The accuracy of determining atmospheric extinction during spectrophotometric observations of stars

Details The accuracy of determining atmospheric extinction during spectrophotometric observations of stars The accuracy of determining atmospheric extinction during spectrophotometric observations of stars

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...68t&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Sept.-Oct. 1991, p. 68-74. In Russian.

Computer Science

Atmospheric Attenuation, Interstellar Extinction, Stellar Magnitude, Stellar Spectra, Stellar Spectrophotometry, Computerized Simulation, Root-Mean-Square Errors

Scientific paper

An analysis of the possible accuracy of determining the magnitude of atmospheric extinction during spectrophotometric observations of stars by the numerical modeling method is presented. A dependence of the final values of the rms errors of extraterrestrial magnitudes on the number of stars observed during the night and their relative positions is obtained. Tables illustrating the rms errors of the extraatmospheric magnitudes of stars for the case of linear and real extinction variation are presented.

Affiliated with

Also associated with

No associations

Rating

The accuracy of determining atmospheric extinction during spectrophotometric observations of stars 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 The accuracy of determining atmospheric extinction during spectrophotometric observations of stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The accuracy of determining atmospheric extinction during spectrophotometric observations of stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1876573