output
20022026
most citedParticle-flow reconstruction and global event description with the CMS detector

995 citations

Showing 2025 · astro-ph.HEShow all

7 papers · 2 filters

astro-ph.HE2025★ 1 cited

Revealing the accelerating wind in the inner region of the colliding-wind binary WR 112

John D. Monnier, Yinuo Han, Michael F. Corcoran +17

Colliding winds in massive binaries generate X-ray-bright shocks, synchrotron radio emission, and sometimes even dusty "pinwheel" spirals. We report the first X-ray detections of t…

astro-ph.HE2025

Solar Cycle Variation of Sustained Gamma Ray Emission from the Sun

Nat Gopalswamy, Pertti Mäkelä, Seiji Yashiro +3

We investigated the occurrence rate of the sustained gamma ray emission (SGRE) events from the Sun using data obtained by Fermi Large Area Telescope (LAT) since its launch in 2008.…

astro-ph.HE2025★ 2 cited

The Intermediate Mass Black Hole in Omega Centauri: Constraints on Accretion from JWST

Steven Chen, Jeremy Hare, Oleg Kargaltsev +4

We analyze JWST observations of the central region of the globular cluster Centauri (NGC 5139, Cen hereafter), around the position of the candidate IMBH inferred by \cite{h…

astro-ph.HE2025

Testing Magnetic Field Configurations in Spider Pulsar PSR J1723-2837 with IXPE

Michela Negro, Haocheng Zhang, Niccolò Di Lalla +4

We present the first X-ray polarimetry observations of a redback millisecond pulsar binary, PSR J1723-2837, with the Imaging X-ray Polarimetry Explorer (IXPE). We conduct a spectro…

astro-ph.HE2025★ 5 cited

The Vela pulsar and its pulsar wind nebula Vela-X using 13 years of Fermi-LAT Observations

Alexander Lange, J. Eagle, O. Kargaltsev +2

We present results of more than 13 years of Fermi-LAT data analysis for the Vela pulsar from 60 MeV to 100 GeV and its pulsar wind nebula (PWN), Vela-X, for E > 1 GeV in the off-pu…

astro-ph.HE2025★ 11 cited

Unraveling the structure of the stratified ultra-fast outflows in PDS 456 with XRISM

Yerong Xu, Luigi C. Gallo, Kouichi Hagino +18

Multiple clumpy wind components () in the luminous quasar PDS 456 have recently been resolved by XRISM in the Fe-K band for the first time. In this paper, we i…