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SCALES Status Report

  • R. Deno Stelter
  • , Andrew J. Skemer
  • , Stephanie Sallum
  • , Nicholas MacDonald
  • , Renate Kupke
  • , Christopher Ratliff
  • , Cyril Bourgenot
  • , Gerald Cabak
  • , Michael Gonzales
  • , Cristian A. Rodriguez
  • , Aaron Hunter
  • , Ravinder Banyal
  • , Sivarani Thirupathi
  • , Michael P. Fitzgerald
  • , Marc Kassis
  • , Olivier Absil
  • , Carlos Alvarez
  • , Natasha Batalha
  • , Marc André Boucher
  • , Timothy Brandt
  • Zack Briesemeister, Katherine de Kleer, Imke de Pater, William Deich, Devika Divakar, Étienne Gauvin, Thomas Greene, Amirul Hasan, Philip Hinz, Rebecca Jensen-Clem, Christopher Johnson, K. V. Govinda, Isabel Kain, Mackenzie Lach, Jean Thomas Landry, Michael C. Liu, James Lyke, Kenneth Magnone, Eduardo Marin, Raquel A. Martinez, Dimitri Mawet, Rosalie McGurk, Brittany Miles, Ajin Prakash, Dale Sandford, Ramya Sethuraman, Patrick Sheehan, Ji Man Sohn, Jordan Stone, Arun Surya, Hari Mohan Varshney, Eric Wang

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

SCALES (Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy) is the next-generation, diffraction-limited, thermal infrared, fully cryogenic, coronagraphic exoplanet spectrograph and imager for W.M.Keck Observatory.SCALES is fed by the Keck II Adaptive Optics bench.Both modes use common fore-optics to simplify the optical design and have individual detectors, which are JWST flight spares.The imager mode operates from 1 to 5 microns with selectable narrow- and broadband filters over a field of view 12.3 arcseconds on a side, and the integral field spectrograph mode operates from 2 to 5 microns with both low and mid spectral resolutions (R∼ 100 to R∼ 7500) over a field of view 2.15 arcseconds on a side.The diamond-turned aluminum optics, most of which are already delivered, with the rest being fabricated, provide low distortion, low wavefront error, and high throughput for all modes.The slicing unit, located behind the lenslet array, allows SCALES to reach heretofore unheard-of spatially-resolved spectral resolution for exoplanet and disc observations from the ground with a coronagraphic integral field spectrograph.The SCALES consortium includes UC Observatories, CalTech, W.M.Keck Observatory, the Indian Institute of Astrophysics, and the University of Durham, with over 40 science team members.We report on the overall design and project status during its ongoing fabrication phase, which started in early 2023.

Original languageEnglish (US)
Title of host publicationGround-Based and Airborne Instrumentation for Astronomy X
EditorsJulia J. Bryant, Kentaro Motohara, Joel R. Vernet
PublisherSPIE
ISBN (Electronic)9781510675155
DOIs
StatePublished - 2024
EventGround-Based and Airborne Instrumentation for Astronomy X 2024 - Yokohama, Japan
Duration: Jun 16 2024Jun 21 2024

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume13096
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceGround-Based and Airborne Instrumentation for Astronomy X 2024
Country/TerritoryJapan
CityYokohama
Period6/16/246/21/24

Keywords

  • adaptive optics
  • exoplanets
  • high-contrast
  • instrumentation
  • integral field spectroscopy
  • slenslit
  • thermal infrared

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Instrumentation
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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