Line 1: |
| = List of Astronomical Target for Nika v2 Oct 2010 run = FXD, first draft |
= List of Astronomical Target for Nika Oct 2010 run2 = FXD: final version before run, SL: update sources list files with few more entries, and correct some coordinates (18/10/10) |
| Line 4: | Line 4: |
| Please feel free to add your own preference. This will be discussed in a teleconf at a later date. | 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) |
| Line 6: | Line 9: |
| # Planets Mars, Venus 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 |
| Line 10: | Line 14: |
| # Usual bright quasars for image quality and linearity checks |
Here are the ephemerids for planets [[attachment:Planethorizon.pdf]] |
| Line 13: | Line 16: |
| # List of bright ultracompact HII regions for photometric calibration checks (secondary calibrators) |
and the other objects LST [[attachment:NIKA2010Stronghorizon.pdf| Strong sources]] [[attachment:NIKA2010Weakhorizon2.pdf| Weak sources]] |
| Line 16: | Line 20: |
| # 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 |
| Line 23: | Line 34: |
| # 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 |
| Line 32: | Line 41: |
| # 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 full detailed formatted list [[attachment:Source_list_fmt2010v7.txt]] with fluxes Here is the catalog for Pako [[attachment:NIKAv7.sou.txt]] has been RENAMED to NIKA.sou on the pako computer Here is a short manual on useful "Pako for Nika" commands [[attachment:Pako_helpv2.txt]] |
List of Astronomical Target for Nika Oct 2010 run2
FXD: final version before run, SL: update sources list files with few more entries, and correct some coordinates (18/10/10)
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 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_fmt2010v7.txt with fluxes
Here is the catalog for Pako NIKAv7.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