Detection of the first infra-red quasi periodic oscillation in a black hole X-ray binary
M. Kalamkar, P. Casella, P. Uttley, K. O'Brien, D. Russell, T., Maccarone, M. van der Klis, F. Vincentelli

TL;DR
This study reports the first detection of an infra-red quasi-periodic oscillation in a black hole X-ray binary, revealing correlations across IR, optical, and X-ray bands and suggesting a jet origin for the IR variability.
Contribution
It provides the first evidence of IR QPOs in a black hole binary and explores their relation to X-ray QPOs, advancing understanding of jet and accretion processes.
Findings
IR QPO detected at 0.08 Hz, half the X-ray QPO frequency
Strong IR/X-ray variability correlation with X-rays leading by 100 ms
Jet synchrotron emission likely responsible for IR QPO
Abstract
We present analysis of fast variability of Very Large Telescope/ISAAC (infra-red), \textit{XMM-Newton}/OM (optical) and EPIC-pn (X-ray), and RXTE/PCA (X-ray) observations of the black hole X-ray binary GX 339-4 in a rising hard state of its outburst in 2010. We report the first detection of a Quasi Periodic Oscillation (QPO) in the infra-red band (IR) of a black hole X-ray binary. The QPO is detected at 0.08 Hz in the IR as well as two optical bands (U and V). Interestingly, these QPOs are at half the X-ray QPO frequency at 0.16 Hz, which is classified as the type-C QPO; a weak sub-harmonic close to the IR and optical QPO frequency is also detected in X-rays. The broad band sub-second time scale variability is strongly correlated in IR/X-ray bands, with X-rays leading the IR by over 100 ms. This short time delay, shape of the cross correlation function and spectral energy distribution…
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