activity
19992026
most citedINTEGRAL discovery of a burst with associated radio emission from the magnetar SGR 1935+2154

348 citations · 2.2k across the 72 of their papers we have counts for

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Showing 2023Show all

8 papers · 1 filter

astro-ph.HE2023★ 1 cited

Hard X-rays and QPO in Swift J1727.8-1613: the rise and plateau of the 2023 outburst

I. Mereminskiy, A. Lutovinov, S. Molkov +5

We report on the detection of type-C quasi-periodic oscillations during the initial stages of the outburst of Swift J1727.8-1613 in 2023. Using data of the INTEGRAL observatory alo…

astro-ph.HE2023★ 29 cited

Complex variations of X-ray polarization in the X-ray pulsar LS V +44 17/RX J0440.9+4431

Victor Doroshenko, Juri Poutanen, Jeremy Heyl +109

We report on Imaging X-ray polarimetry explorer (IXPE) observations of the Be-transient X-ray pulsar LS V +44 17/RX J0440.9+4431 made at two luminosity levels during the giant outb…

astro-ph.HE2023★ 24 cited

A polarimetrically oriented X-ray stare at the accreting pulsar EXO 2030+375

Christian Malacaria, Jeremy Heyl, Victor Doroshenko +104

Accreting X-ray pulsars (XRPs) are presumably ideal targets for polarization measurements, as their high magnetic field strength is expected to polarize the emission up to a polari…

astro-ph.HE2023★ 24 cited

X-ray polarimetry of the accreting pulsar GX 301-2

Valery F. Suleimanov, Sofia V. Forsblom, Sergey S. Tsygankov +102

The phase- and energy-resolved polarization measurements of accreting X-ray pulsars (XRPs) allow us to test different theoretical models of their emission, and they also provide an…

astro-ph.HE2023★ 17 cited

RX J0440.9+4431: another supercritical X-ray pulsar

Alexander Salganik, Sergey S. Tsygankov, Victor Doroshenko +4

In the beginning of 2023 the Be transient X-ray pulsar RX J0440.9+4431 underwent a fist-ever giant outburst observed from the source peaking in the beginning of February and reachi…

astro-ph.HE2023★ 5 cited

Study of the X-ray Pulsar IGR J21343+4738 based on NuSTAR, Swift, and SRG data

A. S. Gorban, S. V. Molkov, A. A. Lutovinov +1

We present the results of our study of the X-ray pulsar IGR J21343+4738 based on NuSTAR, Swift, and SRG observations in the wide energy range 0.3 - 79 keV. The absence of absorptio…