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Detector Array

IGRINS-2 utilizes two Teledyne HAWAII-2RG (H2RG) spectrograph detector arrays, each featuring a 2048x2048 configuration. The outer four pixels on each side are not illuminated and serve as reference pixels, resulting in an effective active area of 2040x2040 pixels. The properties of the HAWAII-2RG (H2RG) detector arrays for the IGRINS-2 are given in the table below. 

Table 1: IGRINS-2 Detector Characteristics
Detector Array Teledyne HAWAII-2RG (H2RG) HgCdTe
Pixel format 2048 x 2048 18 micron pixel
Pixel Scale 0.1"
H K
Dark Current 0.0275 e-/s/pixel 0.0221 e-/s/pixel
Gain 2.5 e-/ADU 1.7 e-/ADU
Quantum efficiency > 80% > 80%
Well depth 40,000 ADU (100,000 e-) 52,000 ADU (93,600 e-)

The H2RG detector is capable of detecting light out to 2.6 um, and employs a HgCdTe detector layer. Instead of using a traditional shutter to control exposure duration, the detector captures images by measuring the difference in signal between two readouts: one at the start and one at the end of the integration. Consequently, the minimum exposure time is constrained by the readout time. To minimize read noise, the Fowler sampling is used, which averages several reads to enhance data quality.

Table 2: IGRINS-2 Detector Read Modes*
Number of Fowler Samples Readout Time (sec) Read noise (e-)
H K
1 1.7 sec 24.8  20.1
2 3.1 sec 16.1  16.4
4 6.0 sec 12.3  12.6
8 11.9 sec 9.7  11.3
16 23.5 sec 8.1  12.0

*Improvements in detector read noise are ongoing, and the values will be updated accordingly.

Gratings

IGRINS-2 uses a silicon immersion echelle grating as the main disperser and volume phase holographic (VPH) gratings as the cross-dispersers. The instrument covers the H and K bands simultaneously in a single exposure.

H K
Central wavelength 1.65 um 2.20 um
Wavelength coverage 1.49 - 1.80 um 1.96 - 2.46 um
Spectral resolution 50,000 45,000
Orders 122 to 98 92 to 71

Slit

IGRINS-2 has a single slit with a size of 0.33" x 5".

Slit Viewing Camera (SVC)

IGRINS-2 is equipped with a Slit Viewing Camera (SVC), which considerably reduces acquisition times and permits real-time monitoring of the telescope tracking and guiding performance. 

Field of View 46" diameter
Color Filter Ks
Plate Scale 0.04 "/pixel