Name | 5709 |
Title | STAR FORMATION RATES IN DISTANT CLUSTER GALAXIES: CYCLE 4 CARRY-OVER |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=5709;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-qba3ld2 |
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=5709&mission=hst |
Publication | A hyperluminous galaxy at z=2.8 found in a deep submillimetre survey, Ivison, R. J.,Smail, Ian,Le Borgne, J.-F., Monthly Notices of the Royal Astronomical Society, 298, 1998-08-01 00:00:00, 1998MNRAS.298..583I||Faint Submillimeter Galaxies: Hubble Space Telescope Morphologies and Colors, Smail, Ian,Ivison, R. J.,Blain, A. W., The Astrophysical Journal, 507, 1998-11-01 00:00:00, 1998ApJ...507L..21S||Lensed galaxies in Abell 370. II. The ultraviolet properties of arclets and the star formation rate at high redshift, Bézecourt, J.,Soucail, G.,Ellis, R. S., Astronomy and Astrophysics, 351, 1999-11-01 00:00:00, 1999A&A...351..433B||Mapping the Evolution of High-Redshift Dusty Galaxies with Submillimeter Observations of a Radio-selected Sample, Barger, A. J.,Cowie, L. L.,Richards, E. A., The Astronomical Journal, 119, 2000-05-01 00:00:00, 2000AJ....119.2092B |
Instrument | WFPC2, WFPC2/WFC |
Temporal Coverage | 1995-06-29T10:01:17Z/1995-06-30T04:11:57Z |
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 | 1996-06-30T13:21:35Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 1996, Star Formation Rates In Distant Cluster Galaxies: Cycle 4 Carry-Over, 1.0, European Space Agency, https://doi.org/10.5270/esa-qba3ld2 |