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• W1639254913 endingPage "106" @default.
• W1639254913 startingPage "106" @default.
• W1639254913 abstract "The black hole candidate (BHC) Swift J1753.5–0127 went into outburst in 2005 June. Rather than fade into quiescence as most BHC transients do, it has remained in a low hard spectral state for most of the ∼9 years after its outburst. Its persistent emission during the hard state is reminiscent of the black hole Cyg X-1 and the BHCs 1E 1740.7–2942 and GRS 1758–258. Thus far, hard X-ray/soft gamma-ray results have mainly focused on the 2005 flare, with a few additional observations during 2007. Here, we present results from INTEGRAL/SPI observations from 2005–2010 spanning the 22–650 keV energy range. Spectral analysis shows a weak high-energy excess () above a cutoff power-law model that is well fit by a power law, suggesting an additional spectral component. Observations of Cyg X-1, 1E 1740.7–2942, and GRS 1758–258 have shown similar spectra requiring an additional high-energy component. The SPI results are compared to previously reported results for Swift J1753.5–0127 as well as observations of other sources." @default.
• W1639254913 created "2016-06-24" @default.
• W1639254913 creator A5013963442 @default.
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• W1639254913 date "2015-07-06" @default.
• W1639254913 modified "2023-09-30" @default.
• W1639254913 title "LONG-TERM MONITORING OF THE BLACK HOLE CANDIDATE SWIFT J1753.5–0127 WITH<i>INTEGRAL</i>/SPI" @default.
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• W1639254913 doi "https://doi.org/10.1088/0004-637x/807/1/106" @default.
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