Application of the Gabor transform to BATSE spectroscopy detector observations of Scorpius X-1

Details Application of the Gabor transform to BATSE spectroscopy detector observations of Scorpius X-1 Application of the Gabor transform to BATSE spectroscopy detector observations of Scorpius X-1

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..675m&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 675-678 (1997).

Mathematics

Neutron Stars, Mathematical Procedures And Computer Techniques, Spectroscopy And Spectrophotometry

Scientific paper

We present an application of the Gabor transform to Scorpius X-1 data obtained using the CGRO BATSE Spectroscopy Detectors (SDs). Two types of data are obtained with the BATSE SDs. The first set consists of the high S/N step fluxes obtained using the Earth-occultation method (see McNamara et al. these proceedings). The second (much larger) set is the 2.048 second time resolution raw flux data obtained between rise and set of Sco X-1. It is this latter set of data for which the Gabor transform is applicable. In this poster we present initial progress towards analysis of the substantial amount (107 points) of 2.048 second time resolution data.

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