Analysis of dark data of the PICNIC ir arrays in the CIBER

D. H. Lee; M. G. Kim; K. Tsumura; M. Zemcov; U. W. Nam; J. Bock; J. Battle; V. Hristov; T. Renbarger; T. Matsumoto; I. Sullivan; L. R. Levenson; P. Mason; S. Matsuura; G. H. Kim

doi:10.5140/JASS.2010.27.4.401

Analysis of dark data of the PICNIC ir arrays in the CIBER

D. H. Lee, M. G. Kim, K. Tsumura, M. Zemcov, U. W. Nam, J. Bock, J. Battle, V. Hristov, T. Renbarger, T. Matsumoto, I. Sullivan, L. R. Levenson, P. Mason, S. Matsuura, G. H. Kim

Creative Interdisciplinary Research Division

Research output: Contribution to journal › Article › peer-review

6 Citations (Scopus)

Abstract

We have measured and analyzed the dark data of two PICNIC IR arrays (P574 and P560) obtained through the Cosmic Infrared Background ExpeRiment (CIBER). First, we identified three types of bad pixels: the cold, the hot, and the transient, which are figured in total as 0.06% for P574 and 0.19% for P560. Then, after the bad pixels were masked, we determined the dark noise to be 20.5 ± 0.05 e- and 16.1 ± 0.05 e-, and the dark current to be 0.6 ± 0.05 e-/sec and 0.7 ± 0.05 e-/sec for P574 and P560, respectively. Finally, we discussed glitches and readout modes for a future mission.

Original language	English
Pages (from-to)	401-406
Number of pages	6
Journal	Journal of Astronomy and Space Sciences
Volume	27
Issue number	4
DOIs	https://doi.org/10.5140/JASS.2010.27.4.401
Publication status	Published - 2010 Dec

Keywords

Analysis-dark current
Detector-PICNIC
Instrument-CIBER

ASJC Scopus subject areas

Physics and Astronomy(all)
Earth and Planetary Sciences(all)

Access to Document

10.5140/JASS.2010.27.4.401

Cite this

@article{f8c89199fd624754be985dad82eff216,

title = "Analysis of dark data of the PICNIC ir arrays in the CIBER",

abstract = "We have measured and analyzed the dark data of two PICNIC IR arrays (P574 and P560) obtained through the Cosmic Infrared Background ExpeRiment (CIBER). First, we identified three types of bad pixels: the cold, the hot, and the transient, which are figured in total as 0.06% for P574 and 0.19% for P560. Then, after the bad pixels were masked, we determined the dark noise to be 20.5 ± 0.05 e- and 16.1 ± 0.05 e-, and the dark current to be 0.6 ± 0.05 e-/sec and 0.7 ± 0.05 e-/sec for P574 and P560, respectively. Finally, we discussed glitches and readout modes for a future mission.",

keywords = "Analysis-dark current, Detector-PICNIC, Instrument-CIBER",

author = "Lee, {D. H.} and Kim, {M. G.} and K. Tsumura and M. Zemcov and Nam, {U. W.} and J. Bock and J. Battle and V. Hristov and T. Renbarger and T. Matsumoto and I. Sullivan and Levenson, {L. R.} and P. Mason and S. Matsuura and Kim, {G. H.}",

year = "2010",

month = dec,

doi = "10.5140/JASS.2010.27.4.401",

language = "English",

volume = "27",

pages = "401--406",

journal = "Journal of Astronomy and Space Science",

issn = "2093-5587",

publisher = "The Korean Space Science Society",

number = "4",

}

TY - JOUR

T1 - Analysis of dark data of the PICNIC ir arrays in the CIBER

AU - Lee, D. H.

AU - Kim, M. G.

AU - Tsumura, K.

AU - Zemcov, M.

AU - Nam, U. W.

AU - Bock, J.

AU - Battle, J.

AU - Hristov, V.

AU - Renbarger, T.

AU - Matsumoto, T.

AU - Sullivan, I.

AU - Levenson, L. R.

AU - Mason, P.

AU - Matsuura, S.

AU - Kim, G. H.

PY - 2010/12

Y1 - 2010/12

N2 - We have measured and analyzed the dark data of two PICNIC IR arrays (P574 and P560) obtained through the Cosmic Infrared Background ExpeRiment (CIBER). First, we identified three types of bad pixels: the cold, the hot, and the transient, which are figured in total as 0.06% for P574 and 0.19% for P560. Then, after the bad pixels were masked, we determined the dark noise to be 20.5 ± 0.05 e- and 16.1 ± 0.05 e-, and the dark current to be 0.6 ± 0.05 e-/sec and 0.7 ± 0.05 e-/sec for P574 and P560, respectively. Finally, we discussed glitches and readout modes for a future mission.

AB - We have measured and analyzed the dark data of two PICNIC IR arrays (P574 and P560) obtained through the Cosmic Infrared Background ExpeRiment (CIBER). First, we identified three types of bad pixels: the cold, the hot, and the transient, which are figured in total as 0.06% for P574 and 0.19% for P560. Then, after the bad pixels were masked, we determined the dark noise to be 20.5 ± 0.05 e- and 16.1 ± 0.05 e-, and the dark current to be 0.6 ± 0.05 e-/sec and 0.7 ± 0.05 e-/sec for P574 and P560, respectively. Finally, we discussed glitches and readout modes for a future mission.

KW - Analysis-dark current

KW - Detector-PICNIC

KW - Instrument-CIBER

UR - http://www.scopus.com/inward/record.url?scp=84868625688&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84868625688&partnerID=8YFLogxK

U2 - 10.5140/JASS.2010.27.4.401

DO - 10.5140/JASS.2010.27.4.401

M3 - Article

AN - SCOPUS:84868625688

SN - 2093-5587

VL - 27

SP - 401

EP - 406

JO - Journal of Astronomy and Space Science

JF - Journal of Astronomy and Space Science

IS - 4

ER -

Analysis of dark data of the PICNIC ir arrays in the CIBER

Abstract

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this