Si:As IBC array performance for SIRTF/IRAC
Si:As IBC array performance for SIRTF/IRAC
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Si:作为 SIRTF/IRAC 的 IBC 阵列性能
DOI:
10.1117/12.406573
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发表时间:
2000
期刊:
影响因子:
--
通讯作者:
M. Jhabvala
中科院分区:
文献类型:
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作者:
R. Mcmurray;Roy R. Johnson;C. Mccreight;M. Mckelvey;J. Garnett;A. Hoffman;N. Lum;W. Lum;Michael S. Smith;K. Sparkman;Andrew G. Toth;G. Domingo;D. Krebs;M. Jhabvala
The goal of achieving background-limited performance in SIRTF's cryogenic telescope environment places stringent demands on focal plane sensitivity. SIRTF's prime imaging instrument, the InfraRed Array Camera (IRAC), employs 256 X 256 Si:As Impurity-Band Conduction (IBC) arrays for its two longest wavelength channels at 5.8 micrometers and 8.0 micrometers . Background-limited performance is achieved at very low levels of zodiacal background radiation with cryo-optimized readout and detector technology from Raytheon. Presented here are performance measurements of IRAC flight candidate IBC arrays. Operating at a temperature of 6 K, these devices meet all IRAC sensitivity requirements, with dark currents well below the 10 e-/s specification, Fowler-sampled noise levels of 16 e-, and excellent photometric stability.