Spectrophotometry of cool stars from objective prism spectra

Details Spectrophotometry of cool stars from objective prism spectra Spectrophotometry of cool stars from objective prism spectra

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984asph.conf..285l&link_type=abstract

In Royal Observatory Astron. Phot. 1984 p 285-293 (SEE N85-16102 07-35)

Astronomy and Astrophysics

Astronomy

Cool Stars, Late Stars, Photographic Plates, Prisms, Stellar Spectra, Stellar Spectrophotometry, Astronomical Photography, Calibrating, Data Reduction, Sensitometry

Scientific paper

A technique for obtaining low dispersion spectrophotometry of cool stars from objective prism plates is presented. Photographic stellar spectra are calibrated by a spot sensitometer and combined with published photoelectric scans. The resulting spectrophotometry covers an extended spectral region with a wavelength spacing increasing from 1.5 A in the blue to 27 A in the near infrared.

Affiliated with

Also associated with

No associations

Rating

Spectrophotometry of cool stars from objective prism spectra 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 Spectrophotometry of cool stars from objective prism spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrophotometry of cool stars from objective prism spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1499056