A Statistical Study on the Low-Frequency QPO Amplitude Spectrum and Amplitude in GRS 1915+105
Shu-Ping Yan, Guo-Qiang Ding, Na Wang, Jin-Lu Qu, and Li-Ming Song

TL;DR
This study analyzes the energy dependence and amplitude of low-frequency QPOs in GRS 1915+105, revealing that their spectral properties are similar across different jet states and likely originate from the corona rather than the jets.
Contribution
It provides a detailed statistical analysis of the LFQPO amplitude spectrum and its relation to jet activity, offering insights into the origin of QPOs in black hole binaries.
Findings
LFQPO amplitude spectrum fits a power-law with exponential cutoff
LFQPO spectra are similar across different jet states
LFQPOs likely originate from the corona, not the jets
Abstract
A statistical study was made on both the energy dependence of the low-frequency quasi-periodic oscillation (QPO) amplitude (LFQPO amplitude spectrum) and the LFQPO amplitude from all the RXTE observations of GRS 1915+105. Based on the two-branch correlation of the LFQPO frequency and the hardness ratio, the observations that were suitable for evaluating the LFQPO amplitude spectrum were divided into two groups. According to a comparison between the radio and X-ray emissions, we deduced that the jets during the two groups of observations are very different. A negative correlation between the LFQPO frequency and the radio flux was found for one group. The LFQPO amplitude spectrum was fitted by a power-law with an exponential cutoff in order to describe it quantitatively. It reveals that as the LFQPO frequency increases, the power-law hardens. And the cutoff energy firstly decreases, and…
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