5 September 2017 The NASA probe-class mission concept, CETUS (Cosmic Evolution Through Ultraviolet Spectroscopy)
Author Affiliations +
Abstract
We report on the early phases of a NASA-sponsored study of CETUS (Cosmic Evolution Through Ultraviolet Spectroscopy), a Probe-class mission concept. By definition, the full lifecycle cost of a Probe mission is greater than $400M (i.e. Explorer missions) and less than $1.00B (“Flagship” missions). The animating idea behind our study is that CETUS can help answer fundamental questions about galaxy evolution by carrying out a massive UV imaging and spectroscopic survey of galaxies and combining its findings with data obtained by other survey telescopes of the 2020’s. The CETUS mission concept comprises a 1.5-m wide-field telescope and three scientific instruments: a near-UV multi-object slit spectrograph with a micro-shutter array as the slit device; a near-UV and far-UV camera with angular resolution of 0.42” (near-UV) or 0.55” (far-UV); and a near-UV or far-UV single-object spectrograph aimed at providing access to the UV after Hubble is gone. We describe the scientific rationale for CETUS and the telescope and instruments in their early design phase.
Conference Presentation
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Sara Heap, William Danchi, James Burge, Kelly Dodson, Anthony Hull, Steven Kendrick, Stephan McCandliss, Gregory Mehle, Lloyd Purves, David Sheikh, Martin Valente, Robert A. Woodruff, "The NASA probe-class mission concept, CETUS (Cosmic Evolution Through Ultraviolet Spectroscopy)", Proc. SPIE 10398, UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts VIII, 103980U (5 September 2017); doi: 10.1117/12.2274202; https://doi.org/10.1117/12.2274202
PROCEEDINGS
11 PAGES + PRESENTATION

SHARE
RELATED CONTENT

WSO-UV ground segment for observation optimisation
Proceedings of SPIE (July 18 2016)
2dF grows up: Echidna for the AAT
Proceedings of SPIE (July 11 2008)
COHSI: the Cambridge OH Suppression Instrument
Proceedings of SPIE (March 21 1997)
Integrating BigBOSS with the Mayall Telescope
Proceedings of SPIE (September 24 2012)
TAUVEX: UV space telescope
Proceedings of SPIE (January 22 1993)

Back to Top