Compass and Scale Image of Cluster Galaxies

About the Data

• Data Description

  Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
  Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.

  Data for galaxies taken with the WFC3/UVIS instrument were obtained as part of the CLASH proposal: 12456, PI: M. Postman (STScI) et al. Data for galaxies taken with the ACS/SBC instrument were obtained from proposal: 12220, PI: R. Mittal (Max Planck Institute for Gravitational Physics) et al. The WFC3/UVIS BCG science team comprises: M. Donahue and T. Connor (Michigan State University), K. Fogarty (STScI), Y. Li (University of Michigan, Ann Arbor), M. Voit (Michigan State University), M. Postman and A. Koekemoer (STScI), J. Moustakas (Siena College, NY), L. Bradley (STScI), and H. Ford (JHU). The ACS/SBC BCG science team comprises: G. Tremblay (Yale University/ESO), C. O’Dea and S. Baum (University of Manitoba/RIT), R. Mittal (RIT/Max Planck Institute for Gravitational Physics), M. McDonald (Kavli Institute/MIT), F. Combes (Observatoire de Paris/CNRS), Y. Li (University of Michigan, Ann Arbor), B. McNamara (Waterloo University, Ontario/Harvard-Smithsonian Center for Astrophysics), M. Bremer (University of Bristol, UK), T. Clarke (Naval Research Laboratory), M. Donahue (Michigan State University), A. Edge (Durham University), A. Fabian (Institute of Astronomy), S. Hamer (Observatoire de Paris/CNRS), M. Hogan (Waterloo University, Ontario), J. Oonk (Netherlands Institute for Radio Astronomy), A. Quillen (University of Rochester), J. Sanders (Max Planck Institute for Extraterrestrial Physics), P. Salomé (Observatoire de Paris/CNRS), and M. Voit (Michigan State University).
• Instrument

  InstrumentThe science instrument used to produce the data.

  HST>WFC3/UVIS and HST>ACS/SBC