Gemini Planet Imager Observational Calibrations II: Detector Performance and Calibration

被引：11

作者：

Ingraham, Patrick ^{[1
,2
]}

Perrin, Marshall D. ^{[3
]}

Sadakuni, Naru ^{[4
]}

Ruffio, Jean-Baptiste ^{[5
,6
]}

Maire, Jerome ^{[7
]}

Chilcote, Jeff ^{[8
]}

Larkin, James ^{[8
]}

Marchis, Franck ^{[5
]}

Galicher, Raphael ^{[9
]}

Weiss, Jason ^{[8
]}

机构：

[1] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA

[2] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada

[3] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[4] Gemini Observ, La Serena, Chile

[5] Carl Sagan Ctr, SETI Inst, Mountain View, CA 94043 USA

[6] Inst Super Aeronaut & Espace, Toulouse, France

[7] Univ Toronto, Dunlap Inst Astrophys, Toronto, ON M5S 3H4, Canada

[8] Univ Calif Los Angeles, Los Angeles, CA USA

[9] UPMC, Univ Paris Diderot, Observ Paris, CNRS,LESIA, F-92190 Meudon, France

来源：

GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY V | 2014年 / 9147卷

关键词：

High Contrast Imaging; Integral field spectrograph; Extrasolar planets; Infrared Detectors;

D O I：

10.1117/12.2057437

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Gemini Planet Imager is a newly commissioned facility instrument designed to measure the near-infrared spectra of young extrasolar planets in the solar neighborhood and obtain imaging polarimetry of circumstellar disks. GPI's science instrument is an integral field spectrograph that utilizes a HAWAII-2RG detector with a SIDECAR ASIC readout system. This paper describes the detector characterization and calibrations performed by the GPI Data Reduction Pipeline to compensate for effects including bad/hot/cold pixels, persistence, non-linearity, vibration induced microphonics and correlated read noise.

引用

页数：11

共 15 条

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PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2014, 111 (35) :12661-12666

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