activity
20172021
most citedMapping the stellar age of the Milky Way bulge with the VVV. I. The method

43 citations · 138 across the 7 of their papers we have counts for

collaborators

14 papers

astro-ph.GA202112 cited

The diffuse interstellar band around 8620 Å II. Kinematics and distance of the DIB carrier

H. Zhao, M. Schultheis, A. Rojas-Arriagada +4

We aim to make use of the measurements from the Giraffe Inner Bulge Survey (GIBS) and the GaiaESO survey (GES) to study the kinematics and distance of the carrier of DIB862…

astro-ph.GA202112 cited

A new distance to the Brick, the dense molecular cloud G0.253+0.016

M. Zoccali, E. Valenti, F. Surot +3

We analyse the near infrared colour magnitude diagram of a field including the giant molecular cloud G0.253+0.016 (a.k.a. The Brick) observed at high spatial resolution, with HAWK-…

astro-ph.GA202016 cited

The diffuse interstellar band around 8620 Å I. Methods and application to the GIBS data set

H. Zhao, M. Schultheis, A. Recio-Blanco +6

We developed a set of procedures to automatically detect and measure the DIB around 8620 Å (the Gaia DIB) for a wide range of temperatures. The DIB profile is fit with a Gaussian f…

astro-ph.SR20202 cited

A hundred new eclipsing binary system candidates studied in a near-infrared window in the VVV survey

L. V. Gramajo, T. Palma, D. Minniti +4

We present the first results obtained from an extensive study of eclipsing binary (EB) system candidates recently detected in the VISTA Variables in the Vía Láctea (VVV) near-infra…

astro-ph.GA2020

Mapping the stellar age of the Milky Way bulge with the VVV. III. High resolution reddening map

F. Surot, E. Valenti, O. A. Gonzalez +4

The detailed study of the Galactic bulge stellar population necessarily requires an accurate representation of the interstellar extinction particularly toward the Galactic plane an…

astro-ph.GA2020

VVVX-Gaia Discovery of a Low Luminosity Globular Cluster in the Milky Way Disk

E. R. Garro, D. Minniti, M. Gómez +20

Milky Way globular clusters (MW GCs) are difficult to identify at low Galactic latitudes because of high differential extinction and heavy star crowding. The new deep near-IR image…