A dataset provided by the European Space Agency

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 McDonald, Michael A.
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
  • Searching for FUV line emission from 107 K gas in massive elliptical galaxies and galaxy clusters as a tracer of turbulent velocities
  • The challenging task of determining star formation rates: the case of a massive stellar burst in the brightest cluster galaxy of Phoenix galaxy cluster
Instrument COS, 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
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, McDonald comma Michael A., 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