activity
19962026
most citedHigher Charmonia

809 citations · 28.2k across the 927 of their papers we have counts for

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Showing 2016Show all

9 papers · 1 filter

nucl-ex2016★ 36 cited

Beta-delayed gamma decay of 26P: Possible evidence of a proton halo

D. Pérez-Loureiro, C. Wrede, M. B. Bennett +23

Background: Measurements of decay provide important nuclear structure information that can be used to probe isospin asymmetries and inform nuclear astrophysics studies. Purpose…

astro-ph.GA2016★ 119 cited

Deep imaging of Eridanus II and its lone star cluster

D. Crnojević, D. J. Sand, D. Zaritsky +3

We present deep imaging of the most distant dwarf discovered by the Dark Energy Survey, Eridanus II (Eri II). Our Magellan/Megacam stellar photometry reaches mag deeper t…

astro-ph.HE2016★ 156 cited

A large light-mass component of cosmic rays at 10^{17} - 10^{17.5} eV from radio observations

S. Buitink, A. Corstanje, H. Falcke +101

Cosmic rays are the highest energy particles found in nature. Measurements of the mass composition of cosmic rays between 10^{17} eV and 10^{18} eV are essential to understand whet…

astro-ph.GA2016★ 19 cited

Globules and Pillars in Cygnus X I. Herschel Far-infrared imaging of the Cyg OB2 environment

N. Schneider, S. Bontemps, F. Motte +21

The radiative feedback of massive stars on molecular clouds creates pillars, globules and other features at the interface between the HII region and molecular cloud. We present her…

astro-ph.HE2016★ 46 cited

Chandra X-Ray Spectroscopy of the Focused Wind in the Cygnus X-1 System. II. The Nondip Spectrum in the Low/Hard State - Modulations with Orbital Phase

Ivica Miškovičová, Natalie Hell, Manfred Hanke +14

The accretion onto the black hole in the system HDE 226868/Cygnus X-1 is powered by the strong line driven stellar wind of the O-type donor star. We study the X-ray properties of t…

astro-ph.GA2016★ 29 cited

What are the megahertz peaked-spectrum sources?

Rocco Coppejans, David Cseh, Sjoert van Velzen +8

Megahertz peaked-spectrum (MPS) sources have spectra that peak at frequencies below 1 GHz in the observer's frame and are believed to be radio-loud active galactic nuclei (AGN). We…

astro-ph.SR2016★ 30 cited

Tracing jet emission at the base of a high-mass YSO. First AMBER/VLTI observations of the Brγemission in IRAS 13481-6124

A. Caratti o Garatti, B. Stecklum, G. Weigelt +9

To probe the circumstellar environment of IRAS 13481-6124, a 20 M_sun high-mass young stellar object (HMYSO) with a parsec-scale jet and accretion disc, we investigate the origin o…

astro-ph.GA2016★ 29 cited

The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering

Ben Chehade, T. Shanks, J. Findlay +10

We present a new redshift survey, the 2dF Quasar Dark Energy Survey pilot (2QDESp), which consists of quasars from deg of the southern sky, base…

astro-ph.HE2016★ 39 cited

Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations

Refiz Duro, Thomas Dauser, Victoria Grinberg +15

We report on the analysis of the broad Fe Kalpha line feature of Cygnus X-1 in the spectra of four simultaneous hard intermediate state observations made with the X-ray Multiple Mi…