activity
19952026
most citedFermi Large Area Telescope Second Source Catalog

1.3k citations · 30.6k across the 387 of their papers we have counts for

collaborators
Showing 2012Show all

28 papers · 1 filter

astro-ph.HE2012★ 34 cited

An energy-conserving, particle dominated, time-dependent model of 3C58 and its observability at high-energies

Diego F. Torres, Analia N. Cillis, Jonatan Martin Rodriguez

We present a time-dependent spectral model of the nebula 3C58 and compare it with available data. The model is for a leptonic nebula, in which particles are subject to synchrotron,…

astro-ph.HE2012

Extended X-ray emission around RRAT J1819-1458

A. Camero-Arranz, N. Rea, M. A. McLaughlin +9

We present new imaging and spectral analysis of the recently discovered extended X-ray emission around the high-magnetic-field rotating radio transient RRAT J1819-1458. We used two…

astro-ph.HE2012★ 13 cited

The extended X-ray emission around RRAT J1819-1458

A. Camero-Arranz, N. Rea, N. Bucciantini +9

We present new imaging and spectral analysis of the recently discovered extended X-ray emission around the high magnetic field rotating radio transient RRAT J1819-1458. We used two…

astro-ph.HE2012★ 16 cited

Observations of the magnetars 4U 0142+61 and 1E 2259+586 with the MAGIC telescopes

The MAGIC Collaboration, J. Aleksić, L. A. Antonelli +153

Magnetars are an extreme, highly magnetized class of isolated neutron stars whose large X-ray luminosity is believed to be driven by their high magnetic field. In this work we stud…

astro-ph.CO2012★ 273 cited

The Imprint of The Extragalactic Background Light in the Gamma-Ray Spectra of Blazars

LAT Collaboration

The light emitted by stars and accreting compact objects through the history of the Universe is encoded in the intensity of the extragalactic background light (EBL). Knowledge of t…

astro-ph.HE2012★ 39 cited

The Simultaneous Low State Spectral Energy Distribution of 1ES 2344+514 from Radio to Very High Energies

MAGIC Collaboration, J. Aleksić, L. A. Antonelli +191

[Abridged] Context. To construct and interpret the spectral energy distribution (SED) of BL Lacertae objects, simultaneous broad-band observations are mandatory. Aims. We present t…

astro-ph.HE2012

Unveiling the super-orbital modulation of LSI +61 303 in X-rays

Jian Li, Diego F. Torres, Shu Zhang +5

We found evidence for the super-orbital modulation in the X-ray emission of LS I +61 303 from the longest monitoring date by the RXTE. The time evolution of the modulated fraction…

astro-ph.HE2012★ 11 cited

INTEGRAL and Swift observations of the Be X-ray binary 4U 1036-56 (RX J1037.5-5647) and its possible relation with gamma-ray transients

Jian Li, Diego F. Torres, Shu Zhang +3

We present timing, spectral, and long-term temporal analysis of the high mass X-ray binary (HMXB) 4U 1036-56 using INTEGRAL and Swift observations. We show that it is a weak hard X…

astro-ph.HE2012★ 13 cited

Impact of the orbital uncertainties on the timing of pulsars in binary systems

G. Andrea Caliandro, Diego F. Torres, Nanda Rea

The detection of pulsations from an X-ray binary is an unambiguous signature of the presence of a neutron star in the system. When the pulsations are missed in the radio band, thei…

astro-ph.IM2012★ 43 cited

LOFT: the Large Observatory For X-ray Timing

M. Feroci, J. W. den Herder, E. Bozzo +245

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is curren…

astro-ph.HE2012★ 117 cited

Time-dependent modeling of pulsar wind nebulae: Study on the impact of the diffusion-loss approximations

Jonatan Martin, Diego F. Torres, Nanda Rea

In this work, we present a leptonic, time-dependent model of pulsar wind nebulae (PWNe). The model seeks a solution for the lepton distribution function considering the full time-e…

astro-ph.HE2012★ 8 cited

INTEGRAL and Swift/XRT observations on IGR J18179-1621

J. Li, S. Zhang, D. F. Torres +3

IGR J18179-1621 is a hard X-ray binary transient discovered recently by INTEGRAL. Here we report on detailed timing and spectral analysis on IGR J18179-1621 in X-rays based on avai…

astro-ph.HE2012★ 65 cited

Multi-wavelength observations of blazar AO 0235+164 in the 2008-2009 flaring state

M. Ackermann, M. Ajello, J. Ballet +208

The blazar AO 0235+164 (z = 0.94) has been one of the most active objects observed by Fermi Large Area Telescope (LAT) since its launch in Summer 2008. In addition to the continuou…

astro-ph.HE2012★ 42 cited

MAGIC observations of the giant radio galaxy M87 in a low-emission state between 2005 and 2007

MAGIC Collaboration, J. Aleksić, E. A. Alvarez +155

We present the results of a long M87 monitoring campaign in very high energy -rays with the MAGIC-I Cherenkov telescope. We aim to model the persistent non-thermal jet emission…

astro-ph.HE2012★ 47 cited

Gamma-ray observations of the Orion Molecular Clouds with the Fermi Large Area Telescope

M. Ackermann, M. Ajello, A. Allafort +142

We report on the gamma-ray observations of giant molecular clouds Orion A and B with the Large Area Telescope (LAT) on-board the Fermi Gamma-ray Space Telescope. The gamma-ray emis…

astro-ph.HE2012★ 394 cited

GeV Observations of Star-forming Galaxies with \textit{Fermi} LAT

Fermi LAT Collaboration, M. Ackermann, M. Ajello +127

Recent detections of the starburst galaxies M82 and NGC 253 by gamma-ray telescopes suggest that galaxies rapidly forming massive stars are more luminous at gamma-ray energies comp…

astro-ph.HE2012★ 239 cited

Fermi LAT Search for Dark Matter in Gamma-ray Lines and the Inclusive Photon Spectrum

LAT Collaboration, M. Ackermann, M. Ajello +117

Dark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-r…

astro-ph.HE2012★ 98 cited

Fermi-LAT Discovery of GeV Gamma-ray Emission from the Vicinity of SNR W44

Yasunobu Uchiyama, Stefan Funk, Hideaki Katagiri +5

We report the detection of GeV gamma-ray emission from the molecular cloud complex that surrounds the supernova remnant (SNR) W44 using the Large Area Telescope (LAT) onboard Fermi…

astro-ph.HE2012★ 27 cited

Detection of VHE γ-rays from HESS J0632+057 during the 2011 February X-ray outburst with the MAGIC Telescopes

The MAGIC Collaboration, J. Aleksić, E. A. Alvarez +158

The very high energy (VHE) γ-ray source HESS J0632+057 has recently been confirmed to be a γ-ray binary. The optical counterpart is the Be star MWC 148, and a compact object of unk…

astro-ph.HE2012★ 18 cited

Building up the spectrum of cosmic-rays in star-forming regions

Diego F. Torres, Analia Cillis, Brian Lacki +1

The common approach to compute the cosmic-ray distribution in an starburst galaxy or region is equivalent to assume that at any point within that environment, there is an accelerat…

astro-ph.HE2012★ 67 cited

Discovery of VHE gamma-rays from the blazar 1ES 1215+303 with the MAGIC Telescopes and simultaneous multi-wavelength observations

MAGIC Collaboration, J. Aleksić, E. A. Alvarez +164

Context. We present the discovery of very high energy (VHE, E > 100GeV) gamma-ray emission from the BL Lac object 1ES 1215+303 by the MAGIC telescopes and simultaneous multi-wavele…

astro-ph.GA2012★ 75 cited

The fundamental plane for radio magnetars

Nanda Rea, Jose' A. Pons, Diego F. Torres +1

High magnetic fields are a distinguishing feature of neutron stars and the existence of sources (the soft gamma repeaters and the anomalous X-ray pulsars) hosting an ultra-magnetiz…

astro-ph.HE2012★ 99 cited

Periodic Emission from the Gamma-ray Binary 1FGL J1018.6-5856

The Fermi LAT Collaboration, M. J. Coe, F. Di Mille +5

Gamma-ray binaries are stellar systems containing a neutron star or black hole with gamma-ray emission produced by an interaction between the components. These systems are rare, ev…

astro-ph.HE2012★ 89 cited

Morphological and spectral properties of the W51 region measured with the MAGIC telescopes

MAGIC Collaboration, J. Aleksić, E. A. Alvarez +157

The W51 complex hosts the supernova remnant W51C which is known to interact with the molecular clouds in the star forming region W51B. In addition, a possible pulsar wind nebula CX…