output
19922026
most citedThe SIESTA method for ab initio order-N materials simulation

12k citations

Showing 2020 · astro-ph.GAShow all

13 papers · 2 filters

astro-ph.GA2020★ 42 cited

Gaia GraL: Gaia DR2 Gravitational Lens Systems. VI. Spectroscopic Confirmation and Modeling of Quadruply-Imaged Lensed Quasars

D. Stern, S. G. Djorgovski, A. Krone-Martins +23

Combining the exquisite angular resolution of Gaia with optical light curves and WISE photometry, the Gaia Gravitational Lenses group (GraL) uses machine learning techniques to ide…

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.GA2020★ 219 cited

Gaia Early Data Release 3: Summary of the contents and survey properties

Gaia Collaboration, A. G. A Brown, A. Vallenari +423

We present the early installment of the third Gaia data release, Gaia EDR3, consisting of astrometry and photometry for 1.8 billion sources brighter than magnitude 21, complemented…

astro-ph.GA2020★ 29 cited

Towards constraining warm dark matter with stellar streams through neural simulation-based inference

Joeri Hermans, Nilanjan Banik, Christoph Weniger +2

A statistical analysis of the observed perturbations in the density of stellar streams can in principle set stringent contraints on the mass function of dark matter subhaloes, whic…

astro-ph.GA2020★ 17 cited

Spectropolarimetry of the changing-look active galactic nucleus Mrk 1018

Damien Hutsemékers, Beatriz Agís González, Frédéric Marin +1

We have obtained new spectropolarimetric observations at visible wavelengths of the changing-look active galactic nucleus (AGN) Mrk 1018. The AGN direct spectrum shows an extremely…

astro-ph.GA2020★ 2 cited

Quasar catalogue for the astrometric calibration of the forthcoming ILMT survey

Amit Kumar Mandal, Bikram Pradhan, Jean Surdej +3

Quasars are ideal targets to use for astrometric calibration of large scale astronomical surveys as they have negligible proper motion and parallax. The forthcoming 4-m Internation…