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Schiappacasse-Ulloa, J.Tang, B.Fernández-Trincado, J.G.Zamora, O.Geisler, D.Frinchaboy, P.Schultheis, M.Dell'Agli, F.Villanova, S.Masseron, T.Mészáros, S.Souto, D.Hasselquist, S.Cunha, K.Smith, V.V.García-Hernández, D.A.Vieira, K.Robin, A.C.Minniti, D.Zasowski, G.Moreno, E.Pérez-Villegas, A.Lane, R.R.Ivans, I.I.Pan, K.Nitschelm, C.Santana, F.A.Carrera, R.Roman-Lopes, A.[A Chemical and Kinematical Analysis of the Intermediate-age Open Cluster IC 166 from APOGEE and Gaia DR2]A Chemical and Kinematical Analysis of the Intermediate-age Open Cluster IC 166 from APOGEE and Gaia DR2

Villanova, S.Randich, S.Geisler, D.Carraro, GiovanniCosta Hechenleitner, Edgardo[The metallicity of the open cluster Tombaugh 2*]

Hamuy Wackenhut, MarioPhillips, M. M.Suntzeff, Nicholas B.Schommer, R. A.Maza Sancho, JoséAntenaza, RobertoWischnjewsky, MarinaValladares, GeraldoMuena, CésarGonzález, L. E.Avilés, R.Wells, LisaSmith, R. C.Navarrete, MauricioCovarrubias, RicardoWilliger, G.Walker, Alistair R.Layden, A. C.Elias, J. H.Baldwin, J. A.Hernández, ManuelTirado, HernánUgarte, PatricioElston, R.Saavedra, NelsonBarrientos, FelipeCosta Hechenleitner, EdgardoLira Teillery, PaulinaRuiz González, María TeresaAnguita, ClaudioGómez, XimenaOrtiz, P.Della Valle, M.Danziger, J.Storm, J.Kim, Y. C.Bailyn, C.Rubenstein, Eric P.Tucker, D.Cersosimo, S.Méndez Bussard, René AlejandroSiciliano, L.Sherry, W.Chaboyer, BrianKoopmann, R. A.Geisler, D.Sarajedini, A.Dey, ArjunTyson, N.Rich, R. MichaelGal, R.Lamontagne, RobertCaldwell, N.Guhathakurta, PuragraPhillips, A. C.Szkody, P.Prosser, C.Ho, Luis C.McMahan, R.Baggley, G.Cheng, K. P.Havlen, R.Wakamatsu, K.Janes, Kenneth A.Malkan, MathewBaganoff, F.Seitzer, P.Shara, M.Sturch, C.Hesser, J.Hartigan, P.Hughes, J.Welch, D. L.Williams, T. B.Ferguson, H.Francis, P. J.French, L.Bolte, M.Roth, J.Odewahn, S.Howell, S.Krzeminski, W.[BVRI light curves for 29 type Ia supernovae]
Autor: Saito, R. K. Hempel, M. Minniti, D. Lucas, P. W. Rejkuba, M. Toledo, I. Gonzalez, O. A. Alonso-García, J. Irwin, M. Gonzalez-Solares, E. Hodgkin, S. T. Lewis, J. R. Cross, N. Ivanov, V. D. Kerins, E. Emerson, J. P. Soto, M. Amôres, E. B. Gurovich, S. Dékány, I. Angeloni, R. Beamin, J. C. Catelan, M. Padilla, N. Zoccali, M. Pietrukowicz, P. Moni Bidin, C. Mauro, F. Geisler, D. Folkes, S. L. Sale, S. E. Borissova, J. Kurtev, R. Ahumada, A. V. Alonso, M. V. Adamson, A. Arias, J. I. Bandyopadhyay, R. M. Barbá, R. H. Barbuy, B. Baume, G. L. Bedin, L. R. Bellini, A. Benjamin, R. Bica, E. Bonatto, C. Bronfman Aguiló, Leonardo Carraro, Giovanni Chenè, A. N. Clariá, J. J. Clarke, J. R. A. Contreras, C. Corvillón, A. Grijs, R. de Dias, B. Drew, J. E. Fariña, C. Feinstein, C. Fernández Lajús, E. Gamen, R. Gieren, W. Goldman, B. González-Fernández, C. Grand, R. J. J. Gunthardt, G. Hambly, N. C. Hanson, M. M. Helminiak, K. G. Hoare, M. G. Huckvale, L. Jordán, A. Kinemuch, K. Longmore, A. López Corredoira, M. Maccarone, T. Majaess, D. Martín, E. L. Masetti, N. Mennickent, R. E. Mirabel, I. F. Monaco, L. Morelli, L. Motta, V. Palma, T. Parisi, M. C. Parker, Q. Peñaloza, F. Pietrzynski, G. Pignata Libralato, Giuliano Popescu, B. Read, M. A. Rojas, A. Roman-Lopes, A. Ruiz González, María Teresa Saviane, I. Schreiber, M. R. Schröder, A. C. Sharma, S. Smith, M. D. Sodré Jr., L. Stead, J. Stephens, A. W. Tamura, M. Tappert, C. Thompson, M. A. Valenti, E. Vanzi, L. Walton, N. A. Weidmann, W. Zijlstr, A.

Saito, R. K.Hempel, M.Minniti, D.Lucas, P. W.Rejkuba, M.Toledo, I.Gonzalez, O. A.Alonso-García, J.Irwin, M.Gonzalez-Solares, E.Hodgkin, S. T.Lewis, J. R.Cross, N.Ivanov, V. D.Kerins, E.Emerson, J. P.Soto, M.Amôres, E. B.Gurovich, S.Dékány, I.Angeloni, R.Beamin, J. C.Catelan, M.Padilla, N.Zoccali, M.Pietrukowicz, P.Moni Bidin, C.Mauro, F.Geisler, D.Folkes, S. L.Sale, S. E.Borissova, J.Kurtev, R.Ahumada, A. V.Alonso, M. V.Adamson, A.Arias, J. I.Bandyopadhyay, R. M.Barbá, R. H.Barbuy, B.Baume, G. L.Bedin, L. R.Bellini, A.Benjamin, R.Bica, E.Bonatto, C.Bronfman Aguiló, LeonardoCarraro, GiovanniChenè, A. N.Clariá, J. J.Clarke, J. R. A.Contreras, C.Corvillón, A.Grijs, R. deDias, B.Drew, J. E.Fariña, C.Feinstein, C.Fernández Lajús, E.Gamen, R.Gieren, W.Goldman, B.González-Fernández, C.Grand, R. J. J.Gunthardt, G.Hambly, N. C.Hanson, M. M.Helminiak, K. G.Hoare, M. G.Huckvale, L.Jordán, A.Kinemuch, K.Longmore, A.López Corredoira, M.Maccarone, T.Majaess, D.Martín, E. L.Masetti, N.Mennickent, R. E.Mirabel, I. F.Monaco, L.Morelli, L.Motta, V.Palma, T.Parisi, M. C.Parker, Q.Peñaloza, F.Pietrzynski, G.Pignata Libralato, GiulianoPopescu, B.Read, M. A.Rojas, A.Roman-Lopes, A.Ruiz González, María TeresaSaviane, I.Schreiber, M. R.Schröder, A. C.Sharma, S.Smith, M. D.Sodré Jr., L.Stead, J.Stephens, A. W.Tamura, M.Tappert, C.Thompson, M. A.Valenti, E.Vanzi, L.Walton, N. A.Weidmann, W.Zijlstr, A.[VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Via Lactea]

Villanova, S.Randich, S.Geisler, D.Carraro, GiovanniCosta Hechenleitner, Edgardo[The metallicity of the open cluster Tombaugh 2]

Hamuy Wackenhut, MarioPhillips, M. M.Suntzeff, Nicholas B.Schommer, R. A.Maza Sancho, JoséAntenaza, RobertoWischnjewsky, MarinaValladares, GeraldoMuena, CésarGonzález, L. E.Avilés, R.Wells, LisaSmith, R. C.Navarrete, MauricioCovarrubias, RicardoWilliger, G.Walker, Alistair R.Layden, A. C.Elias, J. H.Baldwin, J. A.Hernández, ManuelTirado, HernánUgarte, PatricioElston, R.Saavedra, NelsonBarrientos, FelipeCosta Hechenleitner, EdgardoLira Teillery, PaulinaRuiz González, María TeresaAnguita, ClaudioGómez, XimenaOrtiz Arce, PatricioDella Valle, MassimoDanziger, J.Storm, J.Kim, Y. C.Bailyn, C.Rubenstein, Eric P.Tucker, D.Cersosimo, S.Méndez, R. A.Siciliano, L.Sherry, W.Chaboyer, BrianKoopmann, R. A.Geisler, D.Sarajedini, A.Dey, ArjunTyson, N.Rich, R. MichaelGal, R.Lamontagne, RobertCaldwell, N.Guhathakurta, PuragraPhillips, A. C.Szkody, P.Prosser, C.Ho, Luis C.McMahan, R.Baggley, G.Cheng, K. P.Havlen, R.Wakamatsu, K.Janes, Kenneth A.Malkan, MathewBaganoff, F.Seitzer, P.Shara, M.Sturch, C.Hesser, J.Hartigan, P.Hughes, J.Welch, D. L.Williams, T. B.Ferguson, H.Francis, P. J.French, L.Bolte, M.Roth, J.Odewahn, S.Howell, S.Krzeminski, W.[BVRI light curves for 29 type Ia supernovae]

Context. Low-mass dwarf spheroidal galaxies are key objects for our understanding of the chemical evolution of the pristine Universe and the Local Group of galaxies. Abundance ratios in stars of these objects can be used to better understand their star formation and chemical evolution. Aims. We r...


François, P.Monaco, L.Bonifacio, P.Moni Bidin, C.Geisler, D.[Abundance ratios of red giants in low-mass ultra-faint dwarf spheroidal galaxies]Abundance ratios of red giants in low-mass ultra-faint dwarf spheroidal galaxies

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?

NGC 6791 is a unique stellar cluster, key to our understanding of both the multiple stellar population phenomenon and the evolution and assembly of the Galaxy. However, despite many investigations, its nature is still very controversial. Geisler et al. found evidence suggesting that it was the fi...


Villanova, S.Carraro, G.Geisler, D.Monaco, L.Assmann, P.[NGC 6791: A Probable Bulge Cluster without Multiple Populations]NGC 6791: A Probable Bulge Cluster without Multiple Populations

We present wide-field JHKS photometry of 16 Galactic globular clusters located towards the Galactic bulge, calibrated on the Two Micron All-Sky Survey photometric system. Differential reddening corrections and statistical field star decontamination are employed for all of these clusters before fi...


Cohen, R.E.Bidin, C.M.Mauro, F.Bonatto, C.Geisler, D.[Near-infrared photometry of globular clusters towards the Galactic bulge: Observations and photometric metallicity indicators]Near-infrared photometry of globular clusters towards the Galactic bulge: Observations and photometric metallicity indicators

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