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19932026
most citedThe Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

4.1k citations

Showing 2018 · astro-ph.HEShow all

29 papers · 2 filters

astro-ph.HE2018★ 14 cited

Thermal emission and magnetic beaming in the radio and X-ray mode-switching PSR B0943+10

Michela Rigoselli, Sandro Mereghetti, Roberto Turolla +3

PSR B0943+10 is a mode-switching radio pulsar characterized by two emission modes with different radio and X-ray properties. Previous studies, based on simple combinations of black…

astro-ph.HE2018★ 34 cited

Physics and astrophysics of strong magnetic field systems with eXTP

Andrea Santangelo, Silvia Zane, Hua Feng +38

In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies of strongly magnetized objects. We will focus on the physics…

astro-ph.HE2018★ 72 cited

Observatory science with eXTP

Jean J. M. in 't Zand, Enrico Bozzo, Jinlu Qu +181

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring s…

astro-ph.HE2018★ 1 cited

On the origin of supergiant fast X-ray transients

Swetlana Hubrig, Lara Sidoli, Konstantin A. Postnov +3

A fraction of high-mass X-ray binaries are supergiant fast X-ray transients. These systems have on average low X-ray luminosities, but display short flares during which their X-ray…

astro-ph.HE2018★ 173 cited

A -ray determination of the Universe's star-formation history

LAT Collaboration, M. Ajello, K. Helgason +4

The light emitted by all galaxies over the history of the Universe produces the extragalactic background light (EBL) at ultraviolet, optical, and infrared wavelengths. The EBL is a…

astro-ph.HE2018★ 37 cited

Unresolved Gamma-Ray Sky through its Angular Power Spectrum

M. Ackermann, M. Ajello, L. Baldini +107

The gamma-ray sky has been observed with unprecedented accuracy in the last decade by the Fermi large area telescope (LAT), allowing us to resolve and understand the high-energy Un…

astro-ph.HE2018★ 5 cited

The High Mass X-ray Binaries in star-forming galaxies

M. Celeste Artale, Nicola Giacobbo, Michela Mapelli +1

The high mass X-ray binaries (HMXBs) provide an exciting framework to investigate the evolution of massive stars and the processes behind binary evolution. HMXBs have shown to be g…

astro-ph.HE2018★ 267 cited

An embedded X-ray source shines through the aspherical AT2018cow: revealing the inner workings of the most luminous fast-evolving optical transients

Raffaella Margutti, B. D. Metzger, R. Chornock +41

We present the first extensive radio to gamma-ray observations of a fast-rising blue optical transient (FBOT), AT2018cow, over its first ~100 days. AT2018cow rose over a few days t…

astro-ph.HE2018★ 4 cited

Spectral analysis of SXP59.0 during its 2017 outburst and properties of the soft excess in X-ray binary pulsars

N. La Palombara, P. Esposito, F. Pintore +3

We report the results provided by the XMM-Newton observation of the X-ray binary pulsar SXP59.0 during its most recent outburst in April 2017. The source was detected at $f_{\rm X}…

astro-ph.HE2018★ 108 cited

LOFAR discovery of a 23.5-second radio pulsar

C. M. Tan, C. G. Bassa, S. Cooper +16

We present the discovery of PSR J0250+5854, a radio pulsar with a spin period of 23.5 s. This is the slowest-spinning radio pulsar known. PSR J0250+5854 was discovered by the LOFAR…

astro-ph.HE2018★ 64 cited

An INTEGRAL overview of High Mass X-ray Binaries: classes or transitions?

Lara Sidoli, Adamantia Paizis

We analyzed in a systematic way the public INTEGRAL observations spanning from December 2002 to September 2016, to investigate the hard X-ray properties of about 60 High Mass X-ray…

astro-ph.HE2018★ 15 cited

The first ultraviolet detection of the Large Magellanic Cloud pulsar PSR B0540-69 and its multi-wavelength properties

R. P. Mignani, A. Shearer, A. de Luca +9

We observed the young ( yrs) pulsar PSR B0540-69 in the near-ultraviolet (UV) for the first time with the Space Telescope Imaging Spectrograph (STIS) aboard the {\em Hub…

astro-ph.HE2018★ 5 cited

Discovery of X-rays from the old and faint pulsar J1154--6250

Andrei P. Igoshev, Sergey S. Tsygankov, Michela Rigoselli +4

We report on the first X-ray observation of the 0.28 s isolated radio pulsar PSR J1154--6250 obtained with the XMM-Newton observatory in February 2018. A point-like source is firml…

astro-ph.HE2018★ 39 cited

VERITAS and Fermi-LAT observations of new HAWC sources

VERITAS Collaboration, A. U. Abeysekara, A. Archer +280

The HAWC (High Altitude Water Cherenkov) collaboration recently published their 2HWC catalog, listing 39 very high energy (VHE; >100~GeV) gamma-ray sources based on 507 days of obs…

astro-ph.HE2018★ 24 cited

SWIFT J1756.9-2508: spectral and timing properties of its 2018 outburst

A. Sanna, F. Pintore, A. Riggio +8

We discuss the spectral and timing properties of the accreting millisecond X-ray pulsar SWIFT J1756.9-2508 observed by XMM-Newton, NICER and NuSTAR during the X-ray outburst occurr…

astro-ph.HE2018★ 3 cited

The first orbital period of a very bright and fast Nova in M31: M31N 2013-01b

Martino Marelli, Domitilla De Martino, Sandro Mereghetti +5

We present the first X-ray and UV/optical observations of a very bright and fast nova in the disc of M31, M31N 2013-01b. The nova reached a peak magnitude 15 mag and decayed…

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.HE2018★ 395 cited

Compact radio emission indicates a structured jet was produced by a binary neutron star merger

G. Ghirlanda, O. S. Salafia, Z. Paragi +33

The binary neutron star merger event GW170817 was detected through both electromagnetic radiation and gravitational waves. Its afterglow emission may have been produced by either a…

astro-ph.HE2018★ 8 cited

A faint outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021 in NGC 6440

F. Pintore, A. Sanna, A. Riggio +6

SAX J1748.9-2021 is an accreting X-ray millisecond pulsar observed in outburst five times since its discovery in 1998. In early October 2017, the source started its sixth outburst,…

astro-ph.HE2018★ 4 cited

EXTraS discovery of a peculiar flaring X-ray source in the Galactic globular cluster NGC 6540

Sandro Mereghetti, Andrea De Luca, David Salvetti +7

We report the discovery of a flaring X-ray source in the globular cluster NGC 6540, obtained during the EXTraS project devoted to a systematic search for variability in archival da…

astro-ph.HE2018★ 15 cited

Gazing at the ultra-slow magnetar in RCW 103 with NuSTAR and Swift

A. Borghese, F. Coti Zelati, P. Esposito +6

We report on a new NuSTAR observation and on the ongoing Swift XRT monitoring campaign of the peculiar source 1E 161348-5055, located at the centre of the supernova remnant RCW 103…

astro-ph.HE2018★ 5 cited

Discovery of 3 s pulsations from the Brightest Hard X-ray Source in M31

Guillermo A. Rodríguez Castillo, Gian Luca Israel, Paolo Esposito +4

We report the discovery with XMM-Newton of 3-s X-ray pulsations from 3XMM J004232.1+411314, a dipping source that dominates the hard X-ray emission of M31. This finding unambiguous…

astro-ph.HE2018★ 4 cited

Observations of one young and three middle-aged -ray pulsars with the Gran Telescopio Canarias

R. P. Mignani, V. Testa, N. Rea +4

We used the 10.4m Gran Telescopio Canarias to search for the optical counterparts to four isolated -ray pulsars, all detected in the X-rays by either \xmm\ or \chan\ but not yet…

astro-ph.HE2018★ 176 cited

Search for Spatial Extension in High-Latitude Sources Detected by the Fermi Large Area Telescope

LAT Collaboration, Jonathan Biteau

We present a search for spatial extension in high-latitude () sources in recent Fermi point source catalogs. The result is the Fermi High-Latitude Extended Sources Cat…