output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

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372 papers · 1 filter

astro-ph.CO2020★ 29 cited

Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs

Hironao Miyatake, Yosuke Kobayashi, Masahiro Takada +7

We present validation tests of emulator-based halo model method for cosmological parameter inference, assuming hypothetical measurements of the projected correlation function of ga…

astro-ph.SR2020★ 6 cited

Searching for active low-mass stars in CMa star-forming region: multi-band photometry with T80S

J. Gregorio-Hetem, F. Navarete, A. Hetem +10

An exotic environment surrounds the young stellar groups associated with the Canis Major (CMa) OB1/R1 region, which probably was formed under feedback from at least three supernova…

astro-ph.CO2020★ 9 cited

Non-perturbative halo clustering from cosmological density peaks

Tobias Baldauf, Sandrine Codis, Vincent Desjacques +1

Associating the formation sites of haloes with the maxima of the smoothed linear density field, we present non-perturbative predictions for the Lagrangian and evolved halo correlat…

astro-ph.CO2020★ 34 cited

Phase-space structure of protohalos: Vlasov versus Particle-Mesh

Stéphane Colombi

The phase-space structure of primordial dark matter halos is revisited using cosmological simulations with three sine waves and Cold Dark Matter (CDM) initial conditions. The simul…

astro-ph.SR2020★ 18 cited

Census of R Coronae Borealis stars I: Infrared light curves from Palomar Gattini IR

Viraj R. Karambelkar, Mansi M. Kasliwal, Patrick Tisserand +16

We are undertaking the first systematic infrared (IR) census of R Coronae Borealis (RCB) stars in the Milky Way, beginning with IR light curves from the Palomar Gattini IR (PGIR) s…

astro-ph.HE2020★ 5 cited

Neutron stars as probes of dark matter

M. Ángeles Pérez-García, J. Silk

Neutron Stars (NSs) are compact stellar objects that are stable solutions in General Relativity. Their internal structure is usually described using an equation of state that invol…

astro-ph.CO2020★ 31 cited

A fast semi-discrete optimal transport algorithm for a unique reconstruction of the early Universe

Bruno Lévy, Roya Mohayaee, Sebastian von Hausegger

We leverage powerful mathematical tools stemming from optimal transport theory and transform them into an efficient algorithm to reconstruct the fluctuations of the primordial dens…

astro-ph.CO2020★ 82 cited

Dark Energy Survey Year 3 Results: Clustering Redshifts -- Calibration of the Weak Lensing Source Redshift Distributions with redMaGiC and BOSS/eBOSS

M. Gatti, G. Giannini, G. M. Bernstein +94

We present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing source galaxy redshift distributions from clustering measurements. In particular, we cross-…

astro-ph.IM2020★ 7 cited

DRAGraces: A pipeline for the GRACES high-resolution spectrograph at Gemini

André-Nicolas Chené, Shunyuan Mao, Michael Lundquist +2

This paper describes the software DRAGraces (Data Reduction and Analysis for GRACES), which is a pipeline reducing spectra from GRACES (Gemini Remote Access to the CFHT ESPaDOnS Sp…

astro-ph.GA2020★ 3 cited

Discovery of a damped Ly galaxy at z 3 towards the quasar SDSS J011852+040644

Ravi Joshi, Michele Fumagalli, Raghunathan Srianand +11

We report the detection of the host galaxy of a damped Ly system (DLA) with log N(HI) = at towards the background quasar SDSS…

astro-ph.GA2020★ 49 cited

Constraining the quasar radio-loud fraction at with deep radio observations

Yuanqi Liu, Ran Wang, Emmanuel Momjian +8

We carry out a series of deep Karl G. Jansky Very Large Array (VLA) S-band observations of a sample of 21 quasars at . The new observations expand the searches of radio con…

astro-ph.HE2020★ 8 cited

Fast radio burst repeaters produced via Kozai-Lidov feeding of neutron stars in binary systems

Valentin Decoene, Kumiko Kotera, Joseph Silk

Neutron stars are likely surrounded by gas, debris, and asteroid belts. Kozai-Lidov perturbations, induced by a distant, but gravitationally bound companion, can trigger the infall…

astro-ph.CO2020★ 42 cited

The Dark Energy Survey Supernova Program: Modelling selection efficiency and observed core collapse supernova contamination

M. Vincenzi, M. Sullivan, O. Graur +79

The analysis of current and future cosmological surveys of type Ia supernovae (SNe Ia) at high-redshift depends on the accurate photometric classification of the SN events detected…

astro-ph.GA2020★ 20 cited

Star-Gas Misalignment in Galaxies: II. Origins Found from the Horizon-AGN Simulation

Donghyeon J. Khim, Sukyoung K. Yi, Christophe Pichon +5

There have been many studies aiming to reveal the origins of the star-gas misalignment found in galaxies, but there still is a lack of understanding of the contribution from each f…

astro-ph.GA2020★ 6 cited

The properties and environment of very young galaxies in the local Universe

M. Trevisan, G. A. Mamon, T. X. Thuan +3

In the local Universe, there is a handful of dwarf compact star-forming galaxies with extremely low oxygen abundances. It has been proposed that they are young, having formed a lar…

astro-ph.CO2020★ 13 cited

Boosting small-scale structure via primordial black holes and implications for sub-GeV dark matter annihilation

Kenji Kadota, Joseph Silk

We explore the possibility that the annihilation of dark matter (DM) is boosted due to enhanced substructure in the presence of primordial black holes (PBHs) which constitute a sub…

astro-ph.SR2020★ 340 cited

Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars

Gaia Collaboration, R. L. Smart, L. M. Sarro +420

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the…

astro-ph.GA2020★ 112 cited

Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry

Gaia Collaboration, S. A. Klioner, F. Mignard +414

Context. Gaia Early Data Release 3 (Gaia EDR3) provides accurate astrometry for about 1.6 million compact (QSO-like) extragalactic sources, 1.2 million of which have the best-quali…

astro-ph.CO2020★ 34 cited

Close-up view of a luminous star-forming galaxy at z=2.95

S. Berta, A. J. Young, P. Cox +35

(Abridged) Exploiting the sensitivity and broad band width of NOEMA, we have studied the molecular gas and dust in the galaxy HerBS-89a, at z=2.95. High angular resolution images r…

gr-qc2020★ 23 cited

Minimal Theory of Bigravity: construction and cosmology

Antonio De Felice, François Larrouturou, Shinji Mukohyama +1

Following the path of minimalism in alternative theories of gravity, we construct the "Minimal Theory of Bigravity" (MTBG), a theory of two interacting spin-2 fields that propagate…

astro-ph.EP2020★ 113 cited

New constraints on the planetary system around the young active star AU Mic. Two transiting warm Neptunes near mean-motion resonance

E. Martioli, G. Hébrard, A. C. M. Correia +2

AU Mic is a young, active star whose transiting planet was recently detected. We report our analysis of its TESS data, where we modeled the BY Draconis type quasi-periodic rotation…

astro-ph.HE2020★ 17 cited

The potential role of binary neutron star merger afterglows in multimessenger cosmology

S. Mastrogiovanni, R. Duque, E. Chassande-Mottin +2

Binary neutron star mergers offer a new and independent means of measuring the Hubble constant by combining the gravitational-wave inferred source luminosity distance with it…

astro-ph.CO2020★ 55 cited

Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS

R. Cawthon, J. Elvin-Poole, A. Porredon +83

We present clustering redshift measurements for Dark Energy Survey (DES) lens sample galaxies to be used in weak gravitational lensing and galaxy clustering studies. To perform thi…

astro-ph.CO2020★ 70 cited

Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog

S. Everett, B. Yanny, N. Kuropatkin +97

We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the selection and photometric biases of the Dark Energy Survey's (DES) Year 3 (Y3) data…