activity
20082026
most citedOverview of the Advanced X-ray Imaging Satellite (AXIS)

77 citations · 110 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

A Changing-Look Seyfert Discovered by eROSITA Reveals a Two-Component Broad-Line Region

Alex Markowitz, Mirko Krumpe, David Homan +12

Extreme sudden changes in the flow of accreting gas onto SMBHs manifest themselves via large-amplitude continuum variability and changes to broad Balmer emission profiles, driving…

astro-ph.HE2026

BLAZ4R and the eROSITA view of z>4 blazars

Tullia Sbarrato, Silvia Belladitta, Julien Wolf +8

We present BLAZ4R, the first living catalog of confirmed blazars, with a focus on the contribution of eROSITA, on board of the Spectrum Roentgen Gamma (SRG) spacecraft. Blaza…

astro-ph.HE2025

Unprecedentedly bright X-ray flaring in Cygnus X-1 observed by INTEGRAL

P. Thalhammer, T. Bouchet, J. Rodriguez +15

We study three extraordinarily bright X-ray flares originating from Cyg X-1 seen on 2023 July 10 detected with INTEGRAL. The flares had a duration on the order of only ten minutes…

astro-ph.HE2025★ 4 cited

Don't torque like that. Measuring compact object magnetic fields with analytic torque models

J. J. R. Stierhof, E. Sokolova-Lapa, K. Berger +10

Context. Changes of the rotational period observed in various magnetized accreting sources are generally attributed to the interaction between the in-falling plasma and the large-s…

astro-ph.HE2024★ 1 cited

Characterisation of the stellar wind in Cyg X-1 via modelling of colour-colour diagrams

E. V. Lai, B. De Marco, Y. Cavecchi +11

Cygnus X-1 is a high mass X-ray binary where accretion onto the black hole is mediated by the stellar wind from the blue supergiant companion star HDE 226868. Depending on the posi…

astro-ph.HE2024★ 10 cited

INTEGRAL/IBIS polarization detection in the hard and soft intermediate states of Swift J1727.8-1613

Tristan Bouchet, Jérôme Rodriguez, Floriane Cangemi +5

Soft gamma-ray emission (100 keV -- 10 MeV) has previously been detected in the hard state of several microquasars. In some sources, this emission was found to be highly polarized…