output
19922026
Showing 2020Show all

977 papers · 1 filter

astro-ph.HE2020★ 31 cited

Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos

P. Agnes, S. Albergo, I. F. M. Albuquerque +273

Future liquid-argon DarkSide-20k and ARGO detectors, designed for direct dark matter search, will be sensitive also to core-collapse supernova neutrinos, via coherent elastic neutr…

cond-mat.soft2020★ 8 cited

Adsorption of a fabric conditioner on cellulose nanocrystals: Synergistic effects of surfactant vesicles and polysaccharides on softness properties

Evdokia K. Oikonomou, Grazia M. L. Messina, Laurent Heux +2

Concentrated fabric conditioners are water-based formulations containing 10 wt. % of cationic surfactants that are deposited on textile fibers during the rinse cycle in a washing m…

astro-ph.HE2020★ 4 cited

Stellar wind structures in the eclipsing binary system IGR J18027-2016

Federico A. Fogantini, Federico García, Jorge A. Combi +1

IGR J18027-2016 is an obscured high-mass X-ray binary formed by a neutron star accreting from the wind of a supergiant companion with a 4.57 day orbital period. The source sh…

physics.med-ph2020★ 18 cited

18F-FDG-PET dissemination features in diffuse large B cell lymphoma are predictive of outcome

Anne-Ségolène Cottereau, Christophe Nioche, Anne-Sophie Dirand +5

We assessed the predictive value of new radiomic features characterizing the lesion dissemination in baseline 18F-FDG PET and tested whether combining them with baseline metabolic…

nucl-ex2020★ 81 cited

Laser spectroscopy of neutron-rich Hg isotopes: Illuminating the kink and odd-even staggering in charge radii across the shell closure

T. Day Goodacre, A. V. Afanasjev, A. E. Barzakh +41

The mean-square charge radii of Hg () have been studied for the first time and those of Hg () remeasured by the applicat…

astro-ph.IM2020★ 3 cited

Towards a physical understanding of the thermal background in large ground-based telescopes

Leonard Burtscher, Ioannis Politopoulos, Sergio Fernández-Acosta +11

Ground-based thermal-infrared observations have a unique scientific potential, but are also extremely challenging due to the need to accurately subtract the high thermal background…

astro-ph.GA2020★ 84 cited

Dust polarized emission observations of NGC 6334; BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network

D. Arzoumanian, R. Furuya, T. Hasegawa +145

[Abridged] Filaments and hubs have received special attention recently thanks to studies showing their role in star formation. While the column density and velocity structures of b…

astro-ph.GA2020★ 9 cited

MusE GAs FLOw and Wind (MEGAFLOW) VII. A NOEMA pilot program to probe molecular gas in galaxies with measured circumgalactic gas flows

Jonathan Freundlich, Nicolas F. Bouché, Thierry Contini +5

We present a pilot program using IRAM's NOrthern Extended Millimeter Array (NOEMA) to probe the molecular gas reservoirs of six star-forming galaxies whose circumgalact…

astro-ph.GA2020★ 22 cited

First Co-spatial Comparison of Stellar, Neutral-, and Ionized-gas Metallicities in a metal-rich galaxy: M83

Svea Hernandez, Alessandra Aloisi, Bethan L. James +14

We carry out a comparative analysis of the metallicities from the stellar, neutral-gas, and ionized-gas components in the metal-rich spiral galaxy M83. We analyze spectroscopic obs…

physics.geo-ph2020★ 8 cited

Can one use Earth's magnetic axial dipole field intensity to predict reversals?

Kyle Gwirtz, Matthias Morzfeld, Alexandre Fournier +1

We study predictions of reversals of Earth's axial magnetic dipole field that are based solely on the dipole's intensity. The prediction strategy is, roughly, that once the dipole…

astro-ph.IM2020★ 1 cited

FIRST, a Pupil-Remapping Fiber Interferometer at the Subaru Telescope: on-sky results

Sébastien Vievard, Elsa Huby, Sylvestre Lacour +13

FIRST, the Fibered Imager foR a Single Telescope, is a spectro-imager using single-mode fibers for pupil remapping, allowing measurements beyond the telescope diffraction limit. In…

cs.LG2020★ 5 cited

Fast and Accurate -means++ via Rejection Sampling

Vincent Cohen-Addad, Silvio Lattanzi, Ashkan Norouzi-Fard +2

-means++ \cite{arthur2007k} is a widely used clustering algorithm that is easy to implement, has nice theoretical guarantees and strong empirical performance. Despite its wide a…

gr-qc2020★ 13 cited

MICROSCOPE mission: Data analysis principle

Joel Bergé, Quentin Baghi, Emilie Hardy +10

After performing highly sensitive acceleration measurements during two years of drag-free flight around the Earth, MICROSCOPE provided the best constraint on the Weak Equivalence P…

physics.optics2020★ 38 cited

High temperature metamaterial terahertz quantum detector

Mathieu Jeannin, Thomas Bonazzi, Djamal Gacemi +7

We demonstrate a high temperature performance quantum detector of Terahertz (THz) radiation based on three-dimensional metamaterial. The metamaterial unit cell consists of an induc…

cond-mat.dis-nn2020★ 48 cited

Low-frequency vibrational spectrum of mean-field disordered systems

Eran Bouchbinder, Edan Lerner, Corrado Rainone +2

We study a recently introduced and exactly solvable mean-field model for the density of vibrational states of a structurally disordered system. The model is formul…

astro-ph.IM2020

Socio-demographic study of the exoplanet direct imaging community

Lucie Leboulleux, Élodie Choquet, Elsa Huby +2

Astronomy and science are fields in which specific groups remain under-represented despite multiple studies that investigate this issue and propose solutions. In this article, we a…

physics.optics2020★ 18 cited

Efficient Type II Second Harmonic Generation in an Indium Gallium Phosphide on insulator wire waveguide aligned with a crystallographic axis

Nicolas Poulvellarie, Carlos Mas Arabi, Charles Ciret +7

We theoretically and experimentally investigate type II second harmonic generation in III-V-on-insulator wire waveguides. We show that the propagation direction plays a crucial rol…

astro-ph.SR2020★ 1 cited

Probing the internal magnetism of stars using asymptotic magneto-asteroseismology

Stéphane Mathis, Lisa Bugnet, Vincent Prat +3

Our knowledge of the dynamics of stars has undergone a revolution thanks to the simultaneous large amount of high-quality photometric observations collected by space-based asterose…

astro-ph.HE2020★ 31 cited

Observation of a sudden cessation of a very-high-energy gamma-ray flare in PKS 1510-089 with H.E.S.S. and MAGIC in May 2016

H. E. S. S. Collaboration, H. Abdalla, R. Adam +430

The flat spectrum radio quasar (FSRQ) PKS 1510-089 is known for its complex multiwavelength behavior, and is one of only a few FSRQs detected at very high energy (VHE, GeV…

gr-qc2020★ 13 cited

Quadratic DHOST theories revisited

David Langlois, Karim Noui, Hugo Roussille

We present a novel and remarkably simple formulation of degenerate higher-order scalar-tensor (DHOST) theories whose Lagrangian is quadratic in second derivatives of some scalar fi…

astro-ph.EP2020★ 5 cited

Debris discs in binaries: morphology and photometric signatures

Philippe Thebault, Quentin Kral, Johan Olofsson

We aim to see whether debris belts evolving in between two stars may be impacted by the presence of the companion and whether this leaves any detectable signature that could be obs…

astro-ph.SR2020★ 45 cited

TESS observations of Cepheid stars: first light results

E. Plachy, A. Pál, A. Bódi +33

We present the first analysis of Cepheid stars observed by the TESS space mission in Sectors 1 to 5. Our sample consists of 25 pulsators: ten fundamental mode, three overtone and t…

astro-ph.GA2020★ 19 cited

Dust, gas, and metal content in star-forming galaxies at revealed with ALMA and Near-IR spectroscopy

Tomoko L. Suzuki, Masato Onodera, Tadayuki Kodama +8

We conducted sub-millimeter observations with the Atacama Large Millimeter/sub-millimeter Array (ALMA) of star-forming galaxies at , whose gas-phase metallicities have be…

astro-ph.SR2020

The impact of a fossil magnetic field on dipolar mixed-mode frequencies in sub- and red-giant stars

L. Bugnet, V. Prat, S. Mathis +5

Stars more massive than M are known to develop a convective core during the main-sequence: the dynamo process triggered by this convection could be the origin of…