A dataset provided by the European Space Agency

Name 6555
Title What causes the astigmatism in gravitational lenses?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=6555;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-43nng46
Author Schechter, Paul
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=6555&mission=hst
Publication
  • Mass along the Line of Sight to the Gravitational Lens B1608+656: Galaxy Groups and Implications for H0
  • Steepened inner density profiles of group galaxies via interactions: an N-body analysis
  • The Fundamental Plane and the evolution of the M/L ratio of early-type field galaxies up to z~ 1
  • The Fundamental Plane of Gravitational Lens Galaxies and The Evolution of Early-Type Galaxies in Low-Density Environments
  • The Gravitational Lens B1608+656. I. V-, I-, and H-Band Hubble Space Telescope Imaging
  • The Hubble Constant from the Gravitational Lens B1608+656
  • The internal structure of the lens PG1115+080: breaking degeneracies in the value of the Hubble constant
  • The X-Ray Properties of Moderate-Redshift Galaxy Groups Selected by Association with Gravitational Lenses
Instrument WFPC2, WFPC2/PC
Temporal Coverage 1997-05-17T09:06:14Z/1999-07-18T09:03:13Z
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 2000-07-18T16:05:02Z
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, Schechter comma Paul, 2000, 'What causes the astigmatism in gravitational lenses?', 1.0, European Space Agency, https://doi.org/10.5270/esa-43nng46