activity
20042023
most citedPhoto-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18

262 citations · 500 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2023★ 53 cited

The MPIfR-MeerKAT Galactic Plane survey I -- System setup and early results

P. V. Padmanabh, E. D. Barr, S. S. Sridhar +30

Galactic plane radio surveys play a key role in improving our understanding of a wide range of astrophysical phenomena. Performing such a survey using the latest interferometric te…

astro-ph.SR2019★ 4 cited

Revisiting Kepler-444 Part I. Seismic modelling and inversions of stellar structure

G. Buldgen, M. Farnir, C. Pezzotti +10

Context. The CoRoT and Kepler missions have paved the way for synergies between exoplanetology and asteroseismology. The use of seismic data helps providing stringent constraints o…

astro-ph.GA2019★ 262 cited

Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18

F. Anders, A. Khalatyan, C. Chiappini +19

Combining the precise parallaxes and optical photometry delivered by Gaia's second data release (Gaia DR2) with the photometric catalogues of PanSTARRS-1, 2MASS, and AllWISE, we de…

astro-ph2007★ 87 cited

Late stages of the evolution of A-type stars on the main sequence: comparison between observed chemical abundances and diffusion models for 8 Am stars of the Praesepe cluster

L. Fossati, S. Bagnulo, R. Monier +5

Aims. We aim to provide observational constraints on diffusion models that predict peculiar chemical abundances in the atmospheres of Am stars. We also intend to check if chemical…

astro-ph2007★ 50 cited

Theoretical analysis of the atmospheres of CP stars. Effects of the individual abundance patterns

S. A. Khan, D. V. Shulyak

Context. See abstract in the paper. Aims. See abstract in the paper. Methods. See abstract in the paper. Results. We present a homogeneous study of model atmosphere temperature str…

astro-ph2004★ 40 cited

Stellar model atmospheres with magnetic line blanketing

O. Kochukhov, S. Khan, D. Shulyak

Model atmospheres of A and B stars are computed taking into account magnetic line blanketing. These calculations are based on the new stellar model atmosphere code LLModels which i…