activity
19952025
most citedThe Large Observatory for X-ray Timing (LOFT)

214 citations · 608 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2025★ 2 cited

The population of hyperluminous X-ray sources as seen by XMM-Newton

Roberta Amato, Erwan Quintin, Hugo Tranin +7

Ultraluminous and hyperluminous X-ray sources (ULXs and HLXs) are among the brightest astrophysical objects in the X-ray sky. While ULXs most likely host stellar-mass compact objec…

astro-ph.HE2023★ 6 cited

The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources

Matteo Bachetti, Matthew J. Middleton, Ciro Pinto +25

Ultraluminous X-ray sources (ULXs) represent an extreme class of accreting compact objects: from the identification of some of the accretors as neutron stars to the detection of po…

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.HE2016★ 1 cited

Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)

The CTA Consortium, :, A. Abchiche +1387

List of contributions from the Cherenkov Telescope Array (CTA) Consortium presented at the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016), July 11-15,…

astro-ph.HE2014★ 22 cited

Pulse Phase-coherent Timing and Spectroscopy of CXOU J164710.2-45521 Outbursts

Guillermo A. Rodríguez Castillo, Gian Luca Israel, Paolo Esposito +5

We present a long-term phase-coherent timing analysis and pulse-phase resolved spectroscopy for the two outbursts observed from the transient anomalous X-ray pulsar CXOU J164710.2-…

astro-ph.HE2013★ 41 cited

Quiescent state and outburst evolution of SGR 0501+4516

A. Camero, A. Papitto, N. Rea +9

We report on the quiescent state of the Soft Gamma Repeater SGR 0501+4516 observed by XMM-Newton on 2009 August 30. The source exhibits an absorbed flux ~75 times lower than that m…