The MKID exoplanet camera for Subaru SCEXAO

Alexander B. Walter, Neelay Fruitwala, Sarah Steiger, John I. Bailey, Nicholas Zobrist, Noah Swimmer, Isabel Lipartito, Jennifer Pearl Smith, Seth R. Meeker, Clint Bockstiegel, Gregoire Coiffard, Rupert Dodkins, Paul Szypryt, Kristina K. Davis, Miguel Daal, Bruce Bumble, Giulia Collura, Olivier Guyon, Julien Lozi, Sebastien VievardNemanja Jovanovic, Frantz Martinache, Thayne Currie, Benjamin A. Mazin

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

We present the MKID Exoplanet Camera (MEC), a z through J band (800–1400 nm) integral field spectrograph located behind The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) at the Subaru Telescope on Maunakea that utilizes Microwave Kinetic Inductance Detectors (MKIDs) as the enabling technology for high contrast imaging. MEC is the first permanently deployed near-infrared MKID instrument and is designed to operate both as an IFU, and as a focal plane wavefront sensor in a multi-kHz feedback loop with SCExAO. The read noise free, fast time domain information attainable by MKIDs allows for the direct probing of fast speckle fluctuations that currently limit the performance of most high contrast imaging systems on the ground and will help MEC achieve its ultimate goal of reaching contrasts of 10−7 at 2λ/D. Here we outline the instrument details of MEC including the hardware, firmware, and data reduction and analysis pipeline. We then discuss MEC’s current on-sky performance and end with future upgrades and plans.

Original languageEnglish (US)
Article number125005
Pages (from-to)1-13
Number of pages13
JournalPublications of the Astronomical Society of the Pacific
Volume132
Issue number1018
DOIs
StatePublished - 2020
Externally publishedYes

Keywords

  • Astronomical detectors (84)
  • Astronomical instrumentation (799)
  • Unified Astronomy Thesaurus concepts: Direct imaging (387)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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