X- and gamma-ray superfast photometry

Details X- and gamma-ray superfast photometry X- and gamma-ray superfast photometry

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...105....1b&link_type=abstract

Astronomy and Astrophysics, vol. 105, no. 1, Jan. 1982, p.1-5.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Gamma Ray Astronomy, X Ray Sources, Binary Stars, Distribution Functions, Neutron Stars, Random Signals, Signal To Noise Ratios

Scientific paper

Superfast photometry comprises the study of time-varying phenomena whose characteristic time scale is less than the mean time between two photons. Astronomical objects whose light curve can be varied in a random manner are considered, and the possibility of knowing the distribution function parameters in the case of a characteristic time smaller than the average time interval between two photons is demonstrated. The sensitivity of the method is computed, and its usefulness is investigated through consideration of X-ray and gamma-ray satellites in current use and those planned for the next development generation.

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