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20062026
most citedThe Milky Way's circular velocity curve between 4 and 14 kpc from APOGEE data

419 citations · 3.9k across the 76 of their papers we have counts for

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astro-ph.SR201894 cited

A homogeneous analysis of globular clusters from the APOGEE survey with the BACCHUS code. I. The Northern clusters

T. Masseron, D. A. García-Hernández, Sz. Mészáros +12

We analyze a large sample of 885 GCs giants from the APOGEE survey. We used the Cannon results to separate the red giant branch and the asymptotic giant branch stars, not only allo…

astro-ph.GA2018

APOGEE DR14/DR15 Abundances in the Inner Milky Way

G. Zasowski, M. Schultheis, S. Hasselquist +14

We present an overview of the distributions of 11 elemental abundances in the Milky Way's inner regions, as traced by APOGEE stars released as part of SDSS Data Release 14/15 (DR14…

astro-ph.GA2018

Discovery of a disrupting open cluster far into the Milky Way halo: a recent star formation event in the leading arm of the Magellanic stream?

Adrian M. Price-Whelan, David L. Nidever, Yumi Choi +4

We report the discovery of a young (), low-mass (), metal-poor () stellar association at a he…

astro-ph.GA2018

Chemical Cartography with APOGEE: Multi-element abundance ratios

David H. Weinberg, Jon A. Holtzman, Sten Hasselquist +25

We map the trends of elemental abundance ratios across the Galactic disk, spanning R = 3-15 kpc and midplane distance |Z|= 0-2 kpc, for 15 elements in a sample of 20,485 stars meas…

astro-ph.GA2018

A Lonely Giant: The Sparse Satellite Population of M94 Challenges Galaxy Formation

Adam Smercina, Eric F. Bell, Paul A. Price +5

The dwarf satellites of `giant' Milky Way (MW)-mass galaxies are our primary probes of low-mass dark matter halos. The number and velocities of the satellite galaxies of the MW and…

astro-ph.SR2018

44 New & Known M Dwarf Multiples In The SDSS-III/APOGEE M Dwarf Ancillary Science Sample

Jacob Skinner, Kevin R. Covey, Chad F. Bender +28

Binary stars make up a significant portion of all stellar systems. Consequently, an understanding of the bulk properties of binary stars is necessary for a full picture of star for…