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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

Busca, N. G.Delubac, T.Rich, J.Bailey, S.Font Ribera, A.Kirkby, D.Le Goff, J. M.Pieri, M. M.Slosar, A.Aubourg, É.Bautista, J. E.Bizyaev, D.Blomqvist, M.Bolton, A. S.Bovy, J.Brewington, H.Borde, A.Brinkmann, J.Carithers, B.Croft, R. A. C.Dawson, K. S.Ebelke, G.Eisenstein, D. J.Hamilton, J. C.Ho, S.Hogg, D. W.Honscheid, K.Lee, K. G.Lundgren, B.Malanushenko, E.Malanushenko, V.Margala, D.Maraston, C.Mehta, K.Miralda Escudé, J.Myers, A. D.Nichol, R. C.Noterdaeme, P.Olmstead, M. D.Oravetz, D.Palanque-Delabrouille, NathaliePan, K.Pâris, I.Percival, W. J.Petitjean, P.Roe, N. A.Rollinde, E.Ross, N. P.Rossi, G.Schlegel, D. J.Schneider, D. P.Shelden, A.Sheldon, E. S.Simmons, A.Snedden, S.Tinker, J. L.Viel, M.Weaver, B. A.Weinberg, D. H.White, M.Yèche, C.York, D. G.[Baryon acoustic oscillations in the Lyα forest of BOSS quasars]

Palanque-Delabrouille, NathalieMagneville, Ch.Yèche, Ch.Eftekharzadeh, S.Myers, A. D.Petitjean, P.Pâris, I.Aubourg, E.McGreer, I.Fan, X.Dey, A.Schlegel, D.Bailey, S.Bizayev, D.Bolton, A.Dawson, K.Ebelke, G.Ge, J.Malanushenko, E.Malanushenko, V.Oravetz, D.Pan, K.Ross, N. P.Schneider, D. P.Sheldon, E.Simmons, A.Tinker, J.White, M.Willmer, Ch.[Luminosity function from dedicated SDSS-III and MMT data of quasars in 0.7 < z < 4.0 selected with a new approach]

The galaxy integrated Hα star formation rate-stellar mass relation, or SFR(global)-M ∗(global) relation, is crucial for understanding star formation history and evolution of galaxies. However, many studies have dealt with SFR using unresolved measurements, which makes it difficult to separate out...


Pan, H.-A.Lin, L.Hsieh, B.-C.Sánchez, S.F.Ibarra-Medel, H.Boquien, M.Lacerna, I.Argudo-Fernández, M.Bizyaev, D.Cano-Díaz, M.Drory, N.Gao, Y.Masters, K.Pan, K.Tabor, M.Tissera, P.Xiao, T.[SDSS IV MaNGA: Dependence of Global and Spatially Resolved SFR-M ∗ Relations on Galaxy Properties]SDSS IV MaNGA: Dependence of Global and Spatially Resolved SFR-M ∗ Relations on Galaxy Properties

Schiappacasse-Ulloa, J.Tang, B.Fernandez-Trincado, J. G.Zamora, O.Geisler, D.Frinchaboy, P.Schultheis, M.Dell'Agli, F.Villanova, S.Masseron, T.Meszaros, SzSouto, D.Hasselquist, S.Cunha, K.Smith, V. V.Garcia-Hernandez, D. A.Vieira, K.Robin, A. C.Minniti, D.Zasowski, G.Moreno, E.Perez-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

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