A dataset provided by the European Space Agency

Name 14681
Title Tracing Galactic Outflows to the Source: Spatially Resolved Feedback in M83 with COS
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14681;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-79msyb9
Author Aloisi, Alessandra
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14681&mission=hst
Publication
  • Does Circumgalactic O VI Trace Low-pressure Gas Beyond the Accretion Shock? Clues from H I and Low-ion Absorption, Line Kinematics, and Dust Extinction
  • First Cospatial Comparison of Stellar, Neutral-gas, and Ionized-gas Metallicities in a Metal-rich Galaxy: M83
  • Simultaneous Estimates of Star-cluster Age, Metallicity, Mass, and Extinction (SESAMME). I. Presenting an MCMC Approach to Spectral Stellar Population Fitting
  • The First Metallicity Study of M83 Using the Integrated UV Light of Star Clusters
Instrument COS, COS/FUV, COS/NUV
Temporal Coverage 2017-05-12T17:39:29Z/2017-07-31T10:20:38Z
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 2018-07-31T12:16:41Z
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, Aloisi comma Alessandra, 2018, 'Tracing Galactic Outflows to the Source: Spatially Resolved Feedback in M83 with COS', 1.0, European Space Agency, https://doi.org/10.5270/esa-79msyb9