Bibcode
Zasowski, G.; Johnson, Jennifer A.; Frinchaboy, P. M.; Majewski, S. R.; Nidever, D. L.; Rocha Pinto, H. J.; Girardi, L.; Andrews, B.; Chojnowski, S. D.; Cudworth, K. M.; Jackson, K.; Munn, J.; Skrutskie, M. F.; Beaton, R. L.; Blake, C. H.; Covey, K.; Deshpande, R.; Epstein, C.; Fabbian, D.; Fleming, S. W.; García-Hernández, D. A.; Herrero, A.; Mahadevan, S.; Mészáros, Sz.; Schultheis, M.; Sellgren, K.; Terrien, R.; van Saders, J.; Allende-Prieto, C.; Bizyaev, D.; Burton, A.; Cunha, K.; da Costa, L. N.; Hasselquist, S.; Hearty, F.; Holtzman, J.; García Pérez, A. E.; Maia, M. A. G.; O'Connell, R. W.; O'Donnell, C.; Pinsonneault, M.; Santiago, B. X.; Schiavon, R. P.; Shetrone, M.; Smith, V.; Wilson, J. C.
Bibliographical reference
The Astronomical Journal, Volume 146, Issue 4, article id. 81, 28 pp. (2013).
Advertised on:
10
2013
Citations
335
Refereed citations
318
Description
The Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a
high-resolution infrared spectroscopic survey spanning all Galactic
environments (i.e., bulge, disk, and halo), with the principal goal of
constraining dynamical and chemical evolution models of the Milky Way.
APOGEE takes advantage of the reduced effects of extinction at infrared
wavelengths to observe the inner Galaxy and bulge at an unprecedented
level of detail. The survey's broad spatial and wavelength coverage
enables users of APOGEE data to address numerous Galactic structure and
stellar populations issues. In this paper we describe the APOGEE
targeting scheme and document its various target classes to provide the
necessary background and reference information to analyze samples of
APOGEE data with awareness of the imposed selection criteria and
resulting sample properties. APOGEE's primary sample consists of
~105 red giant stars, selected to minimize observational
biases in age and metallicity. We present the methodology and
considerations that drive the selection of this sample and evaluate the
accuracy, efficiency, and caveats of the selection and sampling
algorithms. We also describe additional target classes that contribute
to the APOGEE sample, including numerous ancillary science programs, and
we outline the targeting data that will be included in the public data
releases.
Related projects
Numerical Simulation of Astrophysical Processes
Numerical simulation through complex computer codes has been a fundamental tool in physics and technology research for decades. The rapid growth of computing capabilities, coupled with significant advances in numerical mathematics, has made this branch of research accessible to medium-sized research centers, bridging the gap between theoretical and
Daniel Elías
Nóbrega Siverio
Nucleosynthesis and molecular processes in the late stages of Stellar Evolution
Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch (AGB) - just before they form planetary nebulae (PNe) - where they experience complex nucleosynthetic and molecular processes. AGB stars are important contributors to the enrichment of the
Domingo Aníbal
García Hernández
Physical properties and evolution of Massive Stars
This project aims at the searching, observation and analysis of massive stars in nearby galaxies to provide a solid empirical ground to understand their physical properties as a function of those key parameters that gobern their evolution (i.e. mass, spin, metallicity, mass loss, and binary interaction). Massive stars are central objects to
Sergio
Simón Díaz
Chemical Abundances in Stars
Stellar spectroscopy allows us to determine the properties and chemical compositions of stars. From this information for stars of different ages in the Milky Way, it is possible to reconstruct the chemical evolution of the Galaxy, as well as the origin of the elements heavier than boron, created mainly in stellar interiors. It is also possible to
Carlos
Allende Prieto