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 # Planets
Mars, Venus
for photometric calibration (primary calibrators)
1. Planets
 Mars, Venus
 for photometric calibration (primary calibrators)
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 # Usual bright quasars
for image quality and linearity checks
2. Usual bright quasars
 for image quality and linearity checks
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 # List of bright ultracompact HII regions
    for photometric calibration checks (secondary calibrators)
3. 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
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'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
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 # Cluster of galaxies: RXJ1347-1145, A665, A2163 and CL0016+16 6 Cluster of galaxies: RXJ1347-1145, 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 expanded formatted list [[attachment:Source_list_fmt2010v1.txt]]

List of Astronomical Target for Nika v2 Oct 2010 run

FXD, first draft

Please feel free to add your own preference. This will be discussed in a teleconf at a later date.

1. Planets

  • Mars, Venus for photometric calibration (primary calibrators)

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'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

6 Cluster of galaxies: RXJ1347-1145, 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 expanded formatted list Source_list_fmt2010v1.txt

ListAstroTargetNika2 (last edited 2010-10-22 09:55:48 by PabloMellado)