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20042026
most citedVVV DR1: The First Data Release of the Milky Way Bulge and Southern Plane from the Near-Infrared ESO Public Survey VISTA Variables in the Via Lactea

409 citations · 4.9k across the 94 of their papers we have counts for

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astro-ph.GA2011★ 409 cited

VVV DR1: The First Data Release of the Milky Way Bulge and Southern Plane from the Near-Infrared ESO Public Survey VISTA Variables in the Via Lactea

R. K. Saito, M. Hempel, D. Minniti +107

The ESO Public Survey VISTA Variables in the Via Lactea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for…

astro-ph.GA2011★ 83 cited

The inner Galactic bar traced by the VVV survey

O. A. Gonzalez, M. Rejkuba, D. Minniti +3

We use the VVV survey observations in bulge regions close to the Galactic plane to trace the bar inclination at the Galactic latitude b\sim\pm1° and to investigate a distinct struc…

astro-ph.GA2011★ 71 cited

Three Galactic globular cluster candidates

C. Moni Bidin, F. Mauro, D. Geisler +12

The census of Galactic globular clusters (GCs) is still incomplete, and about ten new objects are supposed to await discovery, hidden behind the crowded and reddened regions of the…

astro-ph.IM2011★ 17 cited

MAD about the Large Magellanic Cloud: preparing for the era of Extremely Large Telescopes

G. Fiorentino, E. Tolstoy, E. Diolaiti +3

We present J, H, Ks photometry from the the Multi conjugate Adaptive optics Demonstrator (MAD), a visitor instrument at the VLT, of a resolved stellar population in a small crowded…

astro-ph.GA2011★ 127 cited

Reddening and metallicity maps of the Milky Way Bulge from VVV and 2MASS. I.The method and minor axis maps

O. A. Gonzalez, M. Rejkuba, M. Zoccali +2

We present a method to obtain reddening maps and to trace structure and metallicity gradients of the bulge using data from the recently started ESO public survey Vista Variables in…

astro-ph.GA2011★ 38 cited

Massive stars in the Cl 1813-178 Cluster. An episode of massive star formation in the W33 complex

Maria Messineo, Ben Davies, Donald F. Figer +5

Young massive (M >10^4 Msun) stellar clusters are a good laboratory to study the evolution of massive stars. Only a dozen of such clusters are known in the Galaxy. Here we report a…