A dataset provided by the European Space Agency

Name 14327
Title See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14327;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-wx05t0f
Author Perlmutter, Saul
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14327&mission=hst
Publication
  • A Binary Offset Effect in CCD Readout and Its Impact on Astronomical Data
  • A Large-scale Kinematic Study of Molecular Gas in High-z Cluster Galaxies: Evidence for High Levels of Kinematic Asymmetry
  • ALMA Observations of Gas-rich Galaxies in z ~ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments
  • Evidence for the Existence of Abundant Intracluster Light at z = 1.24
  • First Weak-lensing Results from See Change: Quantifying Dark Matter in the Two z 1.5 High-redshift Galaxy Clusters SPT-CL J2040-4451 and IDCS J1426+3508
  • Galaxy Merger Candidates in High-redshift Cluster Environments
  • Galaxy populations in the most distant SPT-SZ clusters. I. Environmental quenching in massive clusters at 1.4 z 1.7
  • Galaxy populations in the most distant SPT-SZ clusters. II. Galaxy structural properties in massive clusters at 1.4 z 1.7
  • Low surface brightness galaxies in z > 1 galaxy clusters: HST approaching the progenitors of local ultra diffuse galaxies
  • Resolving CO (2-1) in z ~ 1.6 Gas-rich Cluster Galaxies with ALMA: Rotating Molecular Gas Disks with Possible Signatures of Gas Stripping
  • See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies
  • The delay time distribution of Type-Ia supernovae in galaxy clusters: the impact of extended star-formation histories
  • The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22
  • The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries
  • The H a star formation main sequence in cluster and field galaxies at z ~ 1.6
  • The impact of satellite trails on Hubble Space Telescope observations
  • The missing light of the Hubble Ultra Deep Field
  • The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75
Instrument WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage 2015-10-16T16:18:47Z/2017-03-30T09:01:43Z
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 2017-03-30T20:22:02Z
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, Perlmutter comma Saul, 2017, 'See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts', 1.0, European Space Agency, https://doi.org/10.5270/esa-wx05t0f