output
19932026
most citedThe Gaia mission

7.1k citations

Showing 2014 · astro-ph.HEShow all

26 papers · 2 filters

astro-ph.HE2014

A strong radio brightening at the jet base of M87 during the elevated very-high-energy gamma-ray state in 2012

K. Hada, M. Giroletti, M. Kino +18

The nearby radio galaxy M87 offers a unique opportunity for exploring the connection between gamma-ray production and jet formation at an unprecedented linear resolution. However,…

astro-ph.HE2014★ 1 cited

Radio investigation of Ultra-Luminous X-ray Sources in the SKA Era

Anna Wolter, Anthony P. Rushton, Mar Mezcua +5

A puzzling class of exotic objects, which have been known about for more than 30 years, is reaching a new era of understanding. We have discovered hundreds of Ultra Luminous X-ray…

astro-ph.HE2014★ 52 cited

The radio relic in Abell 2256: overall spectrum and implications for electron acceleration

M. Trasatti, H. Akamatsu, L. Lovisari +5

The galaxy cluster Abell 2256 hosts one of the most intriguing examples in the class of radio relics. It has been found that this radio relic has a rather flat integrated spectrum…

astro-ph.HE2014★ 61 cited

Gamma-ray flaring activity from the gravitationally lensed blazar PKS 1830-211 observed by Fermi LAT

The Fermi LAT Collaboration, A. A. Abdo, M. Ackermann +126

The Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope routinely detects the highly dust-absorbed, reddened, and MeV-peaked flat spectrum radio quasar PKS 1830…

astro-ph.HE2014★ 55 cited

The most powerful flaring activity from the NLSy1 PMN J0948+0022

F. D'Ammando, M. Orienti, J. Finke +73

We report on multifrequency observations performed during 2012 December-2013 August of the first narrow-line Seyfert 1 galaxy detected in gamma rays, PMN J0948+0022 ( = 0.5846).…

astro-ph.HE2014★ 75 cited

Multiwavelength observations of Mrk 501 in 2008

MAGIC Collaboration, J. Aleksić, S. Ansoldi +256

Mrk 501 is one of the brightest blazars at TeV energies and has been extensively studied since its first VHE detection in 1996. Our goal is to characterize in detail the source gam…

astro-ph.HE2014★ 823 cited

The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV

The Fermi LAT collaboration, M. Ackermann, M. Ajello +142

The γ-ray sky can be decomposed into individually detected sources, diffuse emission attributed to the interactions of Galactic cosmic rays with gas and radiation fields, and a res…

astro-ph.HE2014★ 34 cited

Very Long Baseline polarimetry and the gamma-ray connection in Markarian 421 during the broadband campaign in 2011

R. Lico, M. Giroletti, M. Orienti +16

We analyzed data in polarized intensity obtained with the Very Long Baseline Array (VLBA) at twelve epochs (one observation per month from January to December 2011) at 15, 24, and…

astro-ph.HE2014★ 27 cited

Radio-Gamma-ray connection and spectral evolution in 4C +49.22 (S4 1150+49): the Fermi, Swift and Planck view

S. Cutini, S. Ciprini, M. Orienti +23

The Large Area Telescope on board the Fermi Gamma-ray Space Telescope detected a strong gamma-ray flare on 2011 May 15 from a source identified as 4C 49.22, a flat spectrum radio q…

astro-ph.HE2014★ 25 cited

First broadband characterization and redshift determination of the VHE blazar MAGIC J2001+439

MAGIC Collaboration, J. Aleksić, S. Ansoldi +167

We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associated with the unknown-redshift blazar MG4 J200112+4352. Based on its gamma-ray spectral p…

astro-ph.HE2014★ 25 cited

Exploring the multiband emission of TXS 0536+145: the most distant gamma-ray flaring blazar

M. Orienti, F. D'Ammando, M. Giroletti +4

We report results of a multiband monitoring campaign of the flat spectrum radio quasar TXS 0536+145 at redshift 2.69. This source was detected during a very high gamma-ray activity…

astro-ph.HE2014★ 12 cited

Unusual Flaring Activity in the Blazar PKS 1424-418 during 2008-2011

S. Buson, F. Longo, S. Larsson +24

Context. Blazars are a subset of active galactic nuclei (AGN) with jets that are oriented along our line of sight. Variability and spectral energy distribution (SED) studies are cr…

astro-ph.HE2014★ 30 cited

Probing the very-high-energy gamma-ray spectral curvature in the blazar PG 1553+113 with the MAGIC telescopes

MAGIC Collaboration, J. Aleksić, S. Ansoldi +152

PG 1553+113 is a very-high-energy (VHE, ) -ray emitter classified as a BL Lac object. Its redshift is constrained by intergalactic absorption lines in the r…

astro-ph.HE2014★ 330 cited

The Spectrum and Morphology of the Fermi Bubbles

LAT Collaboration

The Fermi bubbles are two large structures in the gamma-ray sky extending to above and below the Galactic center. We analyze 50 months of Fermi Large Area Telescope data…

astro-ph.HE2014★ 75 cited

A hot cocoon in the ultralong GRB 130925A: hints of a PopIII-like progenitor in a low density wind environment

Luigi Piro, Eleonora Troja, Bruce Gendre +7

GRB 130925A is a peculiar event characterized by an extremely long gamma-ray duration (7 ks), as well as dramatic flaring in the X-rays for 20 ks. After this peri…

astro-ph.HE2014★ 33 cited

Infrared properties of blazars: putting the GASP-WEBT sources into context

C. M. Raiteri, M. Villata, M. I. Carnerero +16

The infrared properties of blazars can be studied from the statistical point of view with the help of sky surveys, like that provided by the Wide-field Infrared Survey Explorer (WI…

astro-ph.HE2014★ 61 cited

A strong radio brightening at the jet base of M87 during the elevated very-high-energy gamma-ray state in 2012

K. Hada, M. Giroletti, M. Kino +18

We report our intensive radio monitoring observations of the jet in M87 with the VLBI Exploration of Radio Astrometry (VERA) and the European VLBI Network (EVN) from February 2011…

astro-ph.HE2014★ 48 cited

Unveiling the nature of the unidentified gamma-ray sources V: analysis of the radio candidates with the kernel density estimation

F. Massaro, R. D'Abrusco, A. Paggi +5

Nearly one-third of the gamma-ray sources detected by Fermi are still unidentified, despite significant recent progress in this effort. On the other hand, all the gamma-ray extraga…

astro-ph.HE2014★ 59 cited

Unveiling the nature of the unidentified gamma-ray sources IV: the catalog of potential X-ray counterparts

A. Paggi, F. Massaro, R. D'Abrusco +5

A significant fraction ( %) of the high-energy gamma-ray sources listed in the second LAT (2FGL) catalog are still of unknown origin, being not yet associ…

astro-ph.HE2014★ 47 cited

Deep Broadband Observations of the Distant Gamma-ray Blazar PKS 1424+240

S. Archambault, T. Aune, B. Behera +149

We present deep VERITAS observations of the blazar PKS 1424+240, along with contemporaneous Fermi Large Area Telescope, Swift X-ray Telescope and Swift UV Optical Telescope data be…

astro-ph.HE2014★ 47 cited

Relativistic electrons and magnetic field of the M87 jet on ~ten Schwarzschild radii scale

M. Kino, F. Takahara, K. Hada +1

We explore energy densities of magnetic field and relativistic electrons in the M87 jet. Since the radio core at the jet base is identical to the optically thick surface against sy…

astro-ph.HE2014★ 45 cited

Multifrequency Studies of the Peculiar Quasar 4C +21.35 During the 2010 Flaring Activity

M. Ackermann, M. Ajello, A. Allafort +288

The discovery of rapidly variable Very High Energy (VHE; E > 100 GeV) gamma-ray emission from 4C +21.35 (PKS 1222+216) by MAGIC on 2010 June 17, triggered by the high activity dete…

astro-ph.HE2014★ 126 cited

Limb-Brightened Jet of 3C 84 Revealed by the 43-GHz Very-Long-Baseline-Array Observation

H. Nagai, T. Haga, G. Giovannini +8

We present a study of sub-pc scale radio structure of the radio galaxy 3C 84/NGC 1275 based on the Very Long Baseline Array (VLBA) data at 43 GHz. We discover a limb-brightening in…

astro-ph.HE2014★ 55 cited

Fermi-LAT Detection of Gravitational Lens Delayed Gamma-ray Flares from Blazar B0218+357

C. C. Cheung, S. Larsson, J. D. Scargle +23

Using data from the Fermi Large Area Telescope (LAT), we report the first clear gamma-ray measurement of a delay between flares from the gravitationally lensed images of a blazar.…