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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?

Context. Globular clusters are known to host multiple stellar populations, which are a signature of their formation process. The globular cluster E3 is one of the few low-mass globulars that is thought not to host multiple populations. Aims. We investigate red giant branch stars in E3 with the ai...


Monaco, L.Villanova, S.Carraro, G.Mucciarelli, A.Moni Bidin, C.[Chemical abundance analysis of red giant branch stars in the globular cluster E3]Chemical abundance analysis of red giant branch stars in the globular cluster E3

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

A.R.B., P.d.L., and V.H. acknowledge financial support form the ANR 14-CE33-014-01. This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell'Is...


Recio-Blanco, A.Rojas-Arriagada, A.de Laverny, P.Mikolaitis, S.Hill, V.Zoccali, M.Fernández-Trincado, J. G.Robin, A. C.Babusiaux, C.Gilmore, G.Randich, S.Alfaro, E.C., Allende PrietoBragaglia, A.Carraro, G.Jofré, P.Lardo, C.Monaco, L.Morbidelli, L.Zaggia, S.[The Gaia-ESO Survey: Low-α element stars in the Galactic bulge]The Gaia-ESO Survey: Low-α element stars in the Galactic bulge

Aims. We present observations from the Gaia-ESO Survey in the lines of Hα, [N II], [S II], and He I of nebular emission in the central part of the Carina nebula. Methods. We investigate the properties of the two already known kinematic components (approaching and receding), which account for the ...


Damiani, F.Bonito, R.Magrini, L.Prisinzano, L.Mapelli, M.Micela, G.Kalari, V.Maíz Apellániz, J.Gilmore, G.Randich, S.Alfaro, E.Flaccomio, E.Koposov, S.Klutsch, A.Lanzafame, A. C.Pancino, E.Sacco, G. G.Bayo, A.Carraro, G.Casey, A. R.Costado, M. T.Franciosini, E.Hourihane, A.Lardo, C.Lewis, J.Monaco, L.Morbidelli, L.Worley, C.Zaggia, S.Zwitter, T.Dorda, R.[Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines]Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines

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

Aims. The present study was conducted to determine the optical extinction curve for Cerro Paranal under typical clear-sky observing conditions, with the purpose of providing the community with a function to be used to correct the observed spectra, with an accuracy of 0.01 mag airmass􀀀1. Addition...


Patat, F.Moehler, S.O’Brien, K.Pompei, E.Bensby, T.Carraro, G.de Ugarte Postigo, A.Fox, A.Gavignaud, I.James, G.Korhonen, H.Ledoux, C.Randall, S.Sana, H.Smoker, J.Stefl, S.Szeifert, T.[Optical atmospheric extinction over Cerro Paranal]Optical atmospheric extinction over Cerro Paranal

Context. Rapidly rotating, low-mass members of eclipsing binary systems have measured radii that are significantly larger than predicted by standard evolutionary models. It has been proposed that magnetic activity is responsible for this radius inflation. Aims. By estimating the radii of low-ma...


Jackson, R. J.Jeffries, R. D.Randich, S.Bragaglia, A.Carraro, G.Costado, M. T.Flaccomio, E.Lanzafame, A. C.Lardo, C.Monaco, L.Morbidelli, L.Smiljanic, R.Zaggia, S.[The Gaia-ESO Survey: Stellar radii in the young open clusters NGC 2264, NGC 2547, and NGC 2516]The Gaia-ESO Survey: Stellar radii in the young open clusters NGC 2264, NGC 2547, and NGC 2516

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