A dataset provided by the European Space Agency

Name 10200
Title Dark Matter Constraints from the Merging Cluster 1E0657-56
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10200;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-ft6exjz
Author Jones, Christine
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=10200&mission=hst
Publication
  • A bright, dust-obscured, millimetre-selected galaxy beyond the Bullet Cluster (1E0657-56)
  • A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
  • A Direct Empirical Proof of the Existence of Dark Matter
  • A Multiply Imaged Luminous Infrared Galaxy Behind the Bullet Cluster (1E0657-56)
  • Constraints on the Self-Interaction Cross Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-56
  • Deep luminosity functions and colour-magnitude relations for cluster galaxies at 0.2 < z < 0.6
  • Evolution of the observed Lya luminosity function from z = 6.5 to z = 7.7: evidence for the epoch of reionization?
  • Little change in the sizes of the most massive galaxies since z = 1
  • Looking for dark matter trails in colliding galaxy clusters
  • Lyman Break Galaxies under a Microscope: The Small-Scale Dynamics and Mass of an Arc in the Cluster 1E 0657-56
  • Measuring the Stellar Masses of z ~ 7 Galaxies with the Spitzer UltRaFaint SUrvey Program (SURFS UP)
  • Reconstruction of Cluster Masses Using Particle Based Lensing. I. Application to Weak Lensing
  • Spectroscopic Confirmation of a z = 2.79 Multiply Imaged Luminous Infrared Galaxy Behind the Bullet Cluster
  • Spectroscopic Confirmation of a z = 6.740 Galaxy behind the Bullet Cluster
  • Spitzer Ultra Faint SUrvey Program (SURFS UP). I. An Overview
  • Strong and Weak Lensing United. III. Measuring the Mass Distribution of the Merging Galaxy Cluster 1ES 0657-558
  • The Atacama Cosmology Telescope: Physical Properties and Purity of a Galaxy Cluster Sample Selected via the Sunyaev-Zeldovich Effect
  • The Bullet Cluster 1E0657-558 evidence shows modified gravity in the absence of dark matter
  • The Bullet cluster at its best: weighing stars, gas, and dark matter
  • The Herschel Lensing Survey (HLS): Overview
  • The impact of satellite trails on Hubble Space Telescope observations
  • The nongravitational interactions of dark matter in colliding galaxy clusters
  • Using the Bullet Cluster as a Gravitational Telescope to Study z~7 Lyman Break Galaxies with WFC3 Imaging
  • Using the Bullet Cluster as a Gravitational Telescope to Study z >~ 7 Lyman Break Galaxies
  • z ~ 7-10 Galaxies Behind Lensing Clusters: Contrast with Field Search Results
Instrument ACS, ACS/WFC
Temporal Coverage 2004-10-21T14:10:42Z/2004-10-21T21:19:07Z
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 2005-10-22T02:37:11Z
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, Jones comma Christine, 2005, 'Dark Matter Constraints from the Merging Cluster 1E0657-56', 1.0, European Space Agency, https://doi.org/10.5270/esa-ft6exjz