A dataset provided by the European Space Agency

Name 14638
Title What Makes Radio-detected and Optically-detected Supernova Remnants in NGC6946 Different?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14638;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-q3gzwc4
Author Long, Knox S.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14638&mission=hst
Publication
  • Optical Identification and Spectroscopy of Supernova Remnants in the Galaxy M51
  • Probing the final-stage progenitor evolution for Type IIP Supernova 2017eaw in NGC 6946
  • The dusty progenitor star of the Type II supernova 2017eaw
  • The Supernova Remnant Population of NGC 6946 as Observed in Fe II 1.644 mm with HST
  • The Type II-plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor
Instrument WFC3/IR
Temporal Coverage 2016-10-23T08:19:58Z/2016-10-27T07:35:17Z
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 2017-10-27T17:31:26Z
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, Long et al., 2017, 'What Makes Radio-detected and Optically-detected Supernova Remnants in NGC6946 Different?', 1.0, European Space Agency, https://doi.org/10.5270/esa-q3gzwc4