Relations between X-ray timing features and spectral parameters of Galactic black hole X-ray binaries
H. Stiele (1), T. M. Belloni (1), E. Kalemci (2), S. Motta (3) ((1), INAF-OAB, (2) Sabanc{\i} \"Universitesi, (3) ESAC/ESA)

TL;DR
This study explores the relationship between spectral and timing features in black hole X-ray binaries, confirming known correlations and revealing new insights into their behavior during outbursts using RXTE data.
Contribution
It provides a detailed analysis of spectral-timing correlations across multiple sources and outbursts, utilizing the empirical simpl model and high-energy data from HEXTE.
Findings
Confirmed positive correlation between photon index and QPO frequency.
Discovered anticorrelation between up-scattered photon fraction and QPO frequency.
Observed consistent correlation patterns during outburst decay across different events.
Abstract
We present a study of correlations between spectral and timing parameters for a sample of black hole X-ray binary candidates. Data are taken from GX 339-4, H 1743-322, and XTE J1650-500, as the Rossi X-ray Timing Explorer (RXTE) observed complete outbursts of these sources. In our study we investigate outbursts that happened before the end of 2009 to make use of the high-energy coverage of the HEXTE detector and select observations that show a certain type of quasi-periodic oscillations (type-C QPOs). The spectral parameters are derived using the empirical convolution model simpl to model the Comptonized component of the emission together with a disc blackbody for the emission of the accretion disc. Additional spectral features, namely a reflection component, a high-energy cut-off, and excess emission at 6.4 keV, are taken into account. Our investigations confirm the known positive…
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