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20012021
most citedPhysical parameters of 15 intermediate-age LMC clusters from modelling of HST colour-magnitude diagrams

71 citations · 204 across the 7 of their papers we have counts for

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7 papers

astro-ph.SR2021★ 21 cited

On the Use of Field RR Lyrae as Galactic Probes. V. Optical and radial velocity curve templates

V. F. Braga, J. Crestani, M. Fabrizio +29

We collected the largest spectroscopic catalog of RR Lyrae (RRLs) including 20,000 high-, medium- and low-resolution spectra for 10,000 RRLs. We provide the analy…

astro-ph.SR2020★ 56 cited

On the Use of Field RR Lyrae as Galactic Probes. II. A new S calibration to estimate their metallicity

J. Crestani, M. Fabrizio, V. F. Braga +33

We performed the largest and most homogeneous spectroscopic survey of field RR Lyraes (RRLs). We secured 6,300 high resolution (HR, R35,000) spectra for 143 RRLs (11…

astro-ph.SR2016★ 20 cited

Massive open star clusters using the VVV survey V. Young clusters with an OB stellar population

S. Ramírez Alegría, J. Borissova, A. -N. Chené +6

The ESO public survey VISTA Variables in the Vía Láctea (VVV) has contributed with deep multi-epoch photometry of the Galactic bulge and the adjacent part of the disk over 526 squa…

astro-ph2006★ 71 cited

Physical parameters of 15 intermediate-age LMC clusters from modelling of HST colour-magnitude diagrams

L. O. Kerber, B. X. Santiago, E. Brocato

We analyzed HST/WFPC2 colour-magnitude diagrams (CMDs) of 15 populous Large Magellanic Cloud (LMC) stellar clusters with ages between ~ 0.3 Gyr and ~ 3 Gyr. These (V, B-V) CMDs are…

astro-ph2006★ 21 cited

Mass segregation in rich LMC clusters from modelling of deep HST colour-magnitude diagrams

L. O. Kerber, B. X. Santiago

We used the deep colour-magnitude diagrams (CMDs) of five rich LMC clusters (NGC1805, 1818, 1831, 1868, and Hodge14) observed with HST/WFPC2 to derive their present day mass functi…

astro-ph2003★ 15 cited

The Relationship Between the Sersic Law Profiles Measured Along the Major and Minor Axes of Elliptical Galaxies

Fabricio Ferrari, Horacio Dottori, Nicola Caon +2

In this paper we discuss the reason why the parameters of the Sersic model best-fitting the major axis light profile of elliptical galaxies can differ significantly from those deri…