activity
20022011
most citedSwift and infra-red observations of the blazar 3C~454.3 during the giant X-ray flare of May 2005

117 citations · 1.2k across the 29 of their papers we have counts for

collaborators
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8 papers · 1 filter

astro-ph.HE2011

The Swift Supergiant Fast X-ray Transients Project: recent results

P. Romano, S. Vercellone, V. La Parola +8

We present an overview of our Supergiant Fast X-ray Transients (SFXT) project, that started in 2007, by highlighting the unique observational contribution Swift is giving to this e…

astro-ph.HE2011

A two-year monitoring campaign of Supergiant Fast X-ray Transients with Swift

P. Romano, V. La Parola, G. Cusumano +7

Swift is the only observatory which, due to its unique fast-slewing capability and broad-band energy coverage, can detect outbursts from Supergiant Fast X-ray Transients (SFXTs) fr…

astro-ph.HE2011

Supergiant Fast X-ray Transients with Swift: catching outbursts and monitoring programs

P. Romano, J. A. Kennea, D. N. Burrows +8

Swift is shedding new light on the phenomenon of Supergiant Fast X-ray Transients (SFXTs), a recently discovered class of High-Mass X-ray Binaries, whose optical counterparts are O…

astro-ph.HE20112 cited

Swift Follow-up Observations of MAXI Discovered Galactic Transients

J. A. Kennea, P. Romano, V. Mangano +5

We describe the results of the first year of a program to localize new Galactic Transient sources discovered by MAXI with NASA's Swift mission. Swift is ideally suited for follow-u…

astro-ph.HE201023 cited

Confirmation of the Supergiant Fast X-ray Transient nature of AX J1841.0-0536 from Swift outburst observations

P. Romano, V. Mangano, G. Cusumano +8

Swift observed an outburst from the supergiant fast X-ray transients (SFXT) AX J1841.0-0536 on 2010 June 5, and followed it with XRT for 11 days. The X-ray light curve shows an ini…

astro-ph.HE200936 cited

Swift/XRT monitoring of the Supergiant Fast X-ray Transient IGR J18483-0311 for an entire orbital period

P. Romano, L. Sidoli, L. Ducci +9

IGR J18483-0311 is an X-ray pulsar with transient X-ray activity, belonging to the new class of High Mass X-ray Binaries called Supergiant Fast X-ray Transients. This system is one…