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Performance of Science Grade HgCdTe H4RG-15 Image Sensors

Author(s): Zandian, Majid; Farris, Mark; McLevige, William; Edwall, Dennis; Arkun, Erdem; et al

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dc.contributor.authorZandian, Majid-
dc.contributor.authorFarris, Mark-
dc.contributor.authorMcLevige, William-
dc.contributor.authorEdwall, Dennis-
dc.contributor.authorArkun, Erdem-
dc.contributor.authorHolland, Eric-
dc.contributor.authorGunn, James E-
dc.contributor.authorSmee, Stephen-
dc.contributor.authorHall, Donald NB-
dc.contributor.authorHodapp, Klaus W-
dc.contributor.authorShimono, Atsushi-
dc.contributor.authorTamura, Naoyuki-
dc.contributor.authorCarmody, Michael-
dc.contributor.authorAuyeung, John-
dc.contributor.authorBeletic, James W-
dc.date.accessioned2022-01-25T15:00:34Z-
dc.date.available2022-01-25T15:00:34Z-
dc.date.issued2016en_US
dc.identifier.citationZandian, Majid, Farris, Mark, McLevige, William, Edwall, Dennis, Arkun, Erdem, Holland, Eric, Gunn, James E, Smee, Stephen, Hall, Donald NB, Hodapp, Klaus W, Shimono, Atsushi, Tamura, Naoyuki, Carmody, Michael, Auyeung, John, Beletic, James W. (2016). Performance of Science Grade HgCdTe H4RG-15 Image Sensors. HIGH ENERGY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY VII, 9915 (10.1117/12.2233664en_US
dc.identifier.issn0277-786X-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1fq9q50q-
dc.description.abstractWe present the test results of science grade substrate-removed 4Kx4K HgCdTe H4RG-15 NIR 1.7 mu m and SWIR 2.5 mu m sensor chip assemblies (SCAs). Teledyne’s 4Kx4K, 15 mu m 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.en_US
dc.language.isoen_USen_US
dc.relation.ispartofHIGH ENERGY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY VIIen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titlePerformance of Science Grade HgCdTe H4RG-15 Image Sensorsen_US
dc.typeConference Articleen_US
dc.identifier.doidoi:10.1117/12.2233664-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/conference-proceedingen_US

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