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Bertelli Motta, C.Pasquali, A.Richer, J.Michaud, G.Salaris, M.Bragaglia, A.Magrini, L.Randich, S.Grebel, E.K.Adibekyan, V.Blanco-Cuaresma, S.Drazdauskas, A.Fu, X.Martell, S.Tautvaišiene, G.Gilmore, G.Alfaro, E.J.Bensby, T.Flaccomio, E.Koposov, S.E.Korn, A.J.Lanzafame, A.C.Smiljanic, R.Bayo, A.Carraro, G.Casey, A.R.Costado, M.T.Damiani, F.Franciosini, E.Heiter, U.Hourihane, A.Jofré, P.Lardo, C.Lewis, J.Monaco, L.Morbidelli, L.Sacco, G.G.Sousa, S.G.Worley, C.C.Zaggia, S.[The Gaia-ESO Survey: Evidence of atomic diffusion in M67?]The Gaia-ESO Survey: Evidence of atomic diffusion in M67?

Smiljanic, R.Franciosini, E.Bragaglia, A.Tautvaišiene, G.Fu, X.Pancino, E.Adibekyan, V.Sousa, S.G.Randich, S.Montalbán, J.Pasquini, L.Magrini, L.Drazdauskas, A.García, R.A.Mathur, S.Mosser, B.Régulo, C.De Assis Peralta, R.Hekker, S.Feuillet, D.Valentini, M.Morel, T.Martell, S.Gilmore, G.Feltzing, S.Vallenari, A.Bensby, T.Korn, A.J.Lanzafame, A.C.Recio-Blanco, A.Bayo, A.Carraro, G.Costado, M.T.Frasca, A.Jofré, P.Lardo, C.De Laverny, P.Lind, K.Masseron, T.Monaco, L.Morbidelli, L.Prisinzano, L.Sbordone, L.Zaggia, S.[The Gaia -ESO Survey: Properties of newly discovered Li-rich giants]The Gaia -ESO Survey: Properties of newly discovered Li-rich giants

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

Casey, A. R.Ruchti, G.Masseron, T.Randich, S.Gilmore, G.Lind, K.Kennedy, G. M.Koposov, S. E.Hourihane, A.Franciosini, E.Lewis, J. R.Magrini, L.Morbidelli, L.Sacco, G. G.Worley, C. C.Feltzing, S.Jeffries, R. D.Vallenari, A.Bensby, T.Bragaglia, A.Flaccomio, E.Francois, P.Korn, A. J.Lanzafame, A.Pancino, E.Recio-Blanco, A.Smiljanic, R.Carraro, G.Costado, M. T.Damiani, F.Donati, P.Frasca, A.Jofre, P.Lardo, C.de Laverny, P.Monaco, L.Prisinzano, L.Sbordone, L.Sousa, S. G.Tautvaisien, G.Zaggia, S.Zwitter, T.Delgado Mena, E.Chorniy, Y.Martell, S. L.Silva Aguirre, V.Miglio, A.Chiappini, C.Montalban, J.Morel, T.Valentini, M.[The Gaia-ESO Survey: revisiting the Li-rich giant problem]The Gaia-ESO Survey: revisiting the Li-rich giant problem

The Gaia-ESO Survey was designed to target all major Galactic components (i.e. bulge, thin and thick discs, halo and clusters), with the goal of constraining the chemical and dynamical evolution of the Milky Way. This paper presents the methodology and considerations that drive the selection of t...


Stonkutė, E.Koposov, S. E.Howes, L. M.Feltzing, S.Worley, C. C.Gilmore, G.Ruchti, G. R.Kordopatis, G.Randich, S.Zwitter, T.Bensby, T.Bragaglia, A.Smiljanic, R.Costado, M. T.Tautvaišienė, G.Casey, A. R.Korn, A. J.Lanzafame, A. C.Pancino, E.Franciosini, E.Hourihane, A.Jofré, P.Lardo, C.Lewis, J.Magrini, L.Monaco, L.Morbidelli, L.Sacco, G. G.Sbordone, L.[The Gaia-ESO Survey: the selection function of the Milky Way field stars]The Gaia-ESO Survey: the selection function of the Milky Way field stars

We analyze the kinematics of similar to 2000 giant stars in the direction of the Galactic bulge, extracted from the Gaia-ESO survey in the region -10 degrees less than or similar to l less than or similar to 10 degrees and -11 degrees less than or similar to b less than or similar to -3 degrees. ...


Williams, Angus A.Evans, N. W.Molloy, MatthewKordopatis, GeorgesSmith, M. C.Shen, J.Gilmore, G.Randich, S.Bensby, T.Francois, P.Koposov, S.E.Recio-Blanco, A.Bayo, A.Carraro, G.Casey, A.Costado, T.Franciosini, E.Hourihane, A.de Laverny, P.Lewis, J.Lind, K.Magrini, L.Monaco, L.Morbidelli, L.Sacco, G. GWorley, C.Zaggia, S.Mikolaitis, Š.[THE GAIA-ESO SURVEY: METAL-RICH BANANAS IN THE BULGE]THE GAIA-ESO SURVEY: METAL-RICH BANANAS IN THE BULGE

Smiljanic, R.Franciosini, E.Randich, S.Magrini, L.Bragaglia, A.Pasquini, L.Vallenari, A.Tautvaišienė, G.Biazzo, K.Frasca, A.Donati, P.Delgado Mena, E.Casey, A. R.Geisler, D.Villanova, S.Tang, B.Sousa, S. G.Gilmore, G.Bensby, T.François, P.Koposov, S. E.Lanzafame, A. C.Pancino, E.Recio-Blanco, A.Costado, M. T.Hourihane, A.Lardo, C.de Laverny, P.Lewis, J.Monaco, L.Morbidelli, L.Sacco, G. G.Worley, C. C.Zaggia, S.Martell, S.[The Gaia-ESO Survey: Inhibited extra mixing in two giants of the open cluster Trumpler 20?]The Gaia-ESO Survey: Inhibited extra mixing in two giants of the open cluster Trumpler 20?

Rojas-Arriagada, A.Recio-Blanco, A.de Laverny, P.Schultheis, M.Guiglion, G.Mikolaitis, Š.Kordopatis, G.Hill, V.Gilmore, G.Randich, S.Alfaro, E. J.Bensby, T.Koposov, S. E.Costado, M. T.Franciosini, E.Hourihane, A.Jofré, P.Lardo, C.Lewis, J.Lind, K.Magrini, L.Monaco, L.Morbidelli, L.Sacco, G. G.Worley, C. C.Zaggia, S.Chiappini, C.[The Gaia-ESO Survey: Separating disk chemical substructures with cluster models⋆ Evidence of a separate evolution in the metal-poor thin disk]The Gaia-ESO Survey: Separating disk chemical substructures with cluster models⋆ Evidence of a separate evolution in the metal-poor thin disk

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

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