activity
20042026
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 6.3k across the 124 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

36 papers · 1 filter

astro-ph.HE2023★ 2 cited

Science with a small two-band UV-photometry mission III: Active Galactic Nuclei and nuclear transients

M. Zajaček, B. Czerny, V. K. Jaiswal +14

In this review (the third in the series focused on a small two-band UV-photometry mission), we assess possibilities for a small UV two-band photometry mission in studying accreting…

astro-ph.HE2023

Science with a small two-band UV-photometry mission I: Mission description and follow-up observations of stellar transients

N. Werner, J. Řípa, C. Thöne +33

This is the first in a collection of three papers introducing the science with an ultra-violet (UV) space telescope on an approximately 130~kg small satellite with a moderately fas…

astro-ph.HE2023★ 1 cited

CAvity DEtection Tool (CADET): Pipeline for automatic detection of X-ray cavities in hot galactic and cluster atmospheres

Tomáš Plšek, Norbert Werner, Martin Topinka +1

The study of jet-inflated X-ray cavities provides a powerful insight into the energetics of hot galactic atmospheres and radio-mechanical AGN feedback. By estimating the volumes of…

astro-ph.HE2023★ 23 cited

The peak-flux of GRB 221009A measured with GRBAlpha

Jakub Ripa, Hiromitsu Takahashi, Yasushi Fukazawa +42

The brightest gamma-ray burst ever observed, long-duration GRB 221009A, was detected by GRBAlpha nano-satellite without saturation. We present light curves of the prompt emission i…

astro-ph.HE2022★ 10 cited

Chandra measurements of gas homogeneity and turbulence at intermediate radii in the Perseus Cluster

Martijn de Vries, Adam B. Mantz, Steven W. Allen +6

We present a Chandra study of surface brightness fluctuations in the diffuse intracluster medium of the Perseus Cluster. Our study utilizes deep, archival imaging of the cluster co…

astro-ph.HE2022★ 2 cited

A multifrequency characterization of the extragalactic hard X-ray sky

Matej Kosiba, Harold Andres Peña-Herazo, Francesco Massaro +5

Nowadays we know that the origin of the Cosmic X-ray Background (CXB) is due to the integrated emission of nearby active galactic nuclei. Thus, to obtain a precise estimate of the…