Name | 13456 |
Title | Searching for 300, 000 Degree Gas in the Core of the Phoenix Cluster with HST-COS |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=13456;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-nlnh9pa |
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=13456&mission=hst |
Publication | Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales, McDonald, Michael,McNamara, Brian R.,van Weeren, Reinout J., The Astrophysical Journal, 811, 2015-10-01 00:00:00, 2015ApJ...811..111M||Searching for FUV line emission from 107 K gas in massive elliptical galaxies and galaxy clusters as a tracer of turbulent velocities, Anderson, Michael E.,Sunyaev, Rashid, Monthly Notices of the Royal Astronomical Society, 459, 2016-07-01 00:00:00, 2016MNRAS.459.2806A||The challenging task of determining star formation rates: the case of a massive stellar burst in the brightest cluster galaxy of Phoenix galaxy cluster, Mittal, Rupal,McDonald, M.,Whelan, John T., Monthly Notices of the Royal Astronomical Society, 465, 2017-03-01 00:00:00, 2017MNRAS.465.3143M |
Instrument | COS/FUV, COS/NUV |
Temporal Coverage | 2014-01-17T13:33:48Z/2014-07-11T03:33:52Z |
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 | 2015-07-11T11:38:19Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2015, Searching For 300, 000 Degree Gas In The Core Of The Phoenix Cluster With Hst-Cos, 1.0, European Space Agency, https://doi.org/10.5270/esa-nlnh9pa |