output
19922026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2017Show all

614 papers · 1 filter

hep-ex2017★ 19 cited

Amplitude analysis of the decay and first observation of the CP asymmetry in

LHCb collaboration, R. Aaij, B. Adeva +794

The time-integrated Dalitz plot of the three-body hadronic charmless decay is studied using a collision data…

physics.flu-dyn2017★ 26 cited

Parametric instability and wave turbulence driven by tidal excitation of internal waves

Thomas Le Reun, Benjamin Favier, Michael Le Bars

We investigate the stability of stratified fluid layers undergoing homogeneous and periodic tidal deformation. We first introduce a local model which allows to study velocity and b…

astro-ph.GA2017★ 28 cited

The VIMOS Public Extragalactic Redshift Survey (VIPERS). AGN feedback in [NeV] emitters

D. Vergani, B. Garilli, M. Polletta +36

Using an unconventional single line diagnostic that unambiguously identifies AGNs in composite galaxies we report statistical differences in the properties (stellar age, [OII] lumi…

astro-ph.EP2017★ 56 cited

Tensile Strength of 67P/Churyumov-Gerasimenko Nucleus Material from Overhangs

N. Attree, O. Groussin, L. Jorda +52

We directly measure twenty overhanging cliffs on the surface of comet 67P/Churyumov-Gerasimenko extracted from the latest shape model and estimate the minimum tensile strengths nee…

astro-ph.GA2017★ 13 cited

The ESO's VLT Type Ia supernova spectral set of the final two years of SNLS

C. Balland, F. Cellier-Holzem, C. Lidman +24

We aim to present 70 spectra of 68 new high-redshift type Ia supernovae (SNeIa) measured at ESO's VLT during the final two years of operation (2006-2008) of the Supernova Legacy Su…

physics.plasm-ph2017★ 71 cited

Laser-driven strong magnetostatic fields with applications to charged beam transport and magnetized high energy-density physics

J. J. Santos, M. Bailly-Grandvaux, M. Ehret +28

Powerful laser-plasma processes are explored to generate discharge currents of a few kA in coil targets, yielding magnetostatic fields (B-fields) in excess of kT. The…

physics.plasm-ph2017★ 25 cited

Practical dispersion relations for strongly coupled plasma fluids

Sergey Khrapak

Very simple explicit analytical expressions are discussed, which are able to describe the dispersion relations of longitudinal waves in strongly coupled plasma systems such as one-…

astro-ph.EP2017★ 18 cited

New spectro-photometric characterization of the substellar object HR 2562 B using SPHERE

D. Mesa, J. -L. Baudino, B. Charnay +32

HR2562 is an F5V star located at ~33 pc from the Sun hosting a substellar companion that was discovered using the GPI instrument. The main objective of the present paper is to prov…

astro-ph.EP2017★ 15 cited

Predictions of planet detections with near infrared radial velocities in the up-coming SPIRou Legacy Survey-Planet Search

Ryan Cloutier, Étienne Artigau, Xavier Delfosse +8

The SPIRou near infrared spectro-polarimeter is destined to begin science operations at the Canada-France-Hawaii Telescope in mid-2018. One of the instrument's primary science goal…

astro-ph.GA2017★ 88 cited

Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0

Kameswara Bharadwaj Mantha, Daniel H. McIntosh, Ryan Brennan +37

The rate of major galaxy-galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development (). We us…

astro-ph.SR2017★ 92 cited

The lithium-rotation connection in the 125 Myr-old Pleiades cluster

J. Bouvier, D. Barrado, E. Moraux +9

The evolution of lithium abundance over a star's lifetime is indicative of transport processes operating in the stellar interior. We revisit the relationship between lithium conten…

physics.soc-ph2017★ 250 cited

Can co-location be used as a proxy for face-to-face contacts?

Mathieu Génois, Alain Barrat

Technological advances have led to a strong increase in the number of data collection efforts aimed at measuring co-presence of individuals at different spatial resolutions. It is…

astro-ph.GA2017★ 15 cited

Abundance ratios in dwarf elliptical galaxies

Ş. Şen, R. F. Peletier, A. Boselli +14

We determine abundance ratios of 37 dwarf ellipticals (dEs) in the nearby Virgo cluster. This sample is representative of the early-type population of galaxies in the absolute magn…

math.CO2017★ 1 cited

Cyclotomic shuffles

O. Ogievetsky, V. Petrova

Analogues of 1-shuffle elements for complex reflection groups of type are introduced. A geometric interpretation for in terms of rotational permutations of po…

physics.plasm-ph2017★ 32 cited

Thermal runaway in two-dimensional complex plasma crystals

Lénaïc Couëdel, V. Nosenko, M Rubin-Zuzic +4

The full melting of a two-dimensional plasma crystal was induced in a principally stable monolayer by localized laser stimulation. Two distinct behaviors of the crystal after laser…

astro-ph.SR2017★ 82 cited

SPIRou Input Catalogue: Global properties of 440 M dwarfs observed with ESPaDOnS at CFHT

Pascal Fouqué, Claire Moutou, Lison Malo +13

Present and future high-precision radial-velocity spectrometers dedicated to the discovery of low-mass planets orbiting low-mass dwarfs need to focus on the best selected stars to…

astro-ph.GA2017★ 39 cited

An alternate approach to measure specific star formation rates at 2<z<7

Iary Davidzon, Olivier Ilbert, Andreas L. Faisst +2

We trace the specific star formation rate (sSFR) of massive star-forming galaxies () from to 7. Our method is substantially different…

math.OC2017★ 33 cited

- Regularization of Split Feasibility Problems

Abdellatif Moudafi, Aviv Gibali

Numerous problems in signal processing and imaging, statistical learning and data mining, or computer vision can be formulated as optimization problems which consist in minimizing…

astro-ph.GA2017★ 246 cited

Galaxy growth in a massive halo in the first billion years of cosmic history

D. P. Marrone, J. S. Spilker, C. C. Hayward +34

According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in reg…

astro-ph.GA2017★ 96 cited

From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully-Fisher relation

Anastasia A. Ponomareva, Marc A. W. Verheijen, Emmanouil Papastergis +2

In this paper we investigate the statistical properties of the Baryonic Tully-Fisher relation (BTFr) for a sample of 32 galaxies with accurate distances based on Cepheids and/or TR…

astro-ph.CO2017★ 37 cited

Cosmological constraints from galaxy clustering in the presence of massive neutrinos

Matteo Zennaro, Julien Bel, Jason Dossett +2

The clustering ratio is defined as the ratio between the correlation function and the variance of the smoothed overdensity field. In LCDM cosmologies not accounting for massive neu…

astro-ph.IM2017★ 68 cited

Deep learning Approach for Classifying, Detecting and Predicting Photometric Redshifts of Quasars in the Sloan Digital Sky Survey Stripe 82

Johanna Pasquet-Itam, Jérôme Pasquet

We apply a convolutional neural network (CNN) to classify and detect quasars in the Sloan Digital Sky Survey Stripe 82 and also to predict the photometric redshifts of quasars. The…

astro-ph.GA2017★ 74 cited

Evidence for Merger-Driven Growth in Luminous, High-z, Obscured AGN in the CANDELS/COSMOS Field

J. L. Donley, J. Kartaltepe, D. Kocevski +27

While major mergers have long been proposed as a driver of both AGN activity and the M-sigma relation, studies of moderate to high redshift Seyfert-luminosity AGN hosts have found…

astro-ph.CO2017★ 23 cited

Sub-structure and merger detection in resolved NIKA Sunyaev-Zel'dovich images of distant clusters

R. Adam, O. Hahn, F. Ruppin +48

Sub-structures in the hot gas of galaxy clusters are related to their formation history and to the astrophysical processes at play in the intracluster medium (ICM). The thermal Sun…