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20012026
most citedAPOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

481 citations · 3.2k across the 42 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

astro-ph.SR2022★ 3 cited

The first r-process enhanced star confirmed to be a member of the Galactic bulge

R. Forsberg, R. M. Rich, N. Nieuwmunster +4

Aims. Stars with strong enhancements of r-process elements are rare and tend to be metal-poor, with generally [Fe/H] <-2 dex and found in the halo. In this work we aim to investiga…

astro-ph.GA2022★ 54 cited

BACCHUS Analysis of Weak Lines in APOGEE Spectra (BAWLAS)

Christian R. Hayes, Thomas Masseron, Jennifer Sobeck +11

Elements with weak and blended spectral features in stellar spectra are challenging to measure and require specialized analysis methods to precisely measure their chemical abundanc…

astro-ph.GA2022★ 72 cited

The Open Cluster Chemical Abundances and Mapping Survey: VI. Galactic Chemical Gradient Analysis from APOGEE DR17

Natalie Myers, John Donor, Taylor Spoo +19

The goal of the Open Cluster Chemical Abundances and Mapping (OCCAM) survey is to constrain key Galactic dynamic and chemical evolution parameters by the construction and analysis…

astro-ph.GA2022★ 19 cited

Chemical Evolution of Ytterbium in the Galactic Disk

M. Montelius, R. Forsberg, N. Ryde +8

Measuring the abundances of neutron-capture elements in Galactic disk stars is an important part of understanding key stellar and galactic processes. In the optical wavelength regi…

astro-ph.SR2022★ 46 cited

Detailed Chemical Abundances for a Benchmark Sample of M Dwarfs from the APOGEE Survey

Diogo Souto, Katia Cunha, Verne V. Smith +16

Individual chemical abundances for fourteen elements (C, O, Na, Mg, Al, Si, K, Ca, Ti, V, Cr, Mn, Fe, and Ni) are derived for a sample of M-dwarfs using high-resolution near-infrar…