X-ray spectroscopy for Swift J1753.5-0127

Details X-ray spectroscopy for Swift J1753.5-0127 X-ray spectroscopy for Swift J1753.5-0127

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..552....1m&link_type=abstract

The Astronomer's Telegram, #552

Astronomy and Astrophysics

Astronomy

10

X-Ray, Transients

Scientific paper

The Swift XRT observed J1753.5-0127 starting on July 1st, 2005 at 21:28 UT. The observation revealed a variable source with a power-law spectrum. The spectrum is best fit by a power-law with absorption slightly greater than the total galactic column density in this direction of 1.7e21: nH = 2.0e21 ± 3.7e19 PhoIndex = 2.11 ± 1.1e-2 The source is observed to vary on timescales of 10s of seconds between fluxes of 2.9e-9 to 3.7e-9 erg/cm2/s with shorter timescale spikes (seconds) to 4.8e-9erg/cm2/s (all fluxes 0.5-10keV).

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