A dataset provided by the European Space Agency

Name 12298
Title Towards a Physical Understanding of the Diversity of Type Ia Supernovae
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12298;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-6vkrvis
Author Ellis, Richard S.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12298&mission=hst
Publication
  • A compact circumstellar shell as the source of high-velocity features in SN 2011fe
  • A Physical Model for SN 2001ay, a Normal, Bright, Extremely Slow Declining Type Ia Supernova
  • Artificial Intelligence-Assisted Inversion (AIAI) of Synthetic Type Ia Supernova Spectra
  • A Speed Bump: SN 2021aefx Shows that Doppler Shift Alone Can Explain Early Excess Blue Flux in Some Type Ia Supernovae
  • Decontaminating Swift UVOT Grism Observations of Transient Sources
  • Hubble Space Telescope spectra of the Type Ia supernova SN 2011fe: a tail of low-density, high-velocity material with Z < Z
  • Hubble Space Telescope studies of low-redshift Type Ia supernovae: evolution with redshift and ultraviolet spectral trends
  • Investigating the diversity of Type Ia supernova spectra with the open-source relational data base KAEPORA
  • Metallicity Differences in Type Ia Supernova Progenitors Inferred from Ultraviolet Spectra
  • Neutral-gas-phase metal abundances in Zn II-selected quasar absorption line systems near redshift z = 1.2
  • On spectral line profiles in Type Ia supernova spectra
  • Significant luminosity differences of two twin Type Ia supernovae
  • SOUSA: the Swift Optical/Ultraviolet Supernova Archive
  • Spectral models for early time SN 2011fe observations
  • Spectrophotometric time series of SN 2011fe from the Nearby Supernova Factory
  • Swift Ultraviolet Observations of Supernova 2014J in M82: Large Extinction from Interstellar Dust
  • Swift UVOT grism observations of nearby Type Ia supernovae - I. Observations and data reduction
  • The impact of satellite trails on Hubble Space Telescope observations
  • Theoretical Clues to the Ultraviolet Diversity of Type Ia Supernovae
  • The UV/optical spectra of the Type Ia supernova SN 2010jn: a bright supernova with outer layers rich in iron-group elements
  • Twins for life? A comparative analysis of the Type Ia supernovae 2011fe and 2011by
  • Ultraviolet diversity of Type Ia Supernovae
  • Ultraviolet Line Identifications and Spectral Formation Near Max Light in Type Ia Supernova 2011fe
  • Ultraviolet Observations of Super-Chandrasekhar Mass Type Ia Supernova Candidates with Swift UVOT
Instrument STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage 2010-10-15T23:23:54Z/2011-10-21T05:27:26Z
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 2012-10-21T09:53:51Z
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, Ellis comma Richard S., 2012, 'Towards a Physical Understanding of the Diversity of Type Ia Supernovae', 1.0, European Space Agency, https://doi.org/10.5270/esa-6vkrvis