15 Distant Supernovae

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.

  The optical data from several HST proposals include: 9425 and 9583: PI: M. Giavalisco (STScI) and the GOODS Project 10189, 10339, and 10340: PI: A. Riess (STScI) and the PANS Project The science team includes: A. Riess (STScI/Johns Hopkins University), L.-G. Strolger (Western Kentucky University), S. Casertano, H. Ferguson, and B. Mobasher (STScI), B. Gold (Johns Hopkins University), P. Challis (Harvard-Smithsonian Center for Astrophysics), A. Filippenko, S. Jha, and W. Li (University of California, Berkeley), J. Tonry (Institute for Astronomy, University of Hawaii), R. Foley (University of California, Berkeley), R. Kirshner (Harvard-Smithsonian Center for Astrophysics), M. Dickinson and E. MacDonald (NOAO), D. Eisenstein (Steward Observatory/University of Arizona), M. Livio (STScI), J. Younger (Harvard-Smithsonian Center for Astrophysics), C. Xu and T. Dahlen (STScI), and D. Stern (Jet Propulsion Laboratory/Caltech).
• Instrument

  InstrumentThe science instrument used to produce the data.

  HST>ACS/WFC
• Exposure Dates

  Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.

  Various
• Filters

  FiltersThe camera filters that were used in the science observations.

  Various