HiPERCAM: a quintuple-beam, high-speed optical imager on the 10.4-m Gran Telescopio Canarias

Author:

Dhillon V S12ORCID,Bezawada N3,Black M4,Dixon S D1,Gamble T1,Gao X4,Henry D M4,Kerry P1,Littlefair S P1,Lunney D W4,Marsh T R5,Miller C4,Parsons S G1ORCID,Ashley R P5,Breedt E6ORCID,Brown A1ORCID,Dyer M J1ORCID,Green M J5ORCID,Pelisoli I5ORCID,Sahman D I1,Wild J1ORCID,Ives D J3,Mehrgan L3,Stegmeier J3,Dubbeldam C M7,Morris T J7,Osborn J7ORCID,Wilson R W7ORCID,Casares J28,Muñoz-Darias T28ORCID,Pallé E28,Rodríguez-Gil P28,Shahbaz T28ORCID,Torres M A P28ORCID,de Ugarte Postigo A9,Cabrera-Lavers A102,Corradi R L M102,Domínguez R D102,García-Alvarez D102

Affiliation:

1. Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, UK

2. Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain

3. European Southern Observatory, D-85748 Garching bei München, Germany

4. UK Astronomy Technology Centre, Royal Observatory Edinburgh, Edinburgh EH9 3HJ, UK

5. Department of Physics, University of Warwick, Coventry CV4 7AL, UK

6. Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK

7. Department of Physics, University of Durham, Durham DH1 3LE, UK

8. Departamento de Astrofísica, Universidad de La Laguna s/n, E-38206 La Laguna, Tenerife, Spain

9. Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, E-18008 Granada, Spain

10. GRANTECAN, Cuesta de San José s/n, E-38712 Breña Baja, La Palma, Spain

Abstract

ABSTRACT HiPERCAM is a portable, quintuple-beam optical imager that saw first light on the 10.4-m Gran Telescopio Canarias (GTC) in 2018. The instrument uses re-imaging optics and four dichroic beamsplitters to record $u_{\rm s}\, g_{\rm s}\, r_{\rm s}\, i_{\rm s}\, z_{\rm s}$ (320–1060 nm) images simultaneously on its five CCD cameras, each of 3.1-arcmin (diagonal) field of view. The detectors in HiPERCAM are frame-transfer devices cooled thermo-electrically to 183 K, thereby allowing both long-exposure, deep imaging of faint targets, as well as high-speed (over 1000 windowed frames per second) imaging of rapidly varying targets. A comparison-star pick-off system in the telescope focal plane increases the effective field of view to 6.7 arcmin for differential photometry. Combining HiPERCAM with the world’s largest optical telescope enables the detection of astronomical sources to gs ∼ 23 in 1 s and gs ∼ 28 in 1 h. In this paper, we describe the scientific motivation behind HiPERCAM, present its design, report on its measured performance, and outline some planned enhancements.

Funder

European Research Council

Science and Technology Facilities Council

FEDER

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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