activity
20112023
most citedThe Pisa pre-main sequence tracks and isochrones. A database covering a wide range of Z, Y, mass, and age values

285 citations · 1.4k across the 38 of their papers we have counts for

collaborators

37 papers

astro-ph.SR2023

AESOPUS 2.0: Low-Temperature Opacities with Solid Grains

P. Marigo, P. Woitke, E. Tognelli +3

In this study we compute the equation of state and Rosseland mean opacity from temperatures of T~30000 K down to T~400 K, pushing the capabilities of the AESOPUS code (Marigo et al…

astro-ph.GA2022★ 42 cited

Low mass young stars in the Milky Way unveiled by DBSCAN and Gaia EDR3. Mapping the star forming regions within 1.5 Kpc

L. Prisinzano, F. Damiani, S. Sciortino +6

With an unprecedented astrometric and photometric data precision, Gaia EDR3 gives us, for the first time, the opportunity to systematically detect and map in the optical bands, the…

astro-ph.SR2022★ 11 cited

New calibrated models for the TRGB luminosity and a thorough analysis of theoretical uncertainties

Ippocratis D. Saltas, Emanuele Tognelli

The luminosity of the Tip of the Red Giant Branch (TRGB) is instrumental for the construction of the distance ladder, and its accurate modelling is key for determining the local Hu…

astro-ph.SR2021★ 32 cited

Gaia-ESO Survey: Role of magnetic activity and starspots on pre-main sequence lithium evolution

E. Franciosini, E. Tognelli, S. Degl'Innocenti +24

Pre-main sequence models with inflated radii are needed to simultaneously reproduce the colour-magnitude diagram and the lithium depletion pattern in young open clusters. We tested…

astro-ph.SR2021★ 59 cited

The Gaia-ESO Survey: Membership probabilities for stars in 63 open and 7 globular clusters from 3D kinematics

R. J. Jackson, R. D. Jeffries, N. J. Wright +26

Spectroscopy from the final internal data release of the Gaia-ESO Survey (GES) has been combined with Gaia EDR3 to assign membership probabilities to targets observed towards 63 Ga…

astro-ph.GA2021★ 3 cited

Robust statistical tools for identifying multiple stellar populations in globular clusters in the presence of measurement errors. A case study: NGC 2808

G. Valle, M. Dell'Omodarme, E. Tognelli

The finding of multiple stellar populations (MP), defined by patterns in the stellar element abundances, is nowadays considered a distinctive feature of globular clusters. However,…