The Utrecht Photometric Systems (= UPS) and some results with it

Details The Utrecht Photometric Systems (= UPS) and some results with it The Utrecht Photometric Systems (= UPS) and some results with it

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ssrv...50..257h&link_type=abstract

(IAU, NSERC, Canadian Institute of Theoretical Astrophysics, et al., Colloquium on Algols, 107th, Sidney, Canada, Aug. 15-19, 19

Astronomy and Astrophysics

Astrophysics

4

Eclipsing Binary Stars, Light Curve, Line Spectra, Stellar Luminosity, Stellar Spectrophotometry, Gallium Arsenides, Near Infrared Radiation, Photometers, Photomultiplier Tubes, Signal To Noise Ratios

Scientific paper

The Utrecht Photometric System (UPS), a narrow-band photometric system with wavelength regions in which no telluric lines and almost no stellar/interstellar spectral lines are present, is discussed. The UPS design include photomultipliers with GaAs cathodes that have high sensitivity up to 900 nm. The system and its operation are described. Results are presented from using the UPS to study the components of eclipsing binaries obtained from light curves.

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