Browsing by Author "Pérez, P."

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    Protective mechanisms of S. lycopersicum aqueous fraction (Nucleosides and Flavonoids) on platelet activation and thrombus formation: In vitro, ex vivo and in vivo studies
    (2013) Pereira Garcés, Jaime Ignacio; Fuentes, E.; Alarcón, M.; Valenzuela, C.; Pérez, P.; Astudillo, L.; Palomo, I.
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    The optimal windows for seismically-enhanced gold precipitation in the epithermal environment
    (2016) Sánchez, P.; Reich, M.; Driesner, T.; Cembrano, José; Arancibia Hernández, Gloria Cecilia; Pérez, P.; Heinrich, C.; Rowland, J.; Tardani, D.; Lange, D.; Campos, E.
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    The Vista Variables in the Vía Láctea (VVV) ESO Public Survey: Current Status and First Results
    (2011) Catelan, Marcio; Minniti, D.; Lucas, P. W.; Alonso-García, J.; Angeloni, R.; Beamín, J. C.; Bonatto, C.; Borissova, J.; Contreras, C.; Cross, N.; Dékáany, I.; Emerson, J. P.; Eyheramendy, S.; Geisler, D.; González-Solares, E.; Helminiak, K. G.; Hempel, M.; Irwin, M. J.; Ivanov, V. D.; Jordán, A.; Kerins, E.; Kurtev, R.; Mauro, F.; Moni Bidin, C.; Navarrete, C.; Pérez, P.; Pichara, K.; Read, M.; Rejkuba, M.; Saito, R. K.; Sale, S. E.; Toledo, I.
    Vista Variables in the Vía Láctea (VVV) is an ESO Public Survey that is performing a variability survey of the Galactic bulge and part of the inner disk using ESO's Visible and Infrared Survey Telescope for Astronomy (VISTA). The survey covers 520 { deg}^2 of sky area in the ZYJHK_S filters, for a total observing time of 1929 hours, including ∼ 10^9 point sources and an estimated ∼ 10^6 variable stars. Here we describe the current status of the VVV Survey, in addition to a variety of new results based on VVV data, including light curves for variable stars, newly discovered globular clusters, open clusters, and associations. A set of reddening-free indices based on the ZYJHK_S system is also introduced. Finally, we provide an overview of the VVV Templates Project, whose main goal is to derive well-defined light curve templates in the near-IR, for the automated classification of VVV light curves....