activity
20172026
most citedINTEGRAL discovery of a burst with associated radio emission from the magnetar SGR 1935+2154

348 citations · 527 across the 29 of their papers we have counts for

collaborators
Showing 2022 · astro-ph.HEShow all

5 papers · 2 filters

astro-ph.HE2022

Deep X-ray and radio observations of the first outburst of the young magnetar Swift J1818.0-1607

A. Y. Ibrahim, A. Borghese, N. Rea +23

Swift J1818.0-1607 is a radio-loud magnetar with a spin period of 1.36 s and a dipolar magnetic field strength of B~3E14 G, which is very young compared to the Galactic pulsar popu…

astro-ph.HE2022★ 14 cited

Two decades of X-ray observations of the isolated neutron star RX J1856.5-3754: detection of thermal and non-thermal hard X-rays and refined spin-down measurement

Davide De Grandis, Michela Rigoselli, Sandro Mereghetti +6

The soft X-ray pulsar RX J1856.5-3754 is the brightest member of a small class of thermally-emitting, radio-silent, isolated neutron stars. Its X-ray spectrum is almost indistingui…

astro-ph.HE2022★ 19 cited

Thermal and non-thermal X-ray emission from the rotation-powered radio/-ray pulsar PSR J1740+1000

Michela Rigoselli, Sandro Mereghetti, Sara Anzuinelli +4

We report the results of new XMM-Newton observations of the middle-aged (10 yr) radio pulsar PSR J1740+1000 carried out in 2017-2018. These long pointings (530 ks)…

astro-ph.HE2022★ 2 cited

X-ray observation of the Roche-lobe filling white dwarf plus hot subdwarf system ZTF J213056.71+442046.5

S. Mereghetti, N. La Palombara, T. Kupfer +9

ZTF J213056.71+442046.5 is the prototype of a small class of recently discovered compact binaries composed of a white dwarf and a hot subdwarf that fills its Roche-lobe. Its orbita…

astro-ph.HE2022★ 6 cited

GRB 190919B: Rapid optical rise explained as a flaring activity

Martin Jelínek, Martin Topinka, Sergey Karpov +17

Following the detection of a long GRB 190919B by INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory), we obtained an optical photometric sequence of its optical counterpart.…