Name | 14596 |
Title | Is Lyman Alpha Emitter CR7 Powered by a Direct Collapse Black Hole? |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=14596;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-feuaqni |
Author | European Space Agency |
Description | This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=14596&mission=hst |
Publication | On the nature and physical conditions of the luminous Ly α emitter CR7 and its rest-frame UV components, Sobral, David,Matthee, Jorryt,Brammer, Gabriel, Monthly Notices of the Royal Astronomical Society, 482, 2019-01-01 00:00:00, 2019MNRAS.482.2422S||The nature of CR7 revealed with MUSE: a young starburst powering extended Ly α emission at z = 6.6, Matthee, Jorryt,Pezzulli, Gabriele,Mackenzie, Ruari, Monthly Notices of the Royal Astronomical Society, 498, 2020-08-01 00:00:00, 2020MNRAS.498.3043M |
Instrument | WFC3/IR |
Temporal Coverage | 2017-03-14T08:53:18Z/2017-11-21T19:59:39Z |
Version | 1.0 |
Mission Description | Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited. |
Creator Contact | https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit |
Date Published | 2018-11-22T05:03:11Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2018, Is Lyman Alpha Emitter Cr7 Powered By A Direct Collapse Black Hole?, 1.0, European Space Agency, https://doi.org/10.5270/esa-feuaqni |