activity
20092026
most citedYields of AGB and SAGB models with chemistry of low- and high-metallicity Globular Clusters

284 citations · 3.1k across the 55 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2026

AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release

A. Viitanen, A. Bongiorno, I. Saccheo +37

Contemporary large-scale surveys such as the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) and Euclid present an unprecedented discovery potential for studying A…

astro-ph.GA2024

Synergies between Roman Galactic Plane Survey and other major surveys

Katarzyna Kruszyńska, Rachel A. Street, Steven Gough-Kelly +15

Nancy Grace Roman Space Telescope will revolutionize our understanding of the Galactic Bulge with its Galactic Bulge Time Domain survey. At the same time, Rubin Observatories's Leg…

astro-ph.GA2024

Light curve's recovery with Rubin-LSST: II. UnVEiling the darknesS of The gAlactic buLgE (VESTALE) with RR Lyrae

M. Di Criscienzo, S. Leccia, V. Braga +16

This work is part of VESTALE, a project initiated within the Rubin-LSST Cadence Strategy Optimization Process . Its goal is to explore the potential of Rubin-LSST observations aime…

astro-ph.GA2023★ 1 cited

Extragalactic Star Cluster Science with the Nancy Grace Roman Space Telescope's High Latitude Wide Area Survey and the Vera C. Rubin Observatory

Kristen C. Dage, Christopher Usher, Jennifer Sobeck +22

The Nancy Grace Roman Telescope's High Latitude Wide Area Survey will have a number of synergies with the Vera Rubin Observatory's Legacy Survey of Space and Time (LSST), particula…

astro-ph.GA2017★ 41 cited

On the faint-end of the galaxy luminosity function in the Epoch of Reionization: updated constraints from the HST Frontier Fields

B. Yue, M. Castellano, A. Ferrara +12

Ultra-faint galaxies are hosted by small dark matter halos with shallow gravitational potential wells, hence their star formation activity is more sensitive to feedback effects. Th…

astro-ph.GA2017★ 39 cited

HST Grism Observations of a Gravitationally Lensed Redshift 10 Galaxy

Austin Hoag, Maruša Bradač, Gabriel B. Brammer +11

We present deep spectroscopic observations of a Lyman-break galaxy candidate (hereafter MACS1149-JD) at with the Space Telescope () WFC3/…

astro-ph.GA2017★ 208 cited

The Star Formation Main Sequence in the Hubble Space Telescope Frontier Fields

Paola Santini, Adriano Fontana, Marco Castellano +13

We investigate the relation between the star formation rate (SFR) and the stellar mass (M), i.e. the Main Sequence (MS) relation of star-forming galaxies, at 1.3<=z<6 in the first…

astro-ph.GA2014★ 110 cited

The dust production rate of AGB stars in the Magellanic Clouds

Raffaella Schneider, Rosa Valiante, Paolo Ventura +4

We compare theoretical dust yields for stars with mass 1 Msun < mstar < 8 Msun, and metallicities 0.001 < Z < 0.008 with observed dust production rates (DPR) by carbon- rich and ox…

astro-ph.GA2012★ 4 cited

Star Formation in the Starburst Cluster in NGC 3603

Matteo Correnti, Francesco Paresce, Rossella Aversa +7

We have used new, deep, visible and near infrared observations of the compact starburst cluster in the giant HII region NGC 3603 and its surroundings with the WFC3 on HST and HAWK-…

astro-ph.GA2010★ 29 cited

Terzan 5: an alternative interpretation for the split horizontal branch

F. D'Antona, P. Ventura, V. Caloi +4

We consider the horizontal branch (HB) of the Globular Cluster Terzan 5, recently shown to be split into two parts, the fainter one (delta M_K ~ 0.3mag) having a lower metallicity…