A dataset provided by the European Space Agency

Name 15335
Title What is the metallicity of the cool ISM in our own Galaxy?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15335;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-p35wrhe
Author De Cia, Annalisa
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15335&mission=hst
Publication
  • Dust depletion of metals from local to distant galaxies. I. Peculiar nucleosynthesis effects and grain growth in the ISM
  • Large metallicity variations in the Galactic interstellar medium
Instrument STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage 2018-06-21T14:37:27Z/2019-07-05T23:49:55Z
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 2020-01-06T01:23:16Z
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, De Cia comma Annalisa, 2020, 'What is the metallicity of the cool ISM in our own Galaxy?', 1.0, European Space Agency, https://doi.org/10.5270/esa-p35wrhe