most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

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astro-ph.IM2017★ 11 cited

Systematic calibration error requirements for gravitational-wave detectors via the Cramér-Rao bound

Evan D. Hall, Craig Cahillane, Kiwamu Izumi +2

Gravitational-wave (GW) laser interferometers such as Advanced LIGO transduce spacetime strain into optical power fluctuation. Converting this optical power fluctuations back into…

astro-ph.SR2017★ 72 cited

Gas and dust from solar metallicity AGB stars

P. Ventura, A. Karakas, F. Dell'Agli +2

We study the asymptotic giant branch (AGB) evolution of stars with masses between . We focus on stars with a solar chemical composition, which allows u…

astro-ph.SR2017★ 22 cited

Three-dimensional simulations of the interaction between the nova ejecta, the accretion disk, and the companion star

Joana Figueira, Jordi Jose, Enrique Garcia-Berro +3

Context. Classical novae are thermonuclear explosions hosted by accreting white dwarfs in stellar binary systems. Material piles up on top of the white dwarf star under mildly dege…

astro-ph.EP2017★ 46 cited

The K2-HERMES Survey. I. Planet Candidate Properties from K2 Campaigns 1-3

Robert A. Wittenmyer, Sanjib Sharma, Dennis Stello +31

Accurate and precise radius estimates of transiting exoplanets are critical for understanding their compositions and formation mechanisms. To know the planet, we must know the host…

physics.comp-ph2017★ 6 cited

Effective transient behaviour of inclusions in diffusion problems

Laurence Brassart, Laurent Stainier

This paper is concerned with the effective transport properties of heterogeneous media in which there is a high contrast between the phase diffusivities. In this case the transient…

astro-ph.HE2017★ 109 cited

Thermonuclear X-ray bursts

Duncan K. Galloway, Laurens Keek

Type-I X-ray bursts arise from unstable thermonuclear burning of accreted fuel on the surface of neutron stars. In this chapter we review the fundamental physics of the burning pro…