List of Astronomical Target for Nika Oct 2011 run3

FXD: Final version before run (12/10/2011), SL update Pako help and IRAM pointing sources (14/10/2011)

Back to the NIKA run3 page

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

Here are the ephemerides for the planets

and the other objects LST Pointing quasars Strong galactic sources Weak galactic sources External galaxies High-z galaxies Clusters of galaxies

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
• 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 + Herschel 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

6 Cluster of galaxies:

• Main target MS0451, 04h54m11.0s, -03d00'53", z=0.55, y0=3E-4, rc=60" seen by ; Bolocam, ACT, CARMA
• other targets include
  • 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).

7. Blind survey

Field coordinates

Aztec1 09h59m42.86s, +02d29'38.2", z=4.65, S1.3mm= 9.4+-1.6 mJy, S850=16mJy, Smolcic 2011, ApJL 731, L27

and/or

GN20 12h37m11.90s, +62d22'12.1", z=4.055, S850um=30mJy, 3.3mm=0.33mJy, Daddi et al 2009, ApJ, 694, 1517

Need 10x10 arcmin field with known faint sources. Hope to achieve 1mJy 1sigma in 1 hour with a 2x2 arcmin field of view (times 25 in 25h) : 25hours total

Here is the full detailed formatted list Source_list_fmt2011v2.1.txt with fluxes

Here is the catalog for Pako NIKA2011v2.1.sou.txt has to be RENAMED to NIKA.sou on the pako computer

Here is a list of IRAM pointing sources with fluxes at 3mm and 2mm (I miss fluxes at 1mm, SL) IRAM_pointing_sources_with_fluxes.xls

Here is a short manual on useful "Pako for Nika" commands Pako_helpv5.txt (updated among few other things with the correct project name for this run: t21, and warning about the need for the correct project name for NCS, and some typos)

Here is a collection of Pako scripts to gain time and have a reference on the observations we will do (to use them rename the files without the .txt, 2nd version updated with slower mapping speed to minimize tracking errors):

nini.pako.txt => run the initial series of commands that always have to be run at the beginning of an observing cession

OTF_small_resol2.pako.txt => OTFMAP 120"x60" in 12 subscan x 12 s ~= 3 min (10"/s) with 2 samples (subscan step) per convolved 1mm HPBW (for focus & quick point source)

OTF_big_resol2.pako.txt => OTFMAP 220"x220" in 55 subscan x 26 s ~= 28 min (8.5"/s) with 2.6 samples (subscan step) per convolved 1mm HPBW (for pixel map)

OTF_big_fast2.pako.txt => OTFMAP 220"x220" in 22 subscan x 20 s ~= 9 min (11"/s) with 1 sample (subscan step) per convolved 1mm HPBW @ (for quick source search pixel map)

OTF_big_extended2.pako.txt => OTFMAP 300"x300" in 50 subscan x 30 s ~= 29 min (10"/s) with 1.7 samples (subscan step) per convolved 1mm HPBW (for extended source < 5')