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IO:I, a near-infrared camera for the Liverpool Telescope

Barnsley, RM, Jermak, HE, Steele, IA, Smith, RJ, Bates, SD and Mottram, CJ (2016) IO:I, a near-infrared camera for the Liverpool Telescope. Journal of Astronomical Telescopes, Instruments, and Systems, 2 (1). ISSN 2329-4124

1507.00906v2.pdf - Accepted Version

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IO:I is a new instrument that has recently been commissioned for the Liverpool Telescope, extending current imaging capabilities beyond the optical and into the near-infrared. Cost has been minimized by the use of a previously decommissioned instrument's cryostat as the base for a prototype and retrofitting it with Teledyne's 1.7-μm cutoff Hawaii-2RG HgCdTe detector, SIDECAR ASIC controller, and JADE2 interface card. The mechanical, electronic, and cryogenic aspects of the cryostat retrofitting process will be reviewed together with a description of the software/hardware setup. This is followed by a discussion of the results derived from characterization tests, including measurements of read noise, conversion gain, full well depth, and linearity. The paper closes with a brief overview of the autonomous data reduction process and the presentation of results from photometric testing conducted on on-sky, pipeline processed data. © 2016 Society of Photo-Optical Instrumentation Engineers (SPIE).

Item Type: Article
Additional Information: Copyright 2016 Society of Photo Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
Subjects: Q Science > QB Astronomy
Divisions: Astrophysics Research Institute
Publisher: Society of Photo Optical Instrumentation Engineers
Date Deposited: 15 Apr 2016 08:12
Last Modified: 04 Sep 2021 13:02
DOI or ID number: 10.1117/1.JATIS.2.1.015002
URI: https://researchonline.ljmu.ac.uk/id/eprint/3420
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