The following table has been taken partly from the original
NIRC2 proposal by Keith Matthews and Tom Soifer, and partly from
information on the as-built instrument.
| Input f/ ratio |
f/15 |
| Wavelength range |
0.9-5.3 microns |
|
Field of view
|
-
Narrow camera: 10x10 arcsec
-
Medium camera: 20x20 arcsec
-
Wide camera: 40x40 arcsec
|
|
Pixel scale
|
-
Narrow camera: 0.009942 arcsec/pixel
(+/- 0.00005")
-
Medium camera: 0.019829 arcsec/pixel
-
Wide camera: 0.039686 arcsec/pixel
|
|
Filters
|
z, Y, J, H, K, Ks, Kp, Lw, Lp, Ms, HeI, Pa_gamma, Jcont,
Pa_beta, H_cont, CH4S, H2, Fe II, CH4L, Br_gamma, Kcont,
CO, H2O, PAH, Br_alpha, Br_alpha_cont
|
|
Pupil masks
|
-
1 circular fixed, circumscribes the telescope pupil.
-
1 hexagonal fixed, inscribes the telescope pupil and
masks spiders. Needs to be used in vertical angle
mode, i.e. telescope following pupil.
-
1 circular rotating, inscribes the telescope pupil and
masks the spiders.
-
3 hexagonal, rotating.
|
|
Slits
|
Slit widths: 10, 20, 30, 40, 60, 80, 120, and 160 milliarcsec
|
|
Coronagraphy
|
-
Circular Lyot stops: 100, 150, 200, 300, 400, 600, 800,
1000, 1500, 2000 milliarcsec
-
Vortex coronagraphs: L/M-band optimized (vortexlm),
K-band optimized (vortexk)
|
|
Grisms
|
-
Low resolution (lowres): Resolving power per pixel in
K with the narrow camera: 10,200
-
Medium resolution (medres): Resolving power per pixel
in K with the narrow camera: 17,300
|
|
Detector
|
-
1024x1024 InSb Aladdin-III array, 27 micron pixels
-
32 simultaneous outputs, grouped in 8 pixels across a
row in each of 4 quadrants
-
Subarray capability down to 32x120 pix
-
Nominal operating temperature: 29 K
-
Gain:
-
Prior to Nov 20, 2023 (transputers): 4 e-/DN
-
Nov 20, 2023 and after (Archon): 8 e-/DN
|
|
Detector readout modes
|
-
Single (sampmode 1): Single read. Used for
engineering purposes.
-
CDS (sampmode 2): Correlated Double
Sampling. One read pair. Normally used for bright
targets and/or high background conditions that require
the minimum integration time for a give sub-array
size.
-
MCDS (sampmode 3 N): Multiple Correlated
Double Sampling. Multiple read pairs (N is
the number of read pairs). Used for faint targets
and/or low background conditions. The readnoise
decreases approximately as 1 over the square root of
the number of read pairs.
-
UTR (sampmode 4 N): Sampling Up The
Ramp. Experimental mode available with the Archon
controller after November 20, 2023. N is
the number of samples up the ramp.
|
|
Minimum frame time
|
-
Prior to Nov 20, 2023 (transputers): 0.182 sec, full
frame in CDS mode
-
Nov 20, 2023 and after (Archon): 0.170 sec, full frame
in CDS mode
|
|
Read noise
|
-
Prior to Nov 20, 2023 (transputers):
-
CDS (sampmode 2): ~45 – 50 e-
-
MCDS with 16 read pairs (sampmode 3 16): ~15 e-
-
Nov 20, 2023 and after (Archon):
-
CDS (sampmode 2): ~45 – 50 e-
-
MCDS with 16 read pairs (sampmode 3 16): ~15 e-
|
|
Dark current
|
< 0.1 electrons/pixel/sec
|
|
QE
|
80% at 1.7 microns
|
|
Well depth
|
-
Prior to Nov 20, 2023 (transputers): ~9,000 DN at ~1%
linearity
-
Nov 20, 2023 and after (Archon): ~4,500 DN at ~1%
linearity
|