A dataset provided by the European Space Agency

Name 14077
Title The frequency and chemical composition of rocky planetary debris around young white dwarfs: Plugging the last gaps
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14077;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-hyf8i7q
Author Gaensicke, Boris T.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14077&mission=hst
Publication
  • An HST COS ultraviolet spectroscopic survey of 311 DA white dwarfs - I. Fundamental parameters and comparative studies
  • The unbiased frequency of planetary signatures around single and binary white dwarfs using Spitzer and Hubble
Instrument COS, COS/FUV
Temporal Coverage 2015-10-16T06:39:49Z/2017-09-28T05:15:41Z
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 2018-09-28T07:55:58Z
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, Gaensicke comma Boris T., 2018, 'The frequency and chemical composition of rocky planetary debris around young white dwarfs: Plugging the last gaps', 1.0, European Space Agency, https://doi.org/10.5270/esa-hyf8i7q