A dataset provided by the European Space Agency

Name 13350
Title How Low Can They Go? Detecting low luminosity supernova progenitors
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=13350;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-hs7oi0v
Author Fruchter, Andrew S.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=13350&mission=hst
Publication
  • Luminosity Models and Density Profiles for Nuclear Star Clusters for a Nearby Volume-limited Sample of 29 Galaxies
  • The very young resolved stellar populations around stripped-envelope supernovae
Instrument WFC3, WFC3/UVIS
Temporal Coverage 2013-11-12T18:37:27Z/2014-04-09T17:12:35Z
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 2015-04-09T21:26:11Z
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, Fruchter et al., 2015, 'How Low Can They Go? Detecting low luminosity supernova progenitors', 1.0, European Space Agency, https://doi.org/10.5270/esa-hs7oi0v