2.7k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- G. Cusumano2 profiles86 · h 43
- P. Romano3 profiles80 · h 49
- A. Segreto52 · h 55
- V. Mangano3 profiles39 · h 68
- T. Mineo4 profiles37 · h 21
- S. Campana3 profiles36 · h 62
- V. La Parola2 profiles34 · h 12
- F. Frontera2 profiles33 · h 52
- D. Burrows2 profiles31 · h 57
- G. Chincarini2 profiles31 · h 59
- G. Tagliaferri2 profiles30 · h 78
- N. Gehrels2 profiles29 · h 120
- National Institute for AstrophysicsIT232 papers
- Pennsylvania State UniversityUS153 papers
- Brera Astronomical ObservatoryIT149 papers
- Centre National de la Recherche ScientifiqueFR129 papers
- Goddard Space Flight CenterUS112 papers
- Astronomical Observatory of RomeIT105 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di TorinoIT99 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT97 papers
- University of PalermoIT96 papers
- University of Rome Tor VergataIT94 papers
- University of TurinIT93 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di CataniaIT87 papers
17 papers · 2 filters
Fermi-LAT Observations of the Gamma-ray Burst GRB 130427A
LAT collaboration, GBM collaboration
The observations of the exceptionally bright gamma-ray burst (GRB) 130427A by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope provide constraints on the nature…
GRB 130427A: a Nearby Ordinary Monster
A. Maselli, A. Melandri, L. Nava +63
Long-duration Gamma-Ray Bursts (GRBs) are an extremely rare outcome of the collapse of massive stars, and are typically found in the distant Universe. Because of its intrinsic lumi…
Spectral and temporal properties of the supergiant fast X-ray transient IGR J18483-0311 observed by INTEGRAL
L. Ducci, V. Doroshenko, M. Sasaki +4
IGR J18483-0311 is a supergiant fast X-ray transient whose compact object is located in a wide (18.5 d) and eccentric (e~0.4) orbit, which shows sporadic outbursts that reach X-ray…
Broadband monitoring tracing the evolution of the jet and disk in the black hole candidate X-ray binary MAXI J1659-152
A. J. van der Horst, P. A. Curran, J. C. A. Miller-Jones +31
MAXI J1659-152 was discovered on 2010 September 25 as a new X-ray transient, initially identified as a gamma-ray burst, but was later shown to be a new X-ray binary with a black ho…
The Swift/BAT Hard X-ray Transient Monitor
Hans A. Krimm, Stephen T. Holland, Robin H. D. Corbet +14
The Swift/Burst Alert Telescope (BAT) hard X-ray transient monitor provides near real-time coverage of the X-ray sky in the energy range 15-50 keV. The BAT observes 88% of the sky…
An active state of the BL Lac Object Markarian 421 detected by INTEGRAL in April 2013
E. Pian, M. Tuerler, M. Fiocchi +22
Multiwavelength variability of blazars offers indirect insight into their powerful engines and on the mechanisms through which energy is propagated from the centre down the jet. Th…
Swift/XRT orbital monitoring of the candidate supergiant fast X-ray transient IGR J17354-3255
L. Ducci, P. Romano, P. Esposito +5
We report on the Swift/X-ray Telescope (XRT) monitoring of the field of view around the candidate supergiant fast X-ray transient (SFXT) IGR J17354-3255, which is positionally asso…
XMM-Newton and Swift observations of XTE J1743-363
E. Bozzo, P. Romano, C. Ferrigno +5
XTEJ1743-363 is a poorly known hard X-ray transient, that displays short and intense flares similar to those observed from Supergiant Fast X-ray Transients. The probable optical co…
An evaluation of the exposure in nadir observation of the JEM-EUSO mission
J. H. Adams, S. Ahmad, J. -N. Albert +258
We evaluate the exposure during nadir observations with JEM-EUSO, the Extreme Universe Space Observatory, on-board the Japanese Experiment Module of the International Space Station…
Swift Observations of the High-mass X-ray Binary IGR J16283-4838 unveil a 288-day Orbital Period
G. Cusumano, A. Segreto, V. La Parola +3
We report on the temporal and spectral properties of the HMXB IGR J16283-4838 in the hard X-ray band. We searched the first 88 months of Swift BAT survey data for long-term periodi…
Swift-BAT hard X-ray sky monitoring unveils the orbital period of the HMXB IGR J18219-1347
V. La Parola, G. Cusumano, A. Segreto +3
IGR J18219-1347 is a hard X-ray source discovered by INTEGRAL in 2010. We have analyzed the X-ray emission of this source exploiting the BAT survey data up to March 2012 and the XR…
Swift discovery of the orbital period of the HMXB IGR J015712-7259 in the Small Magellanic Cloud
A. Segreto, G. Cusumano, V. La Parola +3
In the last years the hard X-ray astronomy has made a significant step forward, thanks to the monitoring of the IBIS/ISGRI telescope on board the INTEGRAL satellite and of the Burs…
Swings between rotation and accretion power in a millisecond binary pulsar
A. Papitto, C. Ferrigno, E. Bozzo +20
It is thought that neutron stars in low-mass binary systems can accrete matter and angular momentum from the companion star and be spun-up to millisecond rotational periods. During…
The 54 days orbital period of AX J1820.5-1434 unveiled by Swift
A. Segreto, V. La Parola, G. Cusumano +3
The hard X-ray survey that Swift-BAT has been performing since late 2004 has provided a considerable database for a large number of sources whose hard X-ray emission was poorly kno…
Finding a 61.0-day orbital period for the HMXB 4U 1036-56 with the Swift-BAT monitoring
G. Cusumano, A. Segreto, V. La Parola +3
Since November 2004, the Burst Alert Telescope on board Swift is producing a monitoring of the entire sky in the 15-150 keV band, recording the timing and spectral behavior of the…
Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
Pierre Auger Collaboration
The observation of ultrahigh energy (UHE) neutrinos has become a priority in experimental astroparticle physics. UHE neutrinos can be detected with a variety of techniques. In part…
Observation of TeV gamma-rays from the unidentified source HESS J1841-055 with the ARGO-YBJ experiment
YBJ Collaboration, B. Bartoli, P. Bernardini +100
We report the observation of a very high energy γ-ray source, whose position is coincident with HESS J1841-055. This source has been observed for 4.5 years by the ARGO-YBJ experime…