activity
19972025
most citedEvidence for Spin and Energy Extraction in a Galactic Black Hole Candidate: The XMM-Newton/EPIC-pn Spectrum of XTE J1650-500

224 citations · 1.9k across the 43 of their papers we have counts for

collaborators

44 papers

astro-ph.GA2025

XMM-Newton Conclusively Identifies an Active Galactic Nucleus in a Green Pea Galaxy

Peter G. Boorman, Jiří Svoboda, Daniel Stern +23

Green Pea galaxies are a class of compact, low-mass, low-metallicity star-forming galaxies in the relatively local universe. They are believed to be analogues of high-redshift gala…

astro-ph.GA2024★ 8 cited

Radio properties of Green Pea galaxies

Abhijeet Borkar, Romana Grossová, Jiří Svoboda +6

Green Peas (GPs) are young, compact, star-forming dwarf galaxies, and local (z~0.3) analogues of the early galaxies (z>6) considered to be mainly responsible for the reionisation o…

astro-ph.GA2022★ 4 cited

Hot magnetic halo of NGC628 (M74)

M. Wezgowiec, R. Beck, M. Hanasz +4

In several spiral galaxies that are observed face-on, large-scale ordered magnetic fields (the so-called magnetic arms) were found. One of the explanations was the action of the ma…

astro-ph.GA2022★ 2 cited

Magnetic fields and hot gas in M101

M. Wezgowiec, R. Beck, M. Hanasz +4

Studies of nearby spiral galaxies in radio and X-ray wavelengths reveal the structure and energy balance of the magnetic fields and the hot interstellar medium (ISM). In some spira…

astro-ph.IM2021

INTEGRAL reloaded: spacecraft, instruments and ground system

Erik Kuulkers, Carlo Ferrigno, Peter Kretschmar +85

ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up t…

astro-ph.GA2020★ 6 cited

Hot gas heating via magnetic arms in spiral galaxies. The case of M 83

M. Wezgowiec, M. Ehle, M. Soida +3

Reconnection heating has been considered as a potential source of the heating of the interstellar medium. In some galaxies, significant polarised radio emission has been found betw…