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Wang, W.Feng, BXiao, ZZhou, XLi, PZhang, WWang, Y.Lindberg Møller, BZhang, P.Luo, MXiao, GLiu, JYang, JChen, S.Rabinowicz, PDChen, X.Zhang, HBCeballos, H.Lou, QZou, MCarvalho, LJCBZeng, CXia, J.Sun, SFu, YWang, H.Lu, CRuan, MZhou, S.Wu, ZLiu, HKannangara, RMJørgensen, KNeale, RLBonde, MHeinz, NZhu, WWang, S.Zhang, Y.Pan, KWen, MMa, PLi, ZHu, MLiao, WHu, WZhang, S.Pei, JGuo, AGuo, JZhang, JZhang, Z.Ye, JOu, WMa, YLiu, XTallon, LJGalens, KOtt, SHuang, JXue, JAn, FYao, QLu, XFregene, Martin A.Becerra López Lavelle, Luis AugustoWu, J.You, FMChen, M.Hu, SWu, G.Zhong, SLing, PChen, Y.Wang, Q.Liu, GLiu, BLi, KPeng, M[Cassava genome from a wild ancestor to cultivated varieties]Cassava genome from a wild ancestor to cultivated varieties

Multiple populations revealed in globular clusters (GCs) are important windows to the formation and evolution of these stellar systems. The metal-rich GCs in the Galactic bulge are an indispensable part of this picture, but the high optical extinction in this region has prevented extensive resear...


Tang, BCohen, REGeisler, DSchiavon, RPMajewski, SRVillanova, SCarrera, RZamora, OGarcia-Hernandez, DAShetrone, MFrinchaboy, PMeza, AFernandez-Trincado, JGMunoz, RRLin, CCLane, RRNitschelm, CPan, KBizyaev, DOravetz, DSimmons, A[Two groups of red giants with distinct chemical abundances in the bulge globular cluster NGC 6553 through the eyes of APOGEE]Two groups of red giants with distinct chemical abundances in the bulge globular cluster NGC 6553 through the eyes of APOGEE

Fernandez-Trincado, JGRobin, ACMoreno, ESchiavon, RPPerez, AEGVieira, KCunha, KZamora, OSneden, CSouto, DCarrera, RJohnson, JAShetrone, MZasowski, GGarcia-Hernandez, DAMajewski, SRReyle, CBlanco-Cuaresma, SMartinez-Medina, LAPerez-Villegas, AValenzuela, OPichardo, BMeza, AMeszaros, SSobeck, JGeisler, DAnders, FSchultheis, MTang, BRoman-Lopes, AMennickent, REPan, KNitschelm, CAllard, F[DISCOVERY OF A METAL-POOR FIELD GIANT WITH A GLOBULAR CLUSTER SECOND-GENERATION ABUNDANCE PATTERN]DISCOVERY OF A METAL-POOR FIELD GIANT WITH A GLOBULAR CLUSTER SECOND-GENERATION ABUNDANCE PATTERN

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