Fourier transform spectroscopy with a deformable mirror

Details Fourier transform spectroscopy with a deformable mirror Fourier transform spectroscopy with a deformable mirror

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004spie.5487.1418k&link_type=abstract

Optical, Infrared, and Millimeter Space Telescopes. Edited by Mather, John C. Proceedings of the SPIE, Volume 5487, pp. 1418-

Mathematics

Scientific paper

During the in-orbit checkout phase of the Infrared Spectrograph1 on board The Spitzer Telescope,2 it was found that the noise of the spectrograph's arrays was correlated with the number of cosmic ray hits. Our analysis reveals that the cause of that effect is most likely due to the algorithms used to correct cosmic ray hits on dark pixels. We also found that the noise characteristics of the pixels that have an illumination that is lower than 1/10 of the full well is artificially raised by the cosmic ray correction by a factor of about 10% if 1% of the pixels are affected by cosmic rays.

Affiliated with

Also associated with

No associations

Rating

Fourier transform spectroscopy with a deformable mirror 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 Fourier transform spectroscopy with a deformable mirror, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fourier transform spectroscopy with a deformable mirror will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1807811