Deconvolving infrared telescope images as point sources on a grid

Details Deconvolving infrared telescope images as point sources on a grid Deconvolving infrared telescope images as point sources on a grid

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4850..813e&link_type=abstract

IR Space Telescopes and Instruments. Edited by John C. Mather . Proceedings of the SPIE, Volume 4850, pp. 813-823 (2003).

Mathematics

Scientific paper

Deconvolution of infrared telescope images can partially recover the distribution of light in the sky. The light from point sources and extended sources is modeled as a grid of closely-spaced points. A matrix of influence coefficients contains the response of the telescope-instrument combination to light at the grid points. A non-negative least-squares routine finds the sky flux densities that reproduce the instrument data. A personal computer program and examples of infrared telescope data deconvolution are presented.

Affiliated with

Also associated with

No associations

Rating

Deconvolving infrared telescope images as point sources on a grid does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Deconvolving infrared telescope images as point sources on a grid, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Deconvolving infrared telescope images as point sources on a grid will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1170310