output
20082026
most citedDark Matter Search Results from a One TonneYear Exposure of XENON1T

1.8k citations

Showing 2014Show all

16 papers · 1 filter

astro-ph.HE2014★ 17 cited

Investigating Variability of Quiescent Neutron Stars in the Globular Clusters NGC 6440 and Terzan 5

A. R. Walsh, E. M. Cackett, F. Bernardini

The quiescent spectrum of neutron star low-mass X-ray binaries typically consists of two components - a thermal component associated with emission from the neutron star surface, an…

astro-ph.EP2014★ 46 cited

A dynamical stability study of Kepler Circumbinary Planetary systems with one planet

C. E. Chavez, N. Georgakarakos, S. Prodan +2

To date, 17 circumbinary planets have been discovered. In this paper, we focus our attention on the stability of the Kepler circumbinary planetary systems with only one planet, i.e…

astro-ph.HE2014★ 31 cited

Shell-Shocked: The Interstellar Medium Near Cygnus X-1

P. H. Sell, S. Heinz, E. Richards +6

We conduct a detailed case-study of the interstellar shell near the high-mass X-ray binary, Cygnus X-1. We present new WIYN optical spectroscopic and Chandra X-ray observations of…

math.AP2014★ 10 cited

Blow-up results for a strongly perturbed semilinear heat equation: Theoretical analysis and numerical method

Van Tien Nguyen, Hatem Zaag

We consider a blow-up solution for a strongly perturbed semilinear heat equation with Sobolev subcritical power nonlinearity. Working in the framework of similarity variables, we f…

astro-ph.SR2014★ 20 cited

Polarimetric and spectroscopic optical observations of the ultra-compact X-ray binary 4U 0614+091

M. C. Baglio, D. Mainetti, P. D'Avanzo +4

Aims: We present a polarimetric and spectroscopic study of the persistent ultra compact X-ray binary 4U 0614+091 aimed at searching for the emission of a relativistic particle jet…

astro-ph.GA2014★ 102 cited

P-MaNGA: Emission Lines Properties - Gas Ionisation and Chemical Abundances from Prototype Observations

F. Belfiore, R. Maiolino, K. Bundy +27

MaNGA (Mapping Nearby Galaxies at Apache Point Observatory) is a SDSS-IV survey that will obtain spatially resolved spectroscopy from 3600 Å to 10300 Å for a representative sample…