Supernovae and Transients with EUCLID and the European ELT

The prospects are described for studies of large samples of supernovæ and other variable objects with two proposed future facilities: (1) the European Extremely Large Telescope, a general-purpose 40-m-class ground-based optical-IR telescope, and (2) Euclid, an M-class mission within ESA's Cosmi...

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Main Author: Hook, I
Format: Conference item
Published: 2012
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author Hook, I
author_facet Hook, I
author_sort Hook, I
collection OXFORD
description The prospects are described for studies of large samples of supernovæ and other variable objects with two proposed future facilities: (1) the European Extremely Large Telescope, a general-purpose 40-m-class ground-based optical-IR telescope, and (2) Euclid, an M-class mission within ESA's Cosmic Vision programme, primarily for cosmology. The capabilities and status of the two facilities are briefly described. Their suitability for the study of time-varying objects in general, and of supernovæ in particular, is discussed. It is shown that Euclid has the potential for NIR imaging of a few thousand Type Ia supernovæ to intermediate z, while the E-ELT will be capable of spectroscopic and classification measurements of Type Ia supernovæ to z=4. © 2012 International Astronomical Union.
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spelling oxford-uuid:b4823d55-a2e3-4516-8cab-b82e7f29cfed2022-03-27T04:26:35ZSupernovae and Transients with EUCLID and the European ELTConference itemhttp://purl.org/coar/resource_type/c_5794uuid:b4823d55-a2e3-4516-8cab-b82e7f29cfedSymplectic Elements at Oxford2012Hook, IThe prospects are described for studies of large samples of supernovæ and other variable objects with two proposed future facilities: (1) the European Extremely Large Telescope, a general-purpose 40-m-class ground-based optical-IR telescope, and (2) Euclid, an M-class mission within ESA's Cosmic Vision programme, primarily for cosmology. The capabilities and status of the two facilities are briefly described. Their suitability for the study of time-varying objects in general, and of supernovæ in particular, is discussed. It is shown that Euclid has the potential for NIR imaging of a few thousand Type Ia supernovæ to intermediate z, while the E-ELT will be capable of spectroscopic and classification measurements of Type Ia supernovæ to z=4. © 2012 International Astronomical Union.
spellingShingle Hook, I
Supernovae and Transients with EUCLID and the European ELT
title Supernovae and Transients with EUCLID and the European ELT
title_full Supernovae and Transients with EUCLID and the European ELT
title_fullStr Supernovae and Transients with EUCLID and the European ELT
title_full_unstemmed Supernovae and Transients with EUCLID and the European ELT
title_short Supernovae and Transients with EUCLID and the European ELT
title_sort supernovae and transients with euclid and the european elt
work_keys_str_mv AT hooki supernovaeandtransientswitheuclidandtheeuropeanelt