activity
20162024
most citedDisk, Corona, Jet Connection in the Intermediate State of MAXI J1820+070 Revealed by NICER Spectral-Timing Analysis

96 citations · 361 across the 17 of their papers we have counts for

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Showing 2019Show all

5 papers · 1 filter

astro-ph.HE2019

Evolution of the accretion disk-corona during bright hard-to-soft state transition: A reflection spectroscopic study with GX 339-4

Navin Sridhar, Javier A. García, James F. Steiner +3

We present the analysis of several observations of the black hole binary GX 339--4 during its bright intermediate states from two different outbursts (2002 and 2004), as observed b…

astro-ph.HE2019

The 2017 Failed Outburst of GX 339-4: Relativistic X-ray Reflection near the Black Hole Revealed by NuSTAR and Swift Spectroscopy

Javier A. García, John A. Tomsick, Navin Sridhar +12

We report on the spectroscopic analysis of the black hole binary GX 339-4 during its recent 2017-2018 outburst, observed simultaneously by the Swift and NuSTAR observatories. Altho…

astro-ph.HE2019

Conflicting disk inclination estimates for the black hole X-ray binary XTE J1550-564

Riley~M. ~T. ~Connors, Javier~A. ~Garcia, James~F. ~Steiner +7

XTE J1550-564 is a black hole X-ray binary for which the dynamical characteristics are well established, and the broadband spectral evolution of the source has been well studied. I…

astro-ph.HE2019

Probing the Black Hole Engine with Measurements of the Relativistic X-ray Reflection Component

Javier A. García, Matteo Bachetti, David R. Ballantyne +21

Over the last decades X-ray spectroscopy has proven to be a powerful tool for the estimation of black hole spin and several other key parameters in dozens of AGN and black hole X-r…

astro-ph.HE2019★ 19 cited

Combining timing characteristics with physical broadband spectral modelling of black hole X-ray binary GX~3394

Riley M. T. Connors, David van Eijnatten, Sera Markoff +6

GX~3394 is a black hole X-ray binary that is a key focus of accretion studies since it goes into outburst roughly every two-to-three years. Tracking of its radio, IR and X-ray f…