| Name | 12613 |
| Title | Are major galaxy mergers a significant mechanism to trigger massive black hole growth at z=2? |
| URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=12613;TAPCLIENT=DOI |
| DOI | https://doi.org/10.5270/esa-r44h1u3 |
| 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=12613&mission=hst |
| Publication | Compact E+A Galaxies as a Progenitor of Massive Compact Quiescent Galaxies at 0.2 < z < 0.8, Zahid, H. Jabran,Baeza Hochmuth, Nicholas,Geller, Margaret J., The Astrophysical Journal, 831, 2016-11-01 00:00:00, 2016ApJ...831..146Z||Decomposing the host galaxy from high-z QSOs using principal component analysis, He, Wei,Wang, Yi-Ping, Research in Astronomy and Astrophysics, 19, 2019-10-01 00:00:00, 2019RAA....19..139H||Do the Most Massive Black Holes at z = 2 Grow via Major Mergers?, Mechtley, M.,Jahnke, K.,Windhorst, R. A., The Astrophysical Journal, 830, 2016-10-01 00:00:00, 2016ApJ...830..156M||The missing light of the Hubble Ultra Deep Field, Borlaff, Alejandro,Trujillo, Ignacio,Román, Javier, Astronomy and Astrophysics, 621, 2019-01-01 00:00:00, 2019A&A...621A.133B |
| Instrument | WFC3, WFC3/IR |
| Temporal Coverage | 2011-10-16T04:02:49Z/2012-09-13T22:49:42Z |
| 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 | 2012-09-14T02:13:27Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2012, Are Major Galaxy Mergers A Significant Mechanism To Trigger Massive Black Hole Growth At Z=2?, 1.0, European Space Agency, https://doi.org/10.5270/esa-r44h1u3 |