NIRC2 Modes and Instrument Properties

Modes

NIRC2 has two basic modes:

  • Near-IR Imaging
  • Near-IR Grism Spectoscopy

Each of the basic modes can be in either Polarimetry mode, or Non-Polarimetry denoted as Standard mode.

Table 1 provides a summary of these modes and characteristics of NIRC2.

Table1: Modes

Mode Image or Dispersion Chracteristics
Near-IR Imaging Imaging 0.96 - 5.0 μm
Narrow: 10" x 10", 0.01"/pix
Medium: 20" x 20", 0.02"/pix
Wide: 40" x 40", 0.04"/pix
Coronagraphy: 10 spots: 0.1" - 2"
Polarimetry: linear, Wollaston prism, J, H, K, Ks, Kp, Lp, Narrow: 5" x 10"
Near-IR Grism Spectroscopy Low & medium dispersion 1 - 5.0 μm
R~ 650 - 19,400
10 slits: 10 - 160 mas widths
Polarimetry: linear, Wollaston prism, 1 - 2.4, 3.4 - 4.1 μm

Instrument Properties

Table 2 shows the current general specifications for NIRC2. For more informaiton, check the Instrument and Data Format and the NIRC2 webpage.

Table2: General Specifications

Property Value
Input f/ ratio f/15N
Wavelength range 0.9-5.3 microns
Field of view 10x10 arcsec
20x20 arcsec
40x40 arcsec
Pixel scale

0.01 arcsec/pixel
0.02 arcsec/pixel
0.04 arcsec/pixel

Filters Z, Y, J, H, K, Ks, Kp, Lw, Lp, Ms, HeIA, HeIB, Pa_gamma, Jcont, Pa_beta, Hcont, H2, CH4S, CH4L, Fe II, Kcont, CO, H2O, PAH, Br_alpha, Br_alpha_cont
Pupil mask two circular fixed,
four hexagonal, rotating
Slits 10, 20, 30, 40, 60, 80, 120, and 160 milliarcsec
Coronagraphic spots circular: 100, 150, 200, 300, 400, 600, 800, 1000, 1500, 2000 milliarcsec
Grisms medres and lowres grisms (see tables 2 & 3), pupil imaging lens, and clear (imaging mode).
Polarimetric imaging field of view 5x10 arcsec
Polarimetric imaging filters J, H, K, Ks, Kp, Lp
Polarimetric spectroscopy 1.0 - 2.4, 3.4 - 4.1 μm
Polarization analyzer Wollaston prism, dual beam
Polarization modulator Rotating half-wave plate; science obs. typically: 0, 45, 22.5, 67.5 deg; calibrations: 0 - 180 deg in steps of 10 or 15 deg
Polarization unsuitable for High precision, less than 0.1%
Minimum frame time 0.182 sec, full frame
Detector 1024x1024 InSb Aladdin-3 array, 27 micron pixels
32 simultaneous outputs, grouped in 8 pixels across a row in each of 4 quadrants
gain ~ 5 electrons/DN
subarray capability
35 K operating temperature
Read noise 38 electrons/read
11.5 DN/sqrt(N) for N samples in MCDS mode, up to N = 64, dropping more slowly beyond that until at least N = 512. (Note that N = 2 corresponds to two reads, or CDS mode.)
Dark current < 0.1 electrons/pixel/sec
QE 80% at 1.7 microns
Well depth 100,000 electrons (at 1% linearity)