output
19932026
most citedThe Gaia mission

7.1k citations

Showing 2019Show all

153 papers · 1 filter

astro-ph.GA2019★ 49 cited

NOEMA redshift measurements of bright Herschel galaxies

R. Neri, P. Cox, A. Omont +31

Using the IRAM NOrthern Extended Millimeter Array (NOEMA), we conducted a program to measure redshifts for 13 bright galaxies detected in the Herschel Astrophysical Large Area Surv…

astro-ph.GA2019★ 72 cited

The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe

Viviana Casasola, Simone Bianchi, Pieter De Vis +18

The purpose of this work is the characterization of the main scaling relations between all the ISM components (dust, atomic/molecular/total gas), gas-phase metallicity, and other g…

astro-ph.HE2019★ 7 cited

Te-REX: a sample of extragalactic TeV-emitting candidates

B. Balmaverde, A. Caccianiga, R. Della Ceca +7

The REX (Radio-Emitting X-ray sources) is a catalogue produced by cross-matching X-ray data from the ROSAT-PSPC archive of pointed observations and radio data from the NRAO VLA Sky…

astro-ph.GA2019★ 78 cited

GASP. XXII The molecular gas content of the JW100 jellyfish galaxy at z~0.05: does ram pressure promote molecular gas formation?

A. Moretti, R. Paladino, B. M. Poggianti +11

Within the GASP survey, aimed at studying the effect of the ram-pressure stripping on the star formation quenching in cluster galaxies, we analyze here ALMA observations of the jel…

astro-ph.GA2019★ 39 cited

Apparent superluminal core expansion and limb brightening in the candidate neutrino blazar TXS 0506+056

E. Ros, M. Kadler, M. Perucho +5

IceCube has reported a very-high-energy neutrino (IceCube-170922A) in a region containing the blazar TXS 0506+056. Correlated γ-ray activity has led to the first high-probability a…

astro-ph.GA2019★ 13 cited

The role of environment in galaxy evolution in the SERVS Survey I: density maps and cluster candidates

Nick Krefting, Anna Sajina, Mark Lacy +10

We use photometric redshifts derived from new -band through 4.5m Spitzer IRAC photometry in the 4.8\,deg of the XMM-LSS field to construct surface density maps in the red…

astro-ph.GA2019★ 32 cited

Cosmic evolution of star-forming galaxies to in the faint low-frequency radio source population

E. F. Ocran, A. R. Taylor, M. Vaccari +4

We study the properties of star-forming galaxies selected at 610 MHz with the GMRT in a survey covering 1.86 deg down to a noise of 7.1\,Jy / beam. These were id…

astro-ph.IM2019★ 43 cited

Wideband 67-116 GHz receiver development for ALMA Band 2

P. Yagoubov, T. Mroczkowski, V. Belitsky +43

ALMA has been operating since 2011, but has not yet been populated with the full suite of intended frequency bands. In particular, ALMA Band 2 (67-90 GHz) is the final band in the…

astro-ph.SR2019★ 14 cited

VLBI observations of the G25.65+1.05 water maser superburst

R. A. Burns, G. Orosz, O. Bayandina +23

This paper reports observations of a 22 GHz water maser `superburst' in the G25.65+1.05 massive star forming region, conducted in response to an alert from the Maser Monitoring Org…

astro-ph.CO2019★ 6 cited

How complex is the cosmic web?

F. Vazza

The growth of large-scale cosmic structure is a beautiful exemplification of how complexity can emerge in our Universe, starting from simple initial conditions and simple physical…

astro-ph.GA2019★ 38 cited

Anomalous peculiar motions of high-mass young stars in the Scutum spiral arm

K. Immer, J. Li, L. H. Quiroga-Nuñez +4

We present trigonometric parallax and proper motion measurements toward 22 GHz water and 6.7 GHz methanol masers in 16 high-mass star-forming regions. These sources are all located…

astro-ph.HE2019★ 30 cited

Investigating the multiwavelength behaviour of the flat spectrum radio quasar CTA 102 during 2013-2017

F. D'Ammando, C. M. Raiteri, M. Villata +94

We present a multiwavelength study of the flat-spectrum radio quasar CTA 102 during 2013-2017. We use radio-to-optical data obtained by the Whole Earth Blazar Telescope, 15 GHz dat…

astro-ph.HE2019★ 7 cited

East Asia VLBI Network observations of the TeV Gamma-Ray Burst 190114C

Tao An, Om Sharan Salafia, Yingkang Zhang +7

Observations of gamma-ray bursts (GRBs) at Very High Energy (VHE) offer a unique opportunity to investigate particle acceleration processes, magnetic fields and radiation fields in…

astro-ph.HE2019

Relativistic Jets in Gamma-Ray-Emitting Narrow-Line Seyfert 1 Galaxies

Filippo D'Ammando

Before the launch of the Fermi Gamma-ray Space Telescope satellite only two classes of active galactic nuclei (AGN) were known to generate relativistic jets and thus to emit up to…

astro-ph.CO2019

SZ contribution to characterize the shape of galaxy cluster haloes

S. Ettori, M. Sereno, S. Burkutean +1

We present the on-going activity to characterize the geometrical properties of the gas and dark matter haloes using multi-wavelength observations of galaxy clusters. The role of th…

astro-ph.CO2019★ 48 cited

Revived Fossil Plasma Sources in Galaxy Clusters

S. Mandal, H. T. Intema, R. J. van Weeren +10

It is well established that particle acceleration by shocks and turbulence in the intra-cluster medium can produce cluster-scale synchrotron emitting sources. However, the detailed…

astro-ph.IM2019★ 229 cited

An ultra-wide bandwidth (704 to 4032 MHz) receiver for the Parkes radio telescope

G. Hobbs, R. N. Manchester, A. Dunning +69

We describe an ultra-wide-bandwidth, low-frequency receiver ("UWL") recently installed on the Parkes radio telescope. The receiver system provides continuous frequency coverage fro…

astro-ph.GA2019★ 33 cited

The Forgotten Quadrant Survey. CO and CO (1-0) survey of the Galactic Plane in the range 220°240° -2.5°0°

M. Benedettini, S. Molinari, A. Baldeschi +12

We present the Forgotten Quadrant Survey (FQS), an ESO large project that used the 12m antenna of the Arizona Radio Observatory to map the Galactic Plane in the range 220°240°…

astro-ph.HE2019★ 33 cited

Low frequency view of GRB 190114C reveals time varying shock micro-physics

K. Misra, L. Resmi, D. A. Kann +25

We present radio and optical afterglow observations of the TeV-bright long Gamma Ray Burst (GRB) 190114C at a redshift of , which was detected by the MAGIC telescope. Our…

astro-ph.HE2019★ 60 cited

New mysteries and challenges from the Toothbrush relic: wideband observations from 550 MHz to 8 GHz

K. Rajpurohit, M. Hoeft, F. Vazza +10

Radio relics are diffuse extended synchrotron sources that originate from shock fronts induced by galaxy cluster mergers. The actual particle acceleration mechanism at the shock fr…

astro-ph.HE2019★ 58 cited

New hard-TeV extreme blazars detected with the MAGIC telescopes

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +175

Extreme high-frequency peaked BL Lac objects (EHBLs) are blazars which exhibit extremely energetic synchrotron emission. They also feature non-thermal gamma-ray emission whose peak…

astro-ph.HE2019★ 10 cited

Bright gamma-ray flares observed in GRB131108A

Donggeun Tak, Z. Lucas Uhm, Bing Zhang

GRB 131108A is a bright long Gamma-Ray Burst (GRB) detected by the Large Area Telescope and the Gamma-ray Burst Monitor on board the Fermi Gamma-ray Space Telescope. Dedicated temp…

astro-ph.GA2019★ 26 cited

The 3D structure of CO depletion in high-mass prestellar regions

S. Bovino, S. Ferrada-Chamorro, A. Lupi +3

Disentangling the different stages of the star-formation process, in particular in the high-mass regime, is a challenge in astrophysics. Chemical clocks could help alleviating this…

astro-ph.IM2019★ 78 cited

Mitigating Internal Instrument Coupling II: A Method Demonstration with the Hydrogen Epoch of Reionization Array

Nicholas S. Kern, Aaron R. Parsons, Joshua S. Dillon +63

We present a study of internal reflection and cross coupling systematics in Phase I of the Hydrogen Epoch of Reionization Array (HERA). In a companion paper, we outlined the mathem…