activity
20212025
most citedGaia Data Release 3. Summary of the variability processing and analysis

143 citations · 266 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

photoD with Rubin's Data Preview 1: first stellar photometric distances and deficit of faint blue stars. Stellar distances with Rubin's DP1

L. Palaversa, E. Donev, Ž. Ivezić +96

Aims: We investigate the utility of Rubin's Data Preview 1 for estimating stellar number density profile in the Milky Way halo. Methods: Stellar broad-band near-UV to near-IR $ugri…

astro-ph.SR2024★ 9 cited

A new dimension in the variability of AGB stars: convection patterns size changes with pulsation

A. Rosales-Guzmán, J. Sanchez-Bermudez, C. Paladini +16

Stellar convection plays an important role in atmospheric dynamics, wind formation and the mass-loss processes in Asymptotic Giant Branch (AGB) stars. However, a direct characteriz…

astro-ph.GA2023★ 7 cited

Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars

Gaia Collaboration, A. Krone-Martins, C. Ducourant +398

Context. Strongly lensed quasars are fundamental sources for cosmology. The Gaia space mission covers the entire sky with the unprecedented resolution of " in the optical, ma…

astro-ph.SR2022★ 143 cited

Gaia Data Release 3. Summary of the variability processing and analysis

L. Eyer, M. Audard, B. Holl +55

Context. Gaia has been in operations since 2014. The third Gaia data release expands from the early data release (EDR3) in 2020 by providing 34 months of multi-epoch observations t…

astro-ph.SR2022★ 86 cited

Gaia Data Release 3: The second Gaia catalogue of Long-Period Variable candidates

T. Lebzelter, N. Mowlavi, I. Lecoeur-Taibi +9

The third Gaia Data Release, covering 34 months of data, includes the second Gaia catalogue of long-period variables (LPVs), with G variability amplitudes larger than 0.1 mag (5-95…

astro-ph.SR2021★ 21 cited

Semi-regular red giants as distance indicators I. The period-luminosity relations of semi-regular variables revisited

Michele Trabucchi, Nami Mowlavi, Thomas Lebzelter

Semi-regular variables (SRVs) are similar to Miras in brightness, and they also follow PLRs, though not necessarily the same as Miras. As potential standard candles they are more c…