Update on the Preliminary Design of SCALES: the Santa Cruz Array of Lenslets for Exoplanet Spectroscopy
arXiv:2012.09098
Abstract
SCALES (Santa Cruz Array of Lenslets for Exoplanet Spectroscopy) is a 2-5 micron high-contrast lenslet integral-field spectrograph (IFS) driven by exoplanet characterization science requirements and will operate at W. M. Keck Observatory. Its fully cryogenic optical train uses a custom silicon lenslet array, selectable coronagraphs, and dispersive prisms to carry out integral field spectroscopy over a 2.2 arcsec field of view at Keck with low () spectral resolution. A small, dedicated section of the lenslet array feeds an image slicer module that allows for medium spectral resolution (), which has not been available at the diffraction limit with a coronagraphic instrument before. Unlike previous IFS exoplanet instruments, SCALES is capable of characterizing cold exoplanet and brown dwarf atmospheres ( K) at bandpasses where these bodies emit most of their radiation while capturing relevant molecular spectral features.
arXiv comment24 pages, 13 figures, SPIE Astronomical Instruments and Telescopes 2020 conference
References in corpus (16)
- Detection of Carbon Monoxide and Water Absorption Lines in an Exoplanet Atmosphere
- Clouds and Chemistry in the Atmosphere of Extrasolar Planet HR8799b
- Accreting Protoplanets in the LkCa 15 Transition Disk
- Masses, Radii, and Cloud Properties of the HR 8799 Planets
- The International Deep Planet Survey I. The frequency of wide-orbit massive planets around A-stars
- Directly Imaged L-T Transition Exoplanets in the Mid-Infrared
- Observing Exoplanets with High Dispersion Coronagraphy. I. The scientific potential of current and next-generation large ground and space telescopes
- High-contrast imaging of Sirius~A with VLT/SPHERE: Looking for giant planets down to one astronomical unit
- No Clear, Direct Evidence for Multiple Protoplanets Orbiting LkCa 15: LkCa 15 bcd are Likely Inner Disk Signals
- Water vapor in the protoplanetary disk of DG Tau
- The LEECH Exoplanet Imaging Survey: Limits on Planet Occurrence Rates Under Conservative Assumptions
- The LEECH Exoplanet Imaging Survey: Characterization of the Coldest Directly Imaged Exoplanet, GJ 504 b, and Evidence for Super-Stellar Metallicity
- The Gemini NICI Planet-Finding Campaign: The Orbit of the Young Exoplanet beta Pictoris b
- Conceptual Design of the Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS) for the Subaru Telescope
- High-resolution Infrared Spectrograph for Exoplanet Characterization with the Keck and Thirty Meter Telescopes
- The Fast Atmospheric Self-Coherent Camera Technique: Laboratory Results and Future Directions