activity
19962017
most citedMACHO Alert 95-30 : First Real-Time Observation of Extended Source Effects in Gravitational Microlensing

162 citations · 799 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2017★ 10 cited

The open cluster King~1 in the second quadrant

R. Carrera, L. Rodríguez Espinosa, L. Casamiquela +4

We analyse the poorly-studied open cluster King~1 in the second Galactic quadrant. From wide-field photometry we have studied the spatial distribution of this cluster. We determine…

astro-ph.SR2016★ 13 cited

The Cepheids of NGC1866: A Precise Benchmark for the Extragalactic Distance Scale and Stellar Evolution from Modern UBVI Photometry

I. Musella, M. Marconi, P. B. Stetson +8

We present the analysis of multiband time-series data for a sample of 24 Cepheids in the field of the Large Magellanic Cloud cluster NGC1866. Very accurate BVI VLT photometry is co…

astro-ph.SR2015

The Carina Project IX: on Hydrogen and helium burning variables

G. Coppola, M. Marconi, P. B. Stetson +14

We present new multi-band (UBVI) time-series data of helium burning variables in the Carina dwarf spheroidal galaxy. The current sample includes 92 RR Lyrae-six of them are new ide…

astro-ph.IM2014

Stellar populations in the ELT perspective

G. Bono, V. F. Braga, M. Fabrizio +11

We discuss the impact that the next generation of Extremely Large Telescopes will have on the open astrophysical problems of resolved stellar populations. In particular, we address…

astro-ph.GA2012★ 60 cited

The Discovery of an Ultra-Faint Star Cluster in the Constellation of Ursa Minor

Ricardo R. Munoz, Marla Geha, Patrick Cote +5

We report the discovery of a new ultra-faint globular cluster in the constellation of Ursa Minor, based on stellar photometry from the MegaCam imager at the Canada-France-Hawaii Te…

astro-ph.SR2010★ 125 cited

Sodium-Oxygen anticorrelation among Horizontal Branch Stars in the Globular Cluster M4

A. F Marino, S. Villanova, A. P. Milone +4

The horizontal branch (HB) morphology of globular clusters (GC) is mainly governed by metallicity. The second parameter problem, well known since the 60's, states that metallicity…