The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, uniform, infrared-based data set 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 Sloan Digital Sky Survey III/Apache Point Observatory Galactic Evolution Experiment. 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 ...
Open Clusters are born and evolve along the Milky Way plane, on them is imprinted the history of the...
We perform an extensive test of theoretical stellar models for main-sequence (MS) stars in ugriz, us...
We obtained high-resolution UVES/FLAMES observations of a sample of nine old open clusters spanning ...
The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, unifo...
The Open Cluster Chemical Abundances and Mapping (OCCAM) survey aims to constrain key Galactic dynam...
In this paper, we make use of data collected for open cluster members by high-resolution spectrosco...
The goal of the Open Cluster Chemical Abundances and Mapping (OCCAM) survey is to constrain key Gala...
The problem of the chemical composition gradient in the Galactic disk is studied based on a sample o...
We present Galactic mean metallicity maps derived from the first year of the SDSS-III APOGEE experim...
Open clusters (OCs) are crucial for studying the formation and evolution of the Galactic disc. Howev...
This thesis has as a main purpose the determination of the chemical composition of Open Clusters for...
Context. The present number of Galactic open clusters that have high resolution abundance determina...
Context. In the framework of the study of the Galactic metallicity gradient and its time e...
Spina, L., et al.Open clusters are unique tracers of the history of our own Galaxy's disc. According...
Open clusters have long been used to study the chemodynamical evolution of the Galactic disc. This r...
Open Clusters are born and evolve along the Milky Way plane, on them is imprinted the history of the...
We perform an extensive test of theoretical stellar models for main-sequence (MS) stars in ugriz, us...
We obtained high-resolution UVES/FLAMES observations of a sample of nine old open clusters spanning ...
The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, unifo...
The Open Cluster Chemical Abundances and Mapping (OCCAM) survey aims to constrain key Galactic dynam...
In this paper, we make use of data collected for open cluster members by high-resolution spectrosco...
The goal of the Open Cluster Chemical Abundances and Mapping (OCCAM) survey is to constrain key Gala...
The problem of the chemical composition gradient in the Galactic disk is studied based on a sample o...
We present Galactic mean metallicity maps derived from the first year of the SDSS-III APOGEE experim...
Open clusters (OCs) are crucial for studying the formation and evolution of the Galactic disc. Howev...
This thesis has as a main purpose the determination of the chemical composition of Open Clusters for...
Context. The present number of Galactic open clusters that have high resolution abundance determina...
Context. In the framework of the study of the Galactic metallicity gradient and its time e...
Spina, L., et al.Open clusters are unique tracers of the history of our own Galaxy's disc. According...
Open clusters have long been used to study the chemodynamical evolution of the Galactic disc. This r...
Open Clusters are born and evolve along the Milky Way plane, on them is imprinted the history of the...
We perform an extensive test of theoretical stellar models for main-sequence (MS) stars in ugriz, us...
We obtained high-resolution UVES/FLAMES observations of a sample of nine old open clusters spanning ...