A dataset provided by the European Space Agency

Name 10496
Title Decelerating and Dustfree: Efficient Dark Energy Studies with Supernovae and Clusters
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10496;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-hsgt29q
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=10496&mission=hst
Publication
  • A Calibration of NICMOS Camera 2 for Low Count Rates
  • A multiwavelength study of active galactic nuclei in clusters of galaxies
  • An Intensive Hubble Space Telescope Survey for z>1 Type Ia Supernovae by Targeting Galaxy Clusters
  • Assembly of the Red Sequence in Infrared-selected Galaxy Clusters from the IRAC Shallow Cluster Survey
  • A3COSMOS and A3GOODSS: Continuum source catalogues and multi-band number counts
  • A3COSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 <= z < 1.6
  • Charge transfer inefficiency in the Hubble Space Telescope since Servicing Mission 4
  • Cluster galaxies in XMMU J2235-2557: galaxy population properties in most massive environments at z ~ 1.4
  • Cluster X-ray luminosity-temperature relation at z 1.5
  • Colour gradients in cluster ellipticals at z ~ 1.4: the hidden content of the galaxy central regions
  • Deep Chandra observation of the galaxy cluster WARPJ1415.1+3612 at z =1 . An evolved cool-core cluster at high redshift
  • Determining Cosmological-model-independent H 0 with Gravitationally Lensed Supernova Refsdal
  • Discovery of an Unusual Optical Transient with the Hubble Space Telescope
  • Dusty Starbursts and the Formation of Elliptical Galaxies: A SCUBA-2 Survey of a z = 1.46 Cluster
  • Galaxy kinematics in the XMMU J2235-2557 cluster field at z 1.4
  • GALFIT-ing AGN Host Galaxies in COSMOS: HST versus Subaru
  • Gamma-ray bursts, quasars, baryonic acoustic oscillations, and supernovae Ia: new statistical insights and cosmological constraints
  • Growth of brightest cluster galaxies via mergers since z=1
  • High-resolution ALMA Study of CO J = 2-1 Line and Dust Continuum Emissions in Cluster Galaxies at z = 1.46
  • Hubble Space Telescope Discovery of a z = 3.9 Multiply Imaged Galaxy Behind the Complex Cluster Lens Warps J1415.1+36 at z = 1.026
  • Hubble Space Telescope Weak-lensing Study of the Galaxy Cluster XMMU J2235.3 - 2557 at z ~ 1.4: A Surprisingly Massive Galaxy Cluster When the Universe is One-third of its Current Age
  • Ha Star Formation Rates of z > 1 Galaxy Clusters in the IRAC Shallow Cluster Survey
  • Isophote Shapes of Early-type Galaxies in Massive Clusters at z ~ 1 and 0
  • Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5
  • Morphological evolution in situ: disc-dominated cluster red sequences at z ~ 1.25
  • Multiwavelength observations of a rich galaxy cluster at z ~ 1. The HST/ACS colour-magnitude diagram
  • Pan-STARRS1 Discovery of Two Ultraluminous Supernovae at z 0.9
  • Physical properties of brightest cluster galaxies up to redshift 1.80 based on HST data
  • Pixel-based correction for Charge Transfer Inefficiency in the Hubble Space Telescope Advanced Camera for Surveys
  • Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae
  • Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
  • Rest-Frame R-band Light Curve of a z ~ 1.3 Supernova Obtained with Keck Laser Adaptive Optics
  • Scaling Relations and Overabundance of Massive Clusters at z >~ 1 from Weak-lensing Studies with the Hubble Space Telescope
  • Sizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 at z = 1.39
  • Spectroscopy of Luminous Compact Blue Galaxies in Distant Clusters. II. Physical Properties of dE Progenitor Candidates
  • Star Formation in High-redshift Cluster Ellipticals
  • Stellar population and dust extinction in an ultraluminous infrared galaxy at z = 1.135
  • Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae
  • Submillimetre source counts in the fields of high-redshift galaxy clusters
  • The accelerated build-up of the red sequence in high-redshift galaxy clusters
  • The dependence of Type Ia Supernovae SALT2 light-curve parameters on host galaxy morphology
  • The Era of Star Formation in Galaxy Clusters
  • The evolution of cluster early-type galaxies over the past 8 Gyr
  • The Evolution of Radio Galaxies and X-Ray Point Sources in Coma Cluster Progenitors since z ~ 1.2
  • The Faint End of the Cluster-galaxy Luminosity Function at High Redshift
  • The Gemini/HST Galaxy Cluster Project: Redshift 0.2-1.0 Cluster Sample, X-Ray Data, and Optical Photometry Catalog
  • The Hubble Space Telescope Cluster Supernova Survey. III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 < Z < 1.46
  • The Hubble Space Telescope Cluster Supernova Survey. II. The Type Ia Supernova Rate in High-redshift Galaxy Clusters
  • The Hubble Space Telescope Cluster Supernova Survey. V. Improving the Dark-energy Constraints above z > 1 and Building an Early-type-hosted Supernova Sample
  • The Hubble Space Telescope Cluster Supernova Survey. VI. The Volumetric Type Ia Supernova Rate
  • The impact of satellite trails on Hubble Space Telescope observations
  • The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z = 1
  • The KMOS Cluster Survey (KCS). II. The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift 1.39 < z < 1.61
  • The KMOS Cluster Survey (KCS). I. The Fundamental Plane and the Formation Ages of Cluster Galaxies at Redshift 1.4 < z < 1.6
  • The morphological transformation of red sequence galaxies in clusters since z ~ 1
  • The morphological transformation of red sequence galaxies in the distant cluster XMMU J1229+0151
  • The Pantheon+ Analysis: Cosmological Constraints
  • The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration Systematic Uncertainty
  • The Pantheon+ Analysis: The Full Data Set and Light-curve Release
  • The XMM Cluster Survey: Active Galactic Nuclei and Starburst Galaxies in XMMXCS J2215.9-1738 at z = 1.46
  • The XMM Cluster Survey: Galaxy Morphologies and the Color-Magnitude Relation in XMMXCS J2215.9 - 1738 at z = 1.46
  • Zooming In on the Progenitors of Superluminous Supernovae With the HST
Instrument ACS, ACS/WFC, NICMOS, NICMOS/NIC2
Temporal Coverage 2005-07-02T15:58:35Z/2006-12-07T07:50:43Z
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 2007-12-08T01:38:49Z
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, 2007, 'Decelerating and Dustfree: Efficient Dark Energy Studies with Supernovae and Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-hsgt29q