activity
20042022
most citedGaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

1k citations · 1.9k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2022★ 37 cited

The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109

C. C. Espaillat, G. J. Herczeg, T. Thanathibodee +59

The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director's Discretionary Program of low-mass pre-main-sequence stars, coupled with forthcoming data fro…

astro-ph.SR2021★ 76 cited

PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis

C. F. Manara, A. Frasca, L. Venuti +69

The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…

astro-ph.IM2020★ 1k cited

Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

L. Lindegren, U. Bastian, M. Biermann +14

Gaia Early Data Release 3 (Gaia EDR3) gives trigonometric parallaxes for nearly 1.5 billion sources. Inspection of the EDR3 data for sources identified as quasars reveals that thei…

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.EP2019★ 5 cited

Kepler Object of Interest Network III. Kepler-82f: A new non-transiting $21 M_\bigoplus$ planet from photodynamical modelling

J. Freudenthal, C. von Essen, A. Ofir +13

Context. The Kepler Object of Interest Network (KOINet) is a multi-site network of telescopes around the globe organised for follow-up observations of transiting planet candidate K…

astro-ph.EP2018★ 30 cited

Kepler Object of Interest Network II. Photodynamical modelling of Kepler-9 over 8 years of transit observations

J. Freudenthal, C. von Essen, S. Dreizler +14

The Kepler Object of Interest Network (KOINet) is a multi-site network of telescopes around the globe organised to follow up transiting planet candidate KOIs with large transit tim…

astro-ph.IM2018★ 211 cited

Gaia Data Release 2: Properties and validation of the radial velocities

D. Katz, P. Sartoretti, M. Cropper +51

For Gaia DR2 (GDR2), 280 million spectra, collected by the RVS instrument on-board Gaia, were processed and median radial velocities were derived for 9.8 million sources brighter t…

astro-ph.SR2018★ 135 cited

Gaia Data Release 2: Variable stars in the colour-absolute magnitude diagram

Gaia Collaboration, L. Eyer, L. Rimoldini +14

The ESA Gaia mission provides a unique time-domain survey for more than 1.6 billion sources with G ~ 21 mag. We showcase stellar variability across the Galactic colour-absolute mag…

astro-ph.EP2018★ 22 cited

Kepler Object of Interest Network I. First results combining ground and space-based observations of Kepler systems with transit timing variations

C. von Essen, A. Ofir, S. Dreizler +35

During its four years of photometric observations, the Kepler space telescope detected thousands of exoplanets and exoplanet candidates. One of Kepler's greatest heritages has been…

astro-ph.IM2016★ 92 cited

Gaia Data Release 1: The reference frame and the optical properties of ICRF sources

F. Mignard, S. Klioner, L. Lindegren +18

As part of the data processing for Gaia Data Release~1 (Gaia DR1) a special astrometric solution was computed, the so-called auxiliary quasar solution. This gives positions for sel…

astro-ph.EP2013★ 49 cited

Curved walls: Grain growth, settling, and composition patterns in T Tauri disk dust sublimation fronts

M. K. McClure, P. D'Alessio, N. Calvet +6

The dust sublimation walls of disks around T Tauri stars represent a directly observable cross-section through the disk atmosphere and midplane. Their emission properties can probe…

astro-ph.SR2013★ 50 cited

Characterizing the stellar photospheres and near-infrared excesses in accreting T Tauri systems

M. K. McClure, N. Calvet, C. Espaillat +6

Using NASA IRTF SpeX data from 0.8 to 4.5 m, we determine self-consistently the stellar properties and excess emission above the photosphere for a sample of classical T Tauri st…

astro-ph2004★ 81 cited

Mc Neil's Nebula in Orion: The Outburst History

C. Briceno, A. K. Vivas, J. Hernandez +6

We present a sequence of I-band images obtained at the Venezuela 1m Schmidt telescope during the outburst of the nebula recently discovered by J.W. McNeil in the Orion L1630 molecu…