activity
20092026
most citedThe eROSITA X-ray telescope on SRG

884 citations · 7.7k across the 224 of their papers we have counts for

collaborators
Showing 2021Show all

29 papers · 1 filter

astro-ph.HE2021★ 5 cited

X-ray spectral-timing variability of 1A 0535+262 during the 2020 giant outburst

P. Reig, R. C. Ma, L. Tao +3

The Be/X-ray binary 1A 0535+262 underwent a giant X-ray outburst in November 2020, peaking at erg s (1--100 keV, 1.8 kpc), the brightest outburst recor…

astro-ph.HE2021★ 13 cited

Searching for TeV gamma-ray emission from SGR\,1935+2154 during its 2020 X-ray and radio bursting phase

H. E. S. S. Collaboration, :, H. Abdalla +251

Magnetar hyperflares are the most plausible explanation for fast radio bursts (FRB) -- enigmatic powerful radio pulses with durations of several milliseconds and high brightness te…

hep-ex2021★ 1 cited

Combined dark matter searches towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, H.E.S.S., MAGIC, and VERITAS

Celine Armand, Eric Charles, Mattia di Mauro +13

Cosmological and astrophysical observations suggest that 85\% of the total matter of the Universe is made of Dark Matter (DM). However, its nature remains one of the most challengi…

astro-ph.HE2021★ 16 cited

eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds

F. Haberl, C. Maitra, S. Carpano +8

During its performance verification phase, the soft X-ray instrument eROSITA aboard the Spektrum-Roentgen-Gamma(SRG) spacecraft observed large regions in the Magellanic Clouds, whe…

astro-ph.HE2021★ 2 cited

Search for dark matter annihilation signals from the Galactic Center with the H.E.S.S. Inner Galaxy Survey

A. Montanari, E. Moulin, D. Malyshev

The presence of dark matter (DM) is suggested by a wealth of astrophysical and cosmological measurements. However, its underlying nature is yet unknown. Among the most promising ca…

astro-ph.HE2021★ 6 cited

SRG/ART-XC, Swift, NICER and NuSTAR study of different states of the transient X-ray pulsar MAXI J0903-531

Sergey S. Tsygankov, Sergey V. Molkov, Victor Doroshenko +6

The results of the broadband spectral and timing study of the recently discovered transient X-ray pulsar MAXI J0903-531 in a wide range of luminosities differing by a factor of ~30…

astro-ph.HE2021★ 2 cited

The young massive stellar cluster Westerlund 1 in rays as seen with H.E.S.S

Lars Mohrmann, Andreas Specovius, Romed Rauth +2

Massive stellar clusters have recently been hypothesised as candidates for the acceleration of hadronic cosmic rays up to PeV energies. Previously, the H.E.S.S. Collaboration has r…

astro-ph.HE2021

Evidence of 100 TeV -ray emission from HESS J1702-420: A new PeVatron candidate

L. Giunti, B. Khelifi, K. Kosack +1

The identification of active PeVatrons, hadronic particle accelerators reaching the knee of the cosmic-ray spectrum (at the energy of few PeV), is crucial to understand the origin…

astro-ph.HE2021

Luminosity dependence of the cyclotron line energy in 1A 0535+262 observed by Insight-HXMT during 2020 giant outburst

L. D. Kong, S. Zhang, L. Ji +11

We report on a detailed spectral analysis of the transient X-ray pulsar 1A~0535+262, which underwent the brightest giant outburst ever recorded for this source from November to Dec…

astro-ph.IM2021

Science verification of the new FlashCam-based camera in the 28m telescope of H.E.S.S

Gerd Pühlhofer, Konrad Bernlöhr, Baiyang Bi +13

In October 2019 the central 28m telescope of the H.E.S.S. experiment has been upgraded with a new camera. The camera is based on the FlashCam design which has been developed in vie…

astro-ph.HE2021

Detection of extended TeV emission around the Geminga pulsar with H.E.S.S

A. M. W. Mitchell, S. Caroff, J. Hinton +1

Highly extended gamma-ray emission around the Geminga pulsar was discovered by Milagro and verified by HAWC. Despite many observations with Imaging Atmospheric Cherenkov Telescopes…

astro-ph.HE2021★ 3 cited

Detection of new Extreme BL Lac objects with H.E.S.S. and Swift XRT

Mathieu de Bony de Lavergne, Tomas Bylund, Manuel Meyer +2

Extreme high synchrotron peaked blazars (EHBLs) are amongst the most powerful accelerators found in nature. Usually the synchrotron peak frequency of an EHBL is above Hz…

astro-ph.HE2021★ 13 cited

LMC N132D: A mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV

H. E. S. S. Collaboration, :, H. Abdalla +233

We analyzed 252 hours of High Energy Stereoscopic System (H.E.S.S.) observations towards the supernova remnant (SNR) LMC N132D that were accumulated between December 2004 and March…

astro-ph.IM2021

Astronomy outreach in Namibia: H.E.S.S. and beyond

Hannah Dalgleish, Heike Prokoph, Sylvia Zhu +6

Astronomy plays a major role in the scientific landscape of Namibia. Because of its excellent sky conditions, Namibia is home to ground-based observatories like the High Energy Spe…

astro-ph.IM2021★ 28 cited

TeV emission of Galactic plane sources with HAWC and H.E.S.S

H. Abdalla, F. Aharonian, F. Ait Benkhali +318

The High Altitude Water Cherenkov (HAWC) observatory and the High Energy Stereoscopic System (H.E.S.S.) are two leading instruments in the ground-based very-high-energy gamma-ray d…

astro-ph.HE2021

eROSITA detection of flares from the Be/X-ray binary A0538-66

L. Ducci, S. Mereghetti, A. Santangelo +8

In 2018, XMM-Newton observed the awakening in X-rays of the Be/X-ray binary (Be/XRB) A0538-66. It showed bright and fast flares close to periastron with properties that had never b…

astro-ph.HE2021★ 13 cited

SRGA J124404.1-632232/SRGU J124403.8-632231: a new X-ray pulsar discovered in the all-sky survey by SRG

V. Doroshenko, R. Staubert, C. Maitra +12

Ongoing all-sky surveys by the the eROSITA and the Mikhail Pavlinsky ART-XC telescopes on-board the Spectrum Roentgen Gamma (SRG) mission have already revealed over a million of X-…

astro-ph.HE2021★ 15 cited

Phase-resolved X-ray spectroscopy of PSR B0656+14 with SRG/eROSITA and XMM-Newton

Axel Schwope, Adriana M. Pires, Jan Kurpas +13

(abridged version) We present a detailed spectroscopic and timing analysis of X-ray observations of the bright radio-to-gamma-ray emitting pulsar PSR B0656+14, which were obtained…

astro-ph.HE2021★ 20 cited

Discovery of the 5 keV cyclotron line followed by three harmonics in SwiftJ1626.6-5156

S. Molkov, V. Doroshenko, A. Lutovinov +4

We report on observations of the Be/X-ray binary system SwiftJ1626.6-5156 performed with NuSTAR during a short outburst in March 2021, following its detection of by the MAXI monito…

astro-ph.HE2021★ 14 cited

Search for dark matter annihilation signals from unidentified Fermi-LAT objects with H.E.S.S

H. E. S. S. Collaboration, H. Abdallah, F. Aharonian +226

Cosmological -body simulations show that Milky Way-sized galaxies harbor a population of unmerged dark matter subhalos. These subhalos could shine in gamma-rays and be eventuall…

astro-ph.HE2021★ 24 cited

Evidence of 100 TeV -ray emission from HESS J1702-420: A new PeVatron candidate

H. Abdalla, F. Aharonian, F. Ait Benkhali +232

The identification of PeVatrons, hadronic particle accelerators reaching the knee of the cosmic ray spectrum (few eV), is crucial to understand the origin of cosmic rays…

astro-ph.HE2021★ 172 cited

Revealing x-ray and gamma ray temporal and spectral similarities in the GRB 190829A afterglow

H. E. S. S. Collaboration

Gamma-ray bursts (GRBs), which are bright flashes of gamma rays from extragalactic sources followed by fading afterglow emission, are associated with stellar core collapse events.…

astro-ph.HE2021★ 19 cited

Search for dark matter annihilation in the dwarf irregular galaxy WLM with H.E.S.S

H. E. S. S. Collaboration, H. Abdallah, R. Adam +232

We search for an indirect signal of dark matter through very high-energy gamma rays from the Wolf-Lundmark-Melotte (WLM) dwarf irregular galaxy. The pair annihilation of dark matte…

astro-ph.IM2021

Time Domain Astronomy with the THESEUS Satellite

S. Mereghetti, S. Balman, M. Caballero-Garcia +74

THESEUS is a medium size space mission of the European Space Agency, currently under evaluation for a possible launch in 2032. Its main objectives are to investigate the early Univ…