4.7 Article

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

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 507, Issue 1, Pages 350-366

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab2130

Keywords

instrumentation: detectors; instrumentation: photometers; techniques: photometric

Funding

  1. European Research Council under the European Union [340040]
  2. Science and Technology Facilities Council (STFC)
  3. State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU)
  4. European Regional Development Fund (FEDER) [AYA2017-83383-P]
  5. Ramon y Cajal Fellowships [RYC-2015-17854, RYC-2015-18148]
  6. STFC Ernest Rutherford Fellowship
  7. European Research Council (ERC) [340040] Funding Source: European Research Council (ERC)

Ask authors/readers for more resources

HiPERCAM is a portable quintuple-beam optical imager that can record images simultaneously with its five CCD cameras, allowing for both deep long-exposure imaging and high-speed imaging. Utilizing frame-transfer devices cooled thermo-electrically, it can achieve detections of astronomical sources at high precision. By combining HiPERCAM with the world's largest optical telescope, it can enhance the effective field of view and achieve detections of astronomical sources with high limits.
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 (320-1060nm) 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 183K, 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 6.7arcmin for differential photometry. Combining HiPERCAM with the world's largest optical telescope enables the detection of astronomical sources to g(s) similar to 23 in 1s and g(s) similar to 28 in 1h. In this paper, we describe the scientific motivation behind HiPERCAM, present its design, report on its measured performance, and outline some planned enhancements.

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