activity
20062020
most citedAcceleration of petaelectronvolt protons in the Galactic Centre

512 citations · 9.5k across the 162 of their papers we have counts for

collaborators

166 papers

astro-ph.HE2020★ 5 cited

Modeling of 35-day superorbital cycle of and light curves of IMXB HZ Her/Her X-1

D. A. Kolesnikov, N. I. Shakura, K. A. Postnov +13

The X-ray binary Her X-1 consists of an accreting neutron star and the optical component HZ Her. The 35-day X-ray superorbital variability of this system is known since its discove…

astro-ph.HE2019★ 11 cited

The giant outburst of 4U 0115+634 in 2011 with Suzaku and RXTE

Matthias Bissinger né Kühnel, Ingo Kreykenbohm, Carlo Ferrigno +19

We present an analysis of X-ray spectra of the high mass X-ray binary 4U 0115+634 as observed with Suzaku and RXTE in 2011 July, during the fading phase of a giant X-ray outburst.…

astro-ph.HE2018★ 241 cited

Cyclotron lines in highly magnetized neutron stars

R. Staubert, J. Trümper, E. Kendziorra +10

Cyclotron lines, also called cyclotron resonant scattering features (CRSF) are spectral features, generally appearing in absorption, in the X-ray spectra of objects containing high…

astro-ph.HE2018★ 50 cited

The -ray spectrum of the core of Centaurus A as observed with H.E.S.S. and Fermi-LAT

H. E. S. S. Collaboration, H. Abdalla, A. Abramowski +249

Centaurus A (Cen A) is the nearest radio galaxy discovered as a very-high-energy (VHE; 100 GeV-100 TeV) -ray source by the High Energy Stereoscopic System (H.E.S.S.). It is a fa…

astro-ph.HE2018★ 16 cited

Infrared and X-ray study of the Galactic SNR G15.9+0.2

Manami Sasaki, Minja M. Maäkelaä, Dmitry Klochkov +2

G15.9+0.2 is a Galactic shell-type supernova remnant (SNR), which was detected in radio and has been confirmed in X-rays based on Chandra observations. An X-ray point source CXOUJ1…

astro-ph.HE2018★ 33 cited

H.E.S.S. discovery of very high energy gamma-ray emission from PKS 0625-354

H. E. S. S. Collaboration, H. Abdalla, A. Abramowski +253

PKS 0625-354 (z=0.055) was observed with the four H.E.S.S. telescopes in 2012 during 5.5 hours. The source was detected above an energy threshold of 200 GeV at a significance level…