Bright flare in the obscured state of GRS 1915+105 as seen by NICER and Swift
astro-ph.HE
Submitted: 2026-04-13
Updated: 2026-09-09
Comments: 16 pages, 13 figures. v2: refereed version
Journal ref: Phys. Rev. D 114, 063018 (2026)
DOI: 10.1103/3j4t-pc75
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- GRS 1915+105 in "Soft State": Nature of Accretion Disk Wind and Origin of X-Ray Emission
- A model-independent analysis of the variability of GRS 1915+105
- An Obscured, Seyfert-2-like State of the Stellar-mass Black Hole GRS 1915+105 Caused by Failed Disk Winds
- The Novel Obscured State of Stellar-mass Black Hole GRS 1915+105
- Observations of a radio-bright, X-ray obscured GRS 1915+105
- A NICER View of a Highly-Absorbed Flare in GRS 1915+105
- The obscured X-ray binaries V404 Cyg, Cyg X-3, V4641 Sgr, and GRS 1915+105
- An Unusual Change in the Radio Jets of GRS 1915+105
- The Burst Alert Telescope (BAT) on the Swift MIDEX Mission
- The MAXI Mission on the ISS: Science and Instruments for Monitoring All Sky X-Ray Images
- Multi-mission view of low-luminosity 'obscured' phase of GRS 1915+105
- Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-ray Data Set
- Optimal binning of X-ray spectra and response matrix design
- The Swift X-ray Telescope
- On the Absorption of X-rays in the Interstellar Medium
- Broad-band gamma-ray and X-ray spectra of NGC 4151 and their implications for physical processes and geometry
- The May 1989 outburst of the Soft X-ray Transient GS 2023+338 (V404 Cyg)
- Self-Consistent Black Hole Accretion Spectral Models and the Forgotten Role of Coronal Comptonization of Reflection Emission
- X-ray reflected spectra from accretion disk models. III. A complete grid of ionized reflection calculations
- Variable iron-line emission near the black hole of Markarian 766
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