activity
20092025
most citedVISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way

1k citations · 6k across the 70 of their papers we have counts for

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astro-ph.SR2019★ 34 cited

First stellar spectroscopy in Leo P

C. J. Evans, N. Castro, O. A. Gonzalez +11

We present the first stellar spectroscopy in the low-luminosity (M_V ~-9.3 mag), dwarf galaxy Leo P. Its significantly low oxygen abundance (3% solar) and relative proximity (~1.6…

astro-ph.SR2018★ 4 cited

unVEil the darknesS of The gAlactic buLgE (VESTALE)

G. Bono, M. Dall'Ora, M. Fabrizio +55

The main aim of this experiment is to provide a complete census of old (t > 10 Gyr, RR Lyrae, type II Cepheids, red horizontal branch), intermediate age (red clump, Miras) and youn…

astro-ph.SR2018★ 29 cited

Oxygen and zinc abundances in 417 Galactic bulge red giants

C. R. da Silveira, B. Barbuy, A. C. S. Friaça +7

Oxygen and zinc in the Galactic bulge are key elements for the understanding of the bulge chemical evolution. Oxygen-to-iron abundance ratios provide a most robust indicator of the…

astro-ph.SR2017★ 35 cited

Galactic Bulge Population II Cepheids in the VVV Survey: Period-Luminosity Relations and a Distance to the Galactic Center

A. Bhardwaj, M. Rejkuba, D. Minniti +7

We present the near-infrared observations of population II Cepheids in the Galactic bulge from VVV survey. We identify 340 population II Cepheids in the Galactic bulge from VVV sur…

astro-ph.SR2015★ 131 cited

Interstellar Extinction Curve Variations Toward the Inner Milky Way: A Challenge to Observational Cosmology

David M. Nataf, Oscar A. Gonzalez, Luca Casagrande +18

We investigate interstellar extinction curve variations toward 4 deg of the inner Milky Way in photometry from the OGLE-III and surveys, with supportin…

astro-ph.SR2015★ 2 cited

Making FORS2 fit for exoplanet observations (again)

H. M. J. Boffin, G. Blanchard, O. A. Gonzalez +10

For about three years, it was known that precision spectrophotometry with FORS2 suffered from systematic errors that made quantitative observations of planetary transits impossible…