Wavelet analysis of fast photometry on Cygnus X-1 with the AstraLux camera

Details Wavelet analysis of fast photometry on Cygnus X-1 with the AstraLux camera Wavelet analysis of fast photometry on Cygnus X-1 with the AstraLux camera

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1053..387l&link_type=abstract

OBSERVATIONAL EVIDENCE FOR BLACK HOLES IN THE UNIVERSE: Proceedings of the 2nd Kolkata Conference on Observational Evidence for

Computer Science

Radio Galaxies, Binary And Multiple Stars, X- And Gamma-Ray Instruments

Scientific paper

We present sub-second fast photometry for the high mass X-ray binary Cygnus X-1. We try to observe variability due to instabilities in the accretion process at optical wavelengths. The observations were carried out using the high speed AstraLux camera at the Calar Alto 2.2 m telescope, Spain, in November 2006 and August 2007. We report that the Cygnus X-1 system light curve sampled every 30 milli-second did not display strong enough evidence of any periodic component related to the source.

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