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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

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

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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