activity
20152021
most citedDiscovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13

338 citations · 424 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2021★ 27 cited

The EXTraS Project: Exploring the X-ray transient and variable sky

A. De Luca, R. Salvaterra, A. Belfiore +29

Temporal variability in flux and spectral shape is ubiquitous in the X-ray sky and carries crucial information about the nature and emission physics of the sources. The EPIC instru…

astro-ph.HE2020★ 36 cited

A Supernova Candidate at z=0.092 in XMM-Newton Archival Data

G. Novara, P. Esposito, A. Tiengo +14

During a search for X-ray transients in the XMM-Newton archive within the EXTraS project, we discovered a new X-ray source that is detected only during a ~5 min interval of a ~21 h…

astro-ph.IM2019★ 7 cited

A science gateway for Exploring the X-ray Transient and variable sky using EGI Federated Cloud

Daniele D'Agostino, Luca Roverelli, Gabriele Zereik +7

Modern soft X-ray observatories can yield unique insights into time domain astrophysics, and a huge amount of information is stored - and largely unexploited - in data archives. Li…

astro-ph.HE2018★ 8 cited

The two tails of PSR J2055+2539 as seen by Chandra: analysis of the nebular morphology and pulsar proper motion

Martino Marelli, Andrea Tiengo, Andrea De Luca +4

We analyzed two Chandra observations of PSR J2055+2539 (for a total integration time of 130 ks) in order to measure its proper motion and study its two elongated nebular feat…

astro-ph.HE2016★ 338 cited

Discovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13

G. L. Israel, A. Papitto, P. Esposito +11

NGC 7793 P13 is a variable (luminosity range ~100) ultraluminous X-ray source (ULX) proposed to host a stellar-mass black hole of less than 15 M in a binary system with o…

astro-ph.SR2015★ 8 cited

Results from DROXO IV. EXTraS discovery of an X-ray flare from the Class I protostar candidate ISO-Oph 85

Daniele Pizzocaro, Beate Stelzer, Roberta Paladini +15

X-ray emission from Young Stellar Objects (YSOs) is crucial to understand star formation. A very limited amount of X-ray results is available for the protostellar (ClassI) phase. A…