output
19932026
most citedThe Gaia mission

7.1k citations

Showing 2014Show all

69 papers · 1 filter

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.IM2014

The SKA Mid-frequency All-sky Continuum Survey: Discovering the unexpected and transforming radio-astronomy

Ray P. Norris, Kaustuv Basu, Michael Brown +5

We show that, in addition to specific science goals, there is a strong case for conducting an all-sky (i.e. the visible 3-pi steradians) SKA continuum survey which does not fit nea…

astro-ph.GA2014

Identifying the first generation of radio powerful AGN in the Universe with the SKA

Jose Afonso, Jordi Casanellas, Isabella Prandoni +4

One of the most challenging and exciting subjects in modern astrophysics is that of galaxy formation at the epoch of reionisation. The SKA, with its revolutionary capabilities in t…

astro-ph.GA2014★ 3 cited

The physics of the radio emission in the quiet side of the AGN population with the SKA

M. Orienti, F. D'Ammando, M. Giroletti +2

Despite targets of many multiwavelength campaigns, the main physical processes at work in AGN are still under debate. In particular the origin of the radio emission and the mechani…

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.GA2014★ 9 cited

Molecular gas and nuclear activity in early-type galaxies: any link with radio-loudness?

Ranieri D. Baldi, Marcello Giroletti, Alessandro Capetti +4

Aims. We want to study the amount of molecular gas in a sample of nearby early-type galaxies (ETGs) which host low-luminosity Active Galactic Nuclei (AGN). We look for possible dif…

astro-ph.GA2014★ 25 cited

New insights from deep VLA data on the potentially recoiling black hole CID-42 in the COSMOS field

Mladen Novak, Vernesa Smolcic, Francesca Civano +12

We present deep 3 GHz VLA observations of the potentially recoiling black hole CID-42 in the COSMOS field. This galaxy shows two optical nuclei in the HST/ACS image and a large vel…

astro-ph.GA2014★ 56 cited

Subarcsecond international LOFAR radio images of the M82 nucleus at 118 MHz and 154 MHz

E. Varenius, J. E. Conway, I. Martí-Vidal +25

The nuclear starburst in the nearby galaxy M82 provides an excellent laboratory for understanding the physics of star formation. This galaxy has been extensively observed in the pa…

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.GA2014★ 26 cited

Discovery of Carbon Radio Recombination Lines in M82

Leah K. Morabito, J. B. R. Oonk, Francisco Salgado +30

Carbon radio recombination lines (RRLs) at low frequencies (<=500 MHz) trace the cold, diffuse phase of the interstellar medium, which is otherwise difficult to observe. We present…

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.CO2014★ 133 cited

On the amplification of magnetic fields in cosmic filaments and galaxy clusters

F. Vazza, M. Brüggen, C. Gheller +1

The amplification of primordial magnetic fields via a small-scale turbulent dynamo during structure formation might be able to explain the observed magnetic fields in galaxy cluste…

astro-ph.SR2014★ 21 cited

Young open clusters in the galactic star forming region NGC 6357

Fabrizio Massi, Andrea Giannetti, Elisa di Carlo +3

NGC6357 is an active star forming region with very young massive open clusters (OC). These clusters contain some of the most massive stars in the Galaxy and strongly interact with…

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.GA2014★ 34 cited

LOFAR low-band antenna observations of the 3C295 and Bootes fields: source counts and ultra-steep spectrum sources

R. J. van Weeren, W. L. Williams, C. Tasse +98

We present LOFAR Low Band observations of the Bootes and 3C295 fields. Our images made at 34, 46, and 62 MHz reach noise levels of 12, 8, and 5 mJy beam, making them the dee…

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.GA2014★ 29 cited

Tentative Detection of the Nitrosylium Ion in Space

J. Cernicharo, S. Bailleux, E. Alekseev +8

We report the tentative detection in space of the nitrosylium ion, NO. The observations were performed towards the cold dense core Barnard 1-b. The identification of the NO…

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.CO2014★ 92 cited

The stripping of a galaxy group diving into the massive cluster A2142

D. Eckert, S. Molendi, M. Owers +7

Structure formation in the current Universe operates through the accretion of group-scale systems onto massive clusters. The detection and study of such accreting systems is crucia…