A dataset provided by the European Space Agency

Name 5652
Title SINS: THE SUPERNOVA INTENSIVE STUDY TARGET OF OPPORTUNITY - CYCLE 4
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=5652;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-c48h64d
Author Kirshner, Robert P.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=5652&mission=hst
Publication
  • Bolometric and UV Light Curves of Core-collapse Supernovae
  • Clues to the Formation of Spiral Structure in M51 from the Ages and Locations of Star Clusters
  • Clusters in the inner spiral arms of M 51: The cluster IMF and the formation history
  • Constraints on the Binary Companion to the SN Ic 1994I Progenitor
  • Hierarchical star formation in M 51: star/cluster complexes
  • Late-Time HST Photometry of SN 1994I: Hints of Positron Annihilation Energy Deposition
  • New Constraints on Mass-dependent Disruption of Star Clusters in M51
  • Ongoing Massive Star Formation in the Bulge of M51
  • PS1-10afx at z = 1.388: Pan-STARRS1 Discovery of a New Type of Superluminous Supernova
  • Star cluster formation and disruption time-scales - I. An empirical determination of the disruption time of star clusters in four galaxies
  • The Age, Mass, and Size Distributions of Star Clusters in M51
  • The Environments of Supernovae in Archival Hubble Space Telescope Images
  • The Fraction of Stars That Form in Clusters in Different Galaxies
  • The Link between the Formation Rates of Clusters and Stars in Galaxies
  • The luminosity function of young star clusters: implications for the maximum mass and luminosity of clusters
  • The Star Cluster Mass-Galactocentric Radius Relation: Implications for Cluster Formation
  • The star cluster population of M 51. II. Age distribution and relations among the derived parameters
  • The star cluster population of M 51. III. Cluster disruption and formation history
  • The structure and environment of young stellar clusters in spiral galaxies
  • The young star cluster population of M51 with LEGUS - I. A comprehensive study of cluster formation and evolution
  • Young massive star clusters in M51
Instrument FOS/RD, WFPC2, WFPC2/PC
Temporal Coverage 1994-05-12T08:11:17Z/1994-05-14T07:14:54Z
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 1995-05-14T13:14:12Z
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, Kirshner comma Robert P., 1995, 'SINS: THE SUPERNOVA INTENSIVE STUDY TARGET OF OPPORTUNITY - CYCLE 4', 1.0, European Space Agency, https://doi.org/10.5270/esa-c48h64d