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Time-varying phenomena are one of the most substantial sources of astrophysical information, and their study has led to many fundamental discoveries in modern astronomy. We have developed an automated tool to search for and analyze variable sources in the near-infrared K s band using the data fro...


Medina, N.Borissova, J.Bayo, A.Kurtev, R.Navarro Molina, C.Kuhn, M.Kumar, N.Lucas, P.W.Catelan, M.Minniti, D.Smith, L.C.[An Automated Tool to Detect Variable Sources in the Vista Variables in the Vía Láctea Survey: The VVV Variables (V4) Catalog of Tiles d001 and d002]An Automated Tool to Detect Variable Sources in the Vista Variables in the Vía Láctea Survey: The VVV Variables (V4) Catalog of Tiles d001 and d002

Magrini, L.Spina, L.Randich, S.Friel, E.Kordopatis, G.Worley, C.Pancino, E.Bragaglia, A.Donati, P.Tautvaišienė, G.Bagdonas, V.Delgado-Mena, E.Adibekyan, V.Sousa, S.G.Jiménez-Esteban, F.M.Sanna, N.Roccatagliata, V.Bonito, R.Sbordone, L.Duffau, S.Gilmore, G.Feltzing, S.Jeffries, R.D.Vallenari, A.Alfaro, E.J.Bensby, T.Francois, P.Koposov, S.Korn, A.J.Recio-Blanco, A.Smiljanic, R.Bayo, A.Carraro, G.Casey, A.R.Costado, M.T.Damiani, F.Franciosini, E.Frasca, A.Hourihane, A.Jofré, P.De Laverny, P.Lewis, J.Masseron, T.Monaco, L.Morbidelli, L.Prisinzano, L.Sacco, G.Zaggia, S.[The Gaia -ESO Survey: The origin and evolution of s -process elements]The Gaia -ESO Survey: The origin and evolution of s -process elements

This paper is based on observations made with ESO telescopes at the La Silla Paranal Observatory under program ID 092.B-0104(A). We have made extensive use of the SIMBAD Database at CDS (Centre de Données astronomiques) Strasbourg, the NASA/IPAC Extragalactic Database (NED), which is operated by ...


Ivanov, V.D.Piatti, A.E.Beamín, J.-C.Minniti, D.Borissova, J.Kurtev, R.Hempel, M.Saito, R.K.[Candidate star clusters toward the inner Milky Way discovered on deep-stacked KS-band images from the VVV Survey]Candidate star clusters toward the inner Milky Way discovered on deep-stacked KS-band images from the VVV Survey

Delgado, A. J.Sampedro, L.Alfaro, E. J.Costado, M. T.Yun, J. L.Frasca, A.Lanzafame, A. C.Drew, J. E.Eislöffel, J.Blomme, R.Morel, T.Lobel, A.Semaan, T.Randich, S.Jeffries, R. D.Micela, G.Vallenari, A.Kalari, V.Gilmore, G.Flaccomio, E.Carraro, G.Lardo, C.Monaco, L.Prisinzano, L.Sousa, S. G.Morbidelli, L.Lewis, J.Koposov, S.Hourihane, A.Worley, C.Casey, A.Franciosini, E.Sacco, G.Magrini, L.[The Gaia-ESO Survey: pre-main-sequence stars in the young open cluster NGC 3293]The Gaia-ESO Survey: pre-main-sequence stars in the young open cluster NGC 3293

Randich, S.Tognelli, E.Jackson, R.Jeffries, R.D.Degl'Innocenti, S.Pancino, E.Fiorentin, P.R.Spagna, A.Sacco, G.Bragaglia, A.Magrini, L.Moroni, P.G.P.Alfaro, E.Franciosini, E.Morbidelli, L.Roccatagliata, V.Bouy, H.Bravi, L.Jiménez-Esteban, F.M.Jordi, C.Zari, E.Tautvaišiene, G.Drazdauskas, A.Mikolaitis, S.Gilmore, G.Feltzing, S.Vallenari, A.Bensby, T.Koposov, S.Korn, A.Lanzafame, A.Smiljanic, R.Bayo, A.Carraro, G.Costado, M.T.Heiter, U.Hourihane, A.Jofré, P.Lewis, J.Monaco, L.Prisinzano, L.Sbordone, L.Sousa, S.G.Worley, C.C.Zaggia, S.[The Gaia -ESO Survey: Open clusters in Gaia -DR1: A way forward to stellar age calibration]The Gaia -ESO Survey: Open clusters in Gaia -DR1: A way forward to stellar age calibration

We show that non-magnetic models for the evolution of pre-main-sequence (PMS) stars cannot simultaneously describe the colour-magnitude diagram (CMD) and the pattern of lithium depletion seen in the cluster of young, low-mass stars surrounding gamma(2) Velorum. The age of 7.5 +/- 1 Myr inferred f...


Jeffries, RDJackson, RJFranciosini, ERandich, SBarrado, DFrasca, AKlutsch, ALanzafame, ACPrisinzano, LSacco, GGGilmore, GVallenari, AAlfaro, EJKoposov, SEPancino, EBayo, ACasey, ARCostado, MTDamiani, FHourihane, ALewis, JJofre, PMagrini, LMonaco, LMorbidelli, LWorley, CCZaggia, SZwitter, T[The Gaia-ESO Survey: lithium depletion in the Gamma Velorum cluster and inflated radii in low-mass pre-main-sequence stars]The Gaia-ESO Survey: lithium depletion in the Gamma Velorum cluster and inflated radii in low-mass pre-main-sequence stars

Merle, T.Van Eck, S.Jorissen, A.Van Der Swaelmen, M.Masseron, T.Zwitter, T.Hatzidimitriou, D.Klutsch, A.Pourbaix, D.Blomme, R.Worley, C.C.Sacco, G.Lewis, J.Abia, C.Traven, G.Sordo, R.Bragaglia, A.Smiljanic, R.Pancino, E.Damiani, F.Hourihane, A.Gilmore, G.Randich, S.Koposov, S.Casey, A.Morbidelli, L.Franciosini, E.Magrini, L.Jofre, P.Costado, M.T.Jeffries, R.D.Bergemann, M.Lanzafame, A.C.Bayo, A.Carraro, G.Flaccomio, E.Monaco, L.Zaggia, S.[The Gaia -ESO Survey: Double-, triple-, and quadruple-line spectroscopic binary candidates]The Gaia -ESO Survey: Double-, triple-, and quadruple-line spectroscopic binary candidates

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