The Open Cluster Chemical Analysis and Mapping Survey: Local Galactic Metallicity Gradient with APOGEE using SDSS DR10
Peter M. Frinchaboy, Benjamin Thompson, Kelly M. Jackson, Julia, O'Connell, Brianne Meyer, Gail Zasowski, Steven R. Majewski, S. Drew, Chojnowksi, Jennifer A. Johnson, Carlos Allende Prieto, Timothy C. Beers,, Dmitry Bizyaev, Howard Brewington, Katia Cunha, Garrett Ebelke

TL;DR
This study uses APOGEE data to analyze open clusters and map the Galactic metallicity gradient, revealing a steep gradient near the Sun and a flattening beyond 10 kpc, improving understanding of Galactic chemical structure.
Contribution
It provides the first high-resolution metallicity measurements for 22 open clusters and investigates the Galactic disk gradients using a large, uniform sample from APOGEE.
Findings
No significant [alpha/M] gradient across the sample.
[M/H] gradient is steep inside 10 kpc and flattens beyond.
Steeper gradient near the Sun than previously reported.
Abstract
The Open Cluster Chemical Analysis and Mapping (OCCAM) Survey aims to produce a comprehensive, uniform, infrared-based dataset for hundreds of open clusters, and constrain key Galactic dynamical and chemical parameters from this sample. This first contribution from the OCCAM survey presents analysis of 141 members stars in 28 open clusters with high-resolution metallicities derived from a large uniform sample collected as part of the SDSS-III/Apache Point Observatory Galactic Evolution Experiment (APOGEE). This sample includes the first high-resolution metallicity measurements for 22 open clusters. With this largest ever uniformly observed sample of open cluster stars we investigate the Galactic disk gradients of both [M/H] and [alpha/M]. We find basically no gradient across this range in [alpha/M], but [M/H] does show a gradient for R_{GC} < 10 kpc and a significant flattening beyond…
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