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19932020
most citedHabitable Zones Around Main-Sequence Stars: New Estimates

1.6k citations

Showing 2013Show all

57 papers · 1 filter

nucl-ex2013★ 47 cited

High-spin structures of 124-131Te: Competition of proton and neutron pair breakings

A. Astier, M. -G. Porquet, Ts. Venkova +13

The 124-131Te nuclei have been produced as fission fragments in two fusion reactions induced by heavy-ions (12C + 238U at 90 MeV bombarding energy and 18O + 208Pb at 85 MeV) and st…

astro-ph.SR2013★ 24 cited

A new procedure for defining a homogenous line-list for solar-type stars

S. G. Sousa, N. C. Santos, V. Adibekyan +9

Context. The homogenization of the stellar parameters is an important goal for large observational spectroscopic surveys, but it is very difficult to achieve it because of the dive…

math.CO2013★ 1 cited

Quasi-symmetric functions as polynomial functions on Young diagrams

Jean-Christophe Aval, Valentin Féray, Jean-Christophe Novelli +1

We determine the most general form of a smooth function on Young diagrams, that is, a polynomial in the interlacing or multirectangular coordinates whose value depends only on the…

astro-ph.GA2013★ 230 cited

The ATLASGAL survey: a catalog of dust condensations in the Galactic plane

T. Csengeri, J. S. Urquhart, F. Schuller +10

The formation processes and the evolutionary stages of high-mass stars are poorly understood compared to low-mass stars. Large-scale surveys are needed to provide an unbiased censu…

astro-ph.HE2013★ 50 cited

Long-term TeV and X-ray Observations of the Gamma-ray Binary HESS J0632+057

VERITAS Collaboration, E. Aliu, S. Archambault +297

HESS J0632+057 is the only gamma-ray binary known so far whose position in the sky allows observations with ground-based observatories both in the northern and southern hemispheres…

physics.optics2013★ 131 cited

Spectral purity transfer between optical wavelengths at the level

Daniele Nicolodi, Béengère Argence, Wei Zhang +3

Ultra-stable lasers and optical frequency combs have been the enabling technologies for the tremendous progress of precise optical spectroscopy in the last ten years. To improve la…

astro-ph.HE2013★ 165 cited

Constraints on axionlike particles with H.E.S.S. from the irregularity of the PKS 2155-304 energy spectrum

H. E. S. S. Collaboration, A. Abramowski, F. Acero +211

Axionlike particles (ALPs) are hypothetical light (sub-eV) bosons predicted in some extensions of the Standard Model of particle physics. In astrophysical environments comprising h…

astro-ph.GA2013★ 115 cited

On the metallicity of open clusters II. Spectroscopy

U. Heiter, C. Soubiran, M. Netopil +1

In a series of three papers, we investigate the current status of published metallicities for open clusters that were derived from a variety of photometric and spectroscopic method…

astro-ph.HE2013★ 33 cited

Fermi LAT and WMAP observations of the supernova remnant HB 21

G. Pivato, J. Hewitt, L. Tibaldo +8

We present the analysis of Fermi Large Area Telescope (LAT) -ray observations of HB~21 (G89.0+4.7). We detect significant -ray emission associated with the remnant: the flux…

astro-ph.HE2013★ 54 cited

H.E.S.S. Observations of the Crab during its March 2013 GeV Gamma-Ray Flare

H. E. S. S. Collaboration, A. Abramowski, F. Aharonian +217

Context. On March 4, 2013, the Fermi-LAT and AGILE reported a flare from the direction of the Crab Nebula in which the high-energy (HE; E > 100 MeV) flux was six times above its qu…

cond-mat.stat-mech2013★ 12 cited

Fluctuation of gauge field for general nonlinear Fokker-Planck equation and covariant version of Fisher information matrix

Takuya Yamano

We clarify a strong link between general nonlinear Fokker-Planck equations with gauge fields associated with nonequilibrium dynamics and the Fisher information of the system. The n…

math.GT2013★ 5 cited

GL^+(2,R)-orbits in Prym eigenform loci

Erwan Lanneau, Duc-Manh Nguyen

This paper is devoted to the classification of GL^+(2,R)-orbit closures of surfaces in the intersection of the Prym eigenform locus with various strata of quadratic differentials.…

astro-ph.HE2013★ 15 cited

HESS J1818-154, a new composite supernova remnant discovered in TeV gamma rays and X-rays

H. E. S. S. Collaboration, A. Abramowski, F. Aharonian +217

Composite supernova remnants (SNRs) constitute a small subclass of the remnants of massive stellar explosions where non-thermal radiation is observed from both the expanding shell-…

math.OA2013★ 4 cited

Maximal amenable subalgebras of von Neumann algebras associated with hyperbolic groups

Rémi Boutonnet, Alessandro Carderi

We prove that for any infinite, maximal amenable subgroup in a hyperbolic group , the von Neumann subalgebra is maximal amenable inside . It provides many new, expl…

math.NT2013

Fourier coefficients of GL(N) automorphic forms in arithmetic progressions

Emmanuel Kowalski, Guillaume Ricotta

We show that the multiple divisor functions of integers in invertible residue classes modulo a prime number, as well as the Fourier coefficients of GL(N) Maass cusp forms for all N…

cond-mat.soft2013★ 11 cited

Light-induced pitch transitions in photosensitive cholesteric liquid crystals: Effects of anchoring energy

Tetiana N. Orlova, Roman I. Iegorov, Alexei D. Kiselev

We experimentally study how the cholesteric pitch, , depends on the equilibrium one, , in planar liquid crystal (LC) cells with both strong and semistrong anchoring conditi…

cond-mat.quant-gas2013★ 48 cited

Thermodynamics and magnetic properties of the anisotropic 3D Hubbard model

Jakub Imriška, Mauro Iazzi, Lei Wang +7

We study the 3D Hubbard model with anisotropic nearest neighbor tunneling amplitudes using the dynamical cluster approximation and compare the results with a quantum simulation exp…

astro-ph.HE2013★ 79 cited

Determination of the Point-Spread Function for the Fermi Large Area Telescope from On-orbit Data and Limits on Pair Halos of Active Galactic Nuclei

LAT Collaboration

The Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope is a pair-conversion telescope designed to detect photons with energies from 20 MeV to > 300 GeV. The pre-laun…

math.DS2013★ 4 cited

A thermodynamic formalism for continuous time Markov chains with values on the Bernoulli Space: entropy, pressure and large deviations

Artur O. Lopes, Adriana Neumann, Philippe Thieullen

Through this paper we analyze the ergodic properties of continuous time Markov chains with values on the one-dimensional spin lattice 1,...,d}^N (also known as the Bernoulli space)…

astro-ph.HE2013★ 56 cited

The Vela-X Pulsar Wind Nebula revisited with 4 years of Fermi-Large Area Telescope observations

M. -H. Grondin, R. W. Romani, M. Lemoine-Goumard +3

The Vela supernova remnant is the closest supernova remnant to Earth containing an active pulsar, the Vela pulsar (PSR B0833-45). This pulsar is the archetype of the middle-aged pu…

astro-ph.HE2013★ 15 cited

Evidence of a Hadronic Origin for the TeV Source J1834-087

D. A. Frail, M. J. Claussen, J. Mehault

We report on the discovery of compact, narrow OH line emission from the hydroxl molecule at 1720 MHz toward the extended TeV source J1834-087. The origin of this high energy emissi…

astro-ph.HE2013★ 66 cited

Constraining the location of rapid gamma-ray flares in the FSRQ 3C 273

B. Rani, B. Lott, T. P. Krichbaum +2

We present a γ-ray photon flux and spectral variability study of the flat-spectrum radio quasar 3C 273 over a rapid flaring activity period between September 2009 to April 2010. Fi…

astro-ph.HE2013★ 125 cited

Constraints on the Galactic Population of TEV Pulsar Wind Nebulae Using Fermi Large Area Telescope Observations

F. Acero, M. Ackermann, M. Ajello +155

Pulsar wind nebulae (PWNe) have been established as the most populous class of TeV gamma-ray emitters. Since launch, the Fermi Large Area Telescope (LAT)identified five high-energy…

cond-mat.soft2013★ 69 cited

Nematic droplets in aqueous dispersions of carbon nanotubes

Nicolas Puech, Eric Grelet, Philippe Poulin +2

Aqueous dispersions of exfoliated, bile-salt stabilized single-wall carbon nanotubes exhibit a first order transition to a nematic liquid-crystalline phase. The nematic phase prese…