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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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. |
first_indexed | 2024-03-07T03:11:57Z |
format | Conference item |
id | oxford-uuid:b4823d55-a2e3-4516-8cab-b82e7f29cfed |
institution | University of Oxford |
last_indexed | 2024-03-07T03:11:57Z |
publishDate | 2012 |
record_format | dspace |
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 |