activity
20192025
most citedGetting ready for the LSST data -- estimating the physical properties of main sequence galaxies

11 citations · 32 across the 7 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2025

FAST-SBF: an automatic procedure for the measurement of Surface Brightness Fluctuations for large sky surveys

Gabriele Riccio, Michele Cantiello, Rebecca Habas +9

The Surface Brightness Fluctuation method is one of the most reliable and efficient ways of measuring distances to galaxies within 100 Mpc. While recent implementations have increa…

astro-ph.GA2025★ 4 cited

Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster IV. A study of the Globular Cluster population in four UDGs

Marco Mirabile, Michele Cantiello, Marina Rejkuba +20

As old stellar systems, globular clusters (GCs) are key fossil tracers of galaxy formation and interaction histories. This paper is part of the LEWIS project, an integral-field spe…

astro-ph.GA2024★ 3 cited

VEGAS-SSS: An intra-group component in the globular cluster system of NGC 5018 group of galaxies using VST data

Pratik Lonare, Michele Cantiello, Marco Mirabile +7

Globular clusters (GCs) are fossil tracer of formation and evolution of galaxies and studying their properties provides crucial insights into past formation and interaction events.…

astro-ph.GA2024★ 10 cited

VEGAS-SSS: Tracing Globular Cluster Populations in the Interacting NGC3640 Galaxy Group

Marco Mirabile, Michele Cantiello, Pratik Lonare +15

Globular clusters (GCs) are among the oldest stellar systems in the universe. As such, GCs population are valuable fossil tracers of galaxy formation and interaction history. We us…

astro-ph.GA2021★ 11 cited

Getting ready for the LSST data -- estimating the physical properties of main sequence galaxies

Gabriele Riccio, Katarzyna Małek, Ambra Nanni +8

In this work we study how to employ the upcoming Legacy Survey of Space and Time (LSST) data to constrain physical properties of normal, star forming galaxies. We use simulated LSS…