NSSDCA ID: 2001-027A-01
Mission Name: WMAPThe WMAP instrument consists of pseudo-correlation differential radiometers fed by two back-to-back 1.5 m primary Gregorian reflectors. This instrument uses five frequency bands from 22 GHz to 90 GHz to facilitate rejection of foreground signals from our own Galaxy. The WMAP instrument has a 3.5 degree x 3.5 degree field of view.
Questions and comments about this experiment can be directed to: Dr. David T. Leisawitz
Name | Role | Original Affiliation | |
---|---|---|---|
Dr. John C. Mather | Co-Investigator | NASA Goddard Space Flight Center | john.c.mather@nasa.gov |
Dr. David T. Wilkinson | Co-Investigator | Princeton University | |
Dr. Edward L. Wright | Co-Investigator | University of California, Los Angeles | wright@astro.ucla.edu |
Mr. Gary F. Hinshaw | Co-Investigator | NASA Goddard Space Flight Center | hinshaw@map.gsfc.nasa.gov |
Dr. Lyman A. Page | Co-Investigator | Princeton University | page@princeton.edu |
Dr. Norman Jarosik | Co-Investigator | Princeton University | jarosik@pupgg.princeton.edu |
Dr. David N. Spergel | Co-Investigator | Princeton University | dns@astro.princeton.edu |
Dr. Stephan S. Meyer | Co-Investigator | University of Chicago | meyer@oddjob.uchicago.edu |
Dr. Charles L. Bennett | Principal Investigator | NASA Goddard Space Flight Center | bennett@map.gsfc.nasa.gov |
The WMAP Archive at LAMBDA