The Vista Variables in the Vía Láctea (VVV) ESO Public Survey: Current Status and First Results
dc.catalogador | pau | |
dc.contributor.author | Catelan, Marcio | |
dc.contributor.author | Minniti, D. | |
dc.contributor.author | Lucas, P. W. | |
dc.contributor.author | Alonso-García, J. | |
dc.contributor.author | Angeloni, R. | |
dc.contributor.author | Beamín, J. C. | |
dc.contributor.author | Bonatto, C. | |
dc.contributor.author | Borissova, J. | |
dc.contributor.author | Contreras, C. | |
dc.contributor.author | Cross, N. | |
dc.contributor.author | Dékáany, I. | |
dc.contributor.author | Emerson, J. P. | |
dc.contributor.author | Eyheramendy, S. | |
dc.contributor.author | Geisler, D. | |
dc.contributor.author | González-Solares, E. | |
dc.contributor.author | Helminiak, K. G. | |
dc.contributor.author | Hempel, M. | |
dc.contributor.author | Irwin, M. J. | |
dc.contributor.author | Ivanov, V. D. | |
dc.contributor.author | Jordán, A. | |
dc.contributor.author | Kerins, E. | |
dc.contributor.author | Kurtev, R. | |
dc.contributor.author | Mauro, F. | |
dc.contributor.author | Moni Bidin, C. | |
dc.contributor.author | Navarrete, C. | |
dc.contributor.author | Pérez, P. | |
dc.contributor.author | Pichara, K. | |
dc.contributor.author | Read, M. | |
dc.contributor.author | Rejkuba, M. | |
dc.contributor.author | Saito, R. K. | |
dc.contributor.author | Sale, S. E. | |
dc.contributor.author | Toledo, I. | |
dc.date.accessioned | 2024-03-05T15:15:05Z | |
dc.date.available | 2024-03-05T15:15:05Z | |
dc.date.issued | 2011 | |
dc.description.abstract | 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.... | |
dc.fuente.origen | ORCID | |
dc.identifier.uri | https://inspirehep.net/literature/898612 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/84106 | |
dc.information.autoruc | Instituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556 | |
dc.language.iso | en | |
dc.nota.acceso | contenido parcial | |
dc.rights | acceso restringido | |
dc.title | The Vista Variables in the Vía Láctea (VVV) ESO Public Survey: Current Status and First Results | |
dc.type | comunicación de congreso | |
sipa.codpersvinculados | 1001556 | |
sipa.trazabilidad | ORCID;2024-01-22 |