Atmospheric extinction monitoring using multi-color starlight

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Optical Constants, Astronomical And Space-Research Instrumentation, Galactic Nuclei, Circumnuclear Matter, And Bulges

Scientific paper

We are using an optical telescope to measure the visual colors from standard stars with well known photometric properties to characterize atmospheric extinction as a function of wavelength and airmass (or zenith angle) at a certain point in time. To improve the flux and energy calibration of Cherenkov air showers recorded by IACT under varying atmospheric conditions, we investigate the correlations between the parameters characterizing the atmospheric transparency as determined by the optical telescope and the shower trigger rate measured with an IACT. This requires that the monitoring telescope is located close to the IACT to see the same part of the atmosphere.
First results from the Automatic Telescope for Optical Monitoring (ATOM), positioned four hundred meters away from the H.E.S.S. IACT telescopes, are presented here.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Atmospheric extinction monitoring using multi-color starlight 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 Atmospheric extinction monitoring using multi-color starlight, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atmospheric extinction monitoring using multi-color starlight will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1100561

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.