Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998stin...0088604w&link_type=abstract
Technical Report, AD-A366959; VRISV-98-01-VOL-1; AFRL-VS-HA-TR-98-0104
Astronomy and Astrophysics
Astronomy
Satellite Observation, Space Surveillance, Satellite Networks, Mathematical Models, Infrared Spectra, Astronomy, Natural Satellites, Infrared Radiation, Spectral Bands, Stellar Spectra, Spectral Emission
Scientific paper
The purpose of this program was to extend and improve the present capability to predict celestial phenomenology pertinent to the design and successful operation of space based surveillance systems using the ultraviolet, optical, and infrared spectral regions. We pursued this goal through analysis and application of existing datasets and, in particular, by analysis of new satellite measurements that became available during the course of the project. Our work was concentrated in four major areas: (1) extension of an existing analytical model of the infrared point source sky (SKY), (2) development of a set of absolutely calibrated spectral stellar irradiance standards for the infrared, (3) analysis of new celestial data obtained by satellite, and (4) support of the infrared celestial measurements taken by the Midcourse Space Experiment (MSX) satellite. Volume 1 summarizes the work performed under the contract, and includes reprints of the major papers published during the contractual period. Volume 2 presents the final release of an all sky network of 422 stars with absolutely calibrated stellar spectra in the 1.2 to 35 um region. Volume 2 also contains reprints of the complete series of published papers documenting the spectral calibration process and assumptions.
Cohen Martin
Walker Russell G.
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