activity
20132024
most citedThe GIRAFFE Inner Bulge Survey (GIBS) III. Metallicity distributions and kinematics of 26 Galactic bulge fields

160 citations · 691 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2024★ 38 cited

The VISTA Variables in the Vía Láctea eXtended (VVVX) ESO public survey: Completion of the observations and legacy

R. K. Saito, M. Hempel, J. Alonso-García +143

The ESO public survey VISTA Variables in the Vía Láctea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from . Upon its conclusion, the c…

astro-ph.GA2016★ 160 cited

The GIRAFFE Inner Bulge Survey (GIBS) III. Metallicity distributions and kinematics of 26 Galactic bulge fields

M. Zoccali, S. Vasquez, O. A. Gonzalez +9

Several recent studies have demonstrated that the Galactic bulge hosts two components with different mean metallicities, and possibly different spatial distribution and kinematics.…

astro-ph.GA2016★ 98 cited

FORS2/VLT survey of Milky Way globular clusters II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale

Bruno Dias, Beatriz Barbuy, Ivo Saviane +5

(ABRIDGED) Globular clusters trace the formation and evolution of the Milky Way and surrounding galaxies, and outline their chemical enrichment history. To accomplish these tasks i…

astro-ph.SR2016★ 15 cited

High resolution spectroscopic analysis of seven giants in the bulge globular cluster NGC 6723

A. Rojas-Arriagada, M. Zoccali, S. Vásquez +5

Globular clusters associated with the Galactic bulge are important tracers of stellar populations in the inner Galaxy. High resolution analysis of stars in these clusters allows us…

astro-ph.GA2015★ 69 cited

The Giraffe Inner Bulge Survey (GIBS) II. Metallicity distributions and alpha element abundances at fixed Galactic latitude

O. A. Gonzalez, M. Zoccali, S. Vasquez +8

High resolution (R22,500) spectra for 400 red clump giants, in four fields within and $\rm -10^{\circ} \lesssim l \lesssim…

astro-ph.GA2015★ 35 cited

The Calcium Triplet metallicity calibration for galactic bulge stars

S. Vasquez, M. Zoccali, V. Hill +4

We present a new calibration of the Calcium II Triplet equivalent widths versus [Fe/H], constructed upon K giant stars in the Galactic bulge. This calibration will be used to deriv…

astro-ph.SR2015★ 9 cited

Chemical Abundances of the Highly Obscured Galactic Globular Clusters 2MASS GC02 and Mercer 5

Francisco Penaloza, Peter Pessev, Sergio Vasquez +3

We present the first high spectral resolution abundance analysis of two newly discovered Galactic globular clusters, namely Mercer 5 and 2MASS GC02 residing in regions of high inte…

astro-ph.GA2014★ 35 cited

FORS2/VLT survey of Milky Way globular clusters I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426 and Terzan 8

Bruno Dias, Beatriz Barbuy, Ivo Saviane +6

(abridged) We have observed almost 1/3 of the globular clusters in the Milky Way, targeting distant and/or highly reddened objects, besides a few reference clusters. A large sample…

astro-ph.GA2014★ 143 cited

The GIRAFFE Inner Bulge Survey (GIBS). I. Survey Description and a kinematical map of the Milky Way bulge

M. Zoccali, O. A. Gonzalez, S. Vasquez +10

The Galactic bulge is a massive, old component of the Milky Way. It is known to host a bar, and it has recently been demonstrated to have a pronounced boxy/peanut structure in its…

astro-ph.SR2013★ 34 cited

Deriving Metallicities from Calcium Triplet Spectroscopy in combination with Near Infrared Photometry

F. Mauro, C. Moni Bidin, D. Geisler +7

Context. [...] One of the most efficient methods is the measurement of the equivalent width (EW) of the Calcium II Triplet (CaT), corrected for the luminosity and temperature effec…

astro-ph.GA2013★ 55 cited

3D kinematics through the X-shaped Milky Way bulge

S. Vásquez, M. Zoccali, V. Hill +10

It has recently been discovered that the Galactic bulge is X-shaped, with the two southern arms of the X both crossing the lines of sight at l=0 and |b|>4, hence producing a double…