Open Access
Proceedings of SPIE - The International Society for Optical Engineering
Performance of science grade HgCdTe H4RG-15 image sensors
Majid Zandian
1
,
Mark Farris
1
,
William McLevige
1
,
Dennis Edwall
1
,
Erdem Arkun
1
,
Eric Holland
1
,
James E. Gunn
2
,
Stephen Smee
3
,
Donald N. B. Hall
4
,
Klaus-W. Hodapp
4
,
Atsushi Shimono
5
,
Naoyuki Tamura
5
,
Micheal Carmody
1
,
John Auyeung
1
,
James W. Beletic
1
1
Teledyne Imaging Sensors (United States)
|
4
Institute for Astronomy (United States)
|
5
Kavli Institute for the Physics and Mathematics of the Universe (Japan)
|
Publication type: Proceedings Article
Publication date: 2016-08-05
SJR: 0.152
CiteScore: 0.5
Impact factor: —
ISSN: 0277786X, 1996756X
Abstract
We present the test results of science grade substrate-removed 4K×4K HgCdTe H4RG-15 NIR 1.7 μm and SWIR 2.5 μm sensor chip assemblies (SCAs). Teledyne’s 4K×4K, 15 μm pixel pitch infrared array, which was developed for the era of Extremely Large Telescopes, is first being used in new instrumentation on existing telescopes. We report the data on H4RG-15 arrays that have achieved science grade performance: very low dark current (<0.01 e-/pixel/sec), high quantum efficiency (70-90%), single CDS readout noise of 18 e-, operability >97%, total crosstalk <1.5%, well capacity >70 ke-, and power dissipation less than 4 mW. These SCAs are substrate-removed HgCdTe which simultaneously detect visible and infrared light, enabling spectrographs to use a single SCA for Visible-IR sensitivity. Larger focal plane arrays can be constructed by assembling mosaics of individual arrays.
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