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20082021
most citedDetection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole

947 citations · 2.4k across the 32 of their papers we have counts for

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Showing 2019Show all

8 papers · 1 filter

astro-ph.IM2019★ 26 cited

Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event

Weicheng Zang, Subo Dong, Andrew Gould +24

We report the lens mass and distance measurements of the nearby microlensing event TCP J05074264+2447555. We measure the microlens parallax vector using Spitzer and gro…

astro-ph.SR2019★ 7 cited

Evidence of a substellar companion to AB Dor C

J. B. Climent, J. P. Berger, J. C. Guirado +5

Studies of fundamental parameters of very low-mass objects are indispensable to provide tests of stellar evolution models that are used to derive theoretical masses of brown dwarfs…

astro-ph.SR2019★ 30 cited

The Araucaria Project: High-precision orbital parallax and masses of eclipsing binaries from infrared interferometry

A. Gallenne, G. Pietrzyński, D. Graczyk +9

Context. The precise determinations of stellar mass at 1% provide important constraints on stellar evolution models. Accurate parallax measurements can also serve as independ…

astro-ph.SR2019★ 1 cited

The Leavitt law of Milky Way Cepheids from Gaia DR2 static companion parallaxes

Louise Breuval, Pierre Kervella, Frédéric Arenou +13

Classical Cepheids (CCs) are at the heart of the empirical extragalactic distance ladder. Milky Way CCs are the only stars of this class accessible to trigonometric parallax measur…

astro-ph.SR2019★ 31 cited

A thin shell of ionized gas explaining the IR excess of classical Cepheids

V. Hocdé, N. Nardetto, E. Lagadec +12

Despite observational evidences, InfraRed (IR) excess of classical Cepheids are seldom studied and poorly understood, but probably induces systematics on the Period-Luminosity (PL)…

astro-ph.SR2019★ 30 cited

Diagnosing 0.1-10 au scale morphology of the FU\,Ori disk using ALMA and VLTI/GRAVITY

Hauyu Baobab Liu, Antoine Mérand, Joel D. Green +11

We report new Atacama Large Millimeter/submillimeter Array Band 3 (86-100 GHz; 80 mas angular resolution) and Band 4 (146-160 GHz; 50 mas angular resolution) observatio…