activity
20062026
most citedDiscovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13

338 citations · 1.3k across the 48 of their papers we have counts for

collaborators

49 papers

astro-ph.HE2026

Understanding Pulsar Magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +21

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.HE2025

Understanding pulsar magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +22

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.HE2025

A magnetar outburst with atypical evolution: the case of Swift J1555.2-5402

A. Borghese, F. Coti Zelati, M. Imbrogno +12

The magnetar Swift J1555.2-5402 was discovered in outburst on 2021 June 3 by the Burst Alert Telescope on board the Swift satellite. Early X-ray follow-up revealed a spin period P~…

astro-ph.HE2021★ 4 cited

Detecting the intrinsic X-ray emission from the O-type donor star and the residual accretion in a Supergiant Fast X-ray Transient during its faintest state

L. Sidoli, K. Postnov, L. Oskinova +4

We report on the results of an XMM-Newton observation of the Supergiant Fast X-ray Transient (SFXT) IGR J08408-4503 performed in June 2020. The source is composed by a compact obje…

astro-ph.HE2020★ 15 cited

The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars

A. Papitto, M. Falanga, W. Hermsen +30

In the last 25 years, a new generation of X-ray satellites imparted a significant leap forward in our knowledge of X-ray pulsars. The discovery of accreting and transitional millis…

astro-ph.HE2020★ 67 cited

A very young radio-loud magnetar

P. Esposito, N. Rea, A. Borghese +20

The magnetar Swift ,J1818.0-1607 was discovered in March 2020 when Swift detected a 9 ms hard X-ray burst and a long-lived outburst. Prompt X-ray observations revealed a spin perio…