#x-ray astronomy

topicx-ray astronomy

8 papers · 1 filter

astro-ph.HE2026

Multiwavelength study of supernova remnants in the Circinus constellation with SRG/eROSITA

A. Khokhriakova, W. Becker

The paper combines optical, radio, and eROSITA X‑ray data to search for and characterize supernova remnant candidates in the Circinus constellation, identifying several new candida…

astro-ph.CO2026

A study of the large-scale formation in the environment of A3266: Infalling groups, filaments, and a premerger cold front

J. Dietl, A. Veronica, T. H. Reiprich +7

The paper uses eROSITA X‑ray data to map the outskirts of the galaxy cluster Abell 3266, revealing a hot X‑ray filament linking the cluster to a nearby group and showing how the cl…

astro-ph.SR2026

The X-ray catalogue of FGK stars within 10 pc: The coronal temperature-brightness relation explained with the RTV scaling law

M. M. Bennedik, B. Stelzer, M. Caramazza +3

The authors compile an X‑ray catalog of FGK main‑sequence stars within 10 pc, derive coronal temperatures and X‑ray fluxes from eROSITA, XMM‑Newton and ROSAT data, and show that th…

astro-ph.IM2026

High-statistics simulations of NewAthena WFI background using Geant4

Matthew K. Heine, Catherine E. Grant, Marshall W. Bautz +14

The paper presents high‑statistics Geant4 simulations of the background caused by cosmic‑ray interactions in the Wide Field Imager of ESA's NewAthena X‑ray observatory, using both…

astro-ph.HE2026

Towards a joint X-ray and gamma-ray analysis of Pulsar Wind Nebulae with Gammapy

Katharina Egg, Alison M. W. Mitchell

The paper describes how the authors adapt eROSITA X-ray data and H.E.S.S. gamma-ray data for joint analysis of pulsar wind nebulae using the Gammapy Python package.

astro-ph.GA2026

When X-ray Features Fail to Identify Intrinsic Emitters: Label Noise and Luminosity Overlap in Machine Learning Classification of AGN and Star-forming Galaxies

Jaymin Ding

The paper shows that adding X‑ray flux as a feature to a Random Forest classifier of AGN and star‑forming galaxies reduces accuracy because the X‑ray luminosities of the two classe…