Optical/X-ray Variability in Swift 1753.5-0127

Details Optical/X-ray Variability in Swift 1753.5-0127 Optical/X-ray Variability in Swift 1753.5-0127

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..562....1h&link_type=abstract

The Astronomer's Telegram, #562

Astronomy and Astrophysics

Astronomy

2

Optical, X-Ray, Binaries, Black Holes, Transients

Scientific paper

Further rapid optical photometry of Swift J1753.5-0127 (Palmer et al., ATEL #546) was obtained at McDonald Observatory on July 6th and 7th, simultaneously with RXTE public observations. Observational details were exactly as for the previous observation (Hynes & Mullally ATEL #554). Closer examination of the optical power spectrum reveals that the apparent red-noise is actually composed of two components.

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