activity
20152022
most citedAPOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

481 citations · 898 across the 11 of their papers we have counts for

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astro-ph.SR2026

Carbon in J0815+4729: Casting A Shadow of Doubt on the Interpretation of CH Absorption in the Most Primitive Stars

Junbo Zhang, Carlos Allende Prieto, Yeisson Osorio +7

We revisit the carbon abundance in the primitive iron-poor star J0815+4729 ([Fe/H] 5.49). J0815+4729 is so carbon-enhanced and oxygen-rich that, in addition to CH and C$_{2}…

astro-ph.SR20227 cited

Accurate Metallicities for Very Metal-Poor Stars from the Ca~II Infrared Triplet

Y. Osorio, D. S. Aguado, C. Allende-Prieto +2

The Ca~II H \& K lines are among the few features available to infer the metallicity of extremely metal-poor stars from medium-resolution spectroscopy. Unfortunately, these lines c…

astro-ph.SR20218 cited

Understanding the angular momentum evolution of T Tauri and Herbig Ae/Be stars

Giovanni Pinzón, Jesús Hernández, Javier Serna +8

We investigate a sample of 6 Herbig Ae/Be stars belonging to the Orion OB1 association, as well as 73 low mass objects, members of the Orionis cluster, in order to explore the…

astro-ph.SR202117 cited

TLUSTY and SYNSPEC Users's Guide IV: Upgraded Versions 208 and 54

Ivan Hubeny, Carlos Allende Prieto, Yeisson Osorio +1

We present a brief description of the newly upgraded versions of the programs TLUSTY, version 208, and SYNSPEC, version 54. TLUSTY is used to generate model stellar atmospheres or…

astro-ph.SR2021

The APOGEE Data Release 16 Spectral Line List

Verne V. Smith, Dmitry Bizyaev, Katia Cunha +15

The updated H-band spectral line list (from λ15,000 - 17,000Å) adopted by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) for the SDSS IV Data Release 16 (DR16)…

astro-ph.SR20219 cited

Probing 3D and NLTE models using APOGEE observations of globular cluster stars

T. Masseron, Y. Osorio, D. A. García-Hernández +3

Hydrodynamical (or 3D) and non-local thermodynamic equilibrium (NLTE) effects are known to affect abundance analyses. However, there are very few observational abundance testsof 3D…