A dataset provided by the European Space Agency

Name 15309
Title Does the Relativistic X-Ray Outflow Quasar PDS 456 Have the Fastest-Ever UV BAL at ~0.3c?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15309;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-br5vexe
Author Hamann, Fred
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15309&mission=hst
Publication
  • Resolving the Soft X-Ray Ultrafast Outflow in PDS 456
Instrument COS, COS/FUV, COS/NUV
Temporal Coverage 2018-09-20T14:28:21Z/2019-09-04T18:07:25Z
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 2020-03-05T02:29:30Z
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, Hamann comma Fred, 2020, 'Does the Relativistic X-Ray Outflow Quasar PDS 456 Have the Fastest-Ever UV BAL at ~0.3c?', 1.0, European Space Agency, https://doi.org/10.5270/esa-br5vexe