The Astronomical Journal (Jan 2024)

FORECASTOR. I. Finding Optics Requirements and Exposure Times for the Cosmological Advanced Survey Telescope for Optical and UV Research Mission

  • Isaac Cheng,
  • Tyrone E. Woods,
  • Patrick Côté,
  • Jennifer Glover,
  • Dhananjhay Bansal,
  • Melissa Amenouche,
  • Madeline A. Marshall,
  • Laurie Amen,
  • John Hutchings,
  • Laura Ferrarese,
  • Kim A. Venn,
  • Michael Balogh,
  • Simon Blouin,
  • Ryan Cloutier,
  • Nolan Dickson,
  • Sarah Gallagher,
  • Martin Hellmich,
  • Vincent Hénault-Brunet,
  • Viraja Khatu,
  • Cameron Lawlor-Forsyth,
  • Cameron Morgan,
  • Harvey Richer,
  • Marcin Sawicki,
  • Robert Sorba

DOI
https://doi.org/10.3847/1538-3881/ad2987
Journal volume & issue
Vol. 167, no. 4
p. 178

Abstract

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The Cosmological Advanced Survey Telescope for Optical and ultraviolet Research (CASTOR) is a proposed Canadian-led 1 m class space telescope that will carry out ultraviolet and blue optical wide-field imaging, spectroscopy, and photometry. CASTOR will provide an essential bridge in the post-Hubble era, preventing a protracted UV-optical gap in space astronomy and enabling an enormous range of discovery opportunities from the solar system to the nature of the cosmos, in conjunction with the other great wide-field observatories of the next decade (e.g., Euclid, Roman, Vera Rubin). FORECASTOR (Finding Optics Requirements and Exposure times for CASTOR) will supply a coordinated suite of mission-planning tools that will serve as the one-stop shop for proposal preparation, data reduction, and analysis for the CASTOR mission. We present the first of these tools: a pixel-based, user-friendly, extensible, multi-mission exposure time calculator built in Python, including a modern browser-based graphical user interface that updates in real time. We then provide several illustrative examples of FORECASTOR’s use that advance the design of planned legacy surveys for the CASTOR mission: a search for the most massive white dwarfs in the Magellanic Clouds, a study of the frequency of flaring activity in M stars and their distribution and impacts on habitability of exoplanets, mapping the proper motions of faint stars in the Milky Way, wide and deep galaxy surveys, and time-domain studies of active galactic nuclei.

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