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IRCS Basic Instrument Parameters

IRCS consists of two arrays. The "Camera" detector is used for imaging and grism spectroscopy. The detector on the "Spectrograph" side is used when a high-resolution spectrum is obtained with the echelle mode. The imaging mode provides two different pixel scale modes, 20 and 52 mas per pixel (due to the installation of the fiber injection module for IRD, 12 mas pixel-scale mode has been suspended).

Camera Spectrograph
Detector both ALADDIN III 10242 InSb array
Pixel size both 27 μm
Pixel scale
w/o AO High (20 mas): 20.42±0.07 mas
Low (52 mas): 52.42±0.07 mas
54.57 x 67.75 mas (slit-length direction x slit-width direction)
w AO High (20 mas): 20.57±0.04 mas
Low (52 mas): 52.77±0.04 mas
54.93 x 68.20 mas (slit-length direction x slit-width direction)
Field of view
w/o AO High (20 mas): 20.91"2
Low (52 mas): 53.68"2
3.5-9.4'' (in slit-length direction)
w AO High (20 mas): 21.06"2
Low (52 mas): 54.04"2
3.5-9.4'' (in slit-length direction)
Gain 5.6 e-/ADU 3.8 e-/ADU
Dark current 0.1 e-/s 0.05 e-/s
Read noise per NDR(1) 43 e- rms 68 e- rms
Saturation level 123 000 e- 129 000 e-
Readout rate(2) both 0.41 s (standard), 0.12 s (fast)

(1) Readout noise for frame = [Readout noise per NDR] / sqrt(NDR)
(2) For full array size (1K x 1K)

Note: If you need old parameters before July 2005 when IRCS was mounted on Cassegrain focus, please see old parameter page.