activity
20172022
most citedOrbital period dependent spatial scatter of Galactic Black Hole Transients

23 citations · 88 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2022★ 10 cited

Using the bispectrum to probe radio X-ray correlations in GRS 1915+105

K. Arur, T. J. Maccarone

We present the results of bicoherence analysis on observations of GRS 1915+105 that exhibit quasi-periodic oscillations (QPOs). The bicoherence is a higher order statistic that can…

astro-ph.HE2020★ 23 cited

Orbital period dependent spatial scatter of Galactic Black Hole Transients

P. Gandhi, A. Rao, P. A. Charles +4

There remain significant uncertainties in the origin and evolution of black holes in binary systems, in particular regarding their birth sites and the influence of natal kicks. The…

astro-ph.HE2019★ 12 cited

A Likely Inclination Dependence in the Non-linear Variability of Quasi Periodic Oscillations from Black Hole Binaries

Arur. K, Maccarone. T. J

We present a systematic analysis of the effects of orbital inclination angle on the non-linear variability properties of type-B and type-C QPOs from black hole binaries. We use the…

astro-ph.HE2019★ 11 cited

Nonlinear Variability of Quasi-Periodic Oscillations in GX 339-4

K. Arur, T. J. Maccarone

We examine the nonlinear variability of quasi-periodic oscillations (QPOs) using the bicoherence, a measure of phase coupling at different Fourier frequencies. We analyse several o…

astro-ph.HE2017★ 15 cited

Chandra X-ray Constraints on the Candidate Ca-rich Gap Transient SN 2016hnk

P. H. Sell, K. Arur, T. J. Maccarone +4

We present a Chandra observation of SN 2016hnk, a candidate Ca-rich gap transient. This observation was specifically designed to test whether or not this transient was the result o…

astro-ph.HE2017★ 17 cited

Selection Effects on the Orbital Period Distribution of Low Mass Black Hole X-ray Binaries

K. Arur, T. J. Maccarone

We investigate the lack of observed low mass black hole binary systems at short periods ( < 4 hours) by comparing the observed orbital period distribution of 17 confirmed low mass…