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Galactic Stellar Populations in the Era of the Sloan Digital Sky Survey and Other Large Surveys
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Studies of stellar populations, understood to mean collections of stars with common spatial, kinematic, chemical, and/or age distributions, have been reinvigorated during the past decade by the advent of large-area sky surveys such as the Sloan Digital Sky Survey, the Two-Micron All Sky Survey, the Radial Velocity Experiment, and others. We review recent analyses of these data that, together with theoretical and modeling advances, are revolutionizing our understanding of the nature of the Milky Way and galaxy formation and evolution in general. The formation of galaxies like the Milky Way was long thought to be a steady process leading to a smooth distribution of stars. However, the abundance of substructure in the multidimensional space of various observables, such as position, kinematics, and metallicity, is now proven beyond doubt and demonstrates the importance of mergers in the growth of galaxies. Unlike smooth models that involve simple components, the new data reviewed here clearly exhibit many irregular structures, such as the Sagittarius dwarf tidal stream and the Virgo and Pisces overdensities in the halo and the Monoceros stream closer to the Galactic plane. These recent developments have made it clear that the Milky Way is a complex and dynamic structure, one that is still being shaped by the merging of neighboring smaller galaxies. We also briefly discuss the next generation of wide-field sky surveys, such as SkyMapper, Panoramic Survey Telescope & Rapid Response System, Global Astrometric Interferometer for Astrophysics, and the Large Synoptic Survey Telescope, which will improve measurement precision manyfold and include billions of individual stars. The ultimate goal, development of a coherent and detailed story of the assembly and evolutionary history of the Milky Way and other large spirals like it, now appears well within reach.
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“Hence, LSST will smoothly extend Gaia ' s error versus magnitude curve about 4 mag fainter ( for illustration, see Figure 21 in Ivezi ć et al. 2012 ) .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Ivezić et al. 2012
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“LSST and Gaia will be highly complementary data sets for studying the Milky Way in the multidimensional space of three-dimensional positions, proper motions, and metallicity”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Ivezić et al. 2012
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FOUR NEW STELLAR DEBRIS STREAMS IN THE GALACTIC HALO
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THE GENESIS OF THE MILKY WAY'S THICK DISK VIA STELLAR MIGRATION
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An Improved Proper-Motion Catalog Combining USNO-B and the Sloan Digital Sky Survey
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Evidence for Stellar Substructure in the Halo and Outer Disk of M31
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The hierarchical origin of galaxy morphologies
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Candidate RR Lyrae Stars Found in Sloan Digital Sky Survey Commissioning Data*
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THE MILKY WAY TOMOGRAPHY WITH SDSS. III. STELLAR KINEMATICS
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Self-citationTHE CASE FOR THE DUAL HALO OF THE MILKY WAY
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A Survey of Proper Motion Stars. XIII. The Halo Population
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Kinematics of SDSS subdwarfs: structure and substructure of the Milky Way halo
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QUANTIFYING KINEMATIC SUBSTRUCTURE IN THE MILKY WAY'S STELLAR HALO
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The VMC survey. I. Strategy and first data
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Tracing the Galactic Anticenter Stellar Stream with 2MASS M Giants
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CARBON-ENHANCED METAL-POOR STARS IN THE INNER AND OUTER HALO COMPONENTS OF THE MILKY WAY
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MAPPING THE GALACTIC HALO. VIII. QUANTIFYING SUBSTRUCTURE
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Modelling the Galactic bar using OGLE-II Red Clump Giant StarsPreprint
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Orbital eccentricity as a probe of thick disc formation scenarios
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Self-citationTwo Disk Components from a Gas‐Rich Disk‐Disk Merger
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Distance determination for RAVE stars using stellar models
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VELOCITY DISPERSION PROFILE OF THE MILKY WAY HALO
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FIRST RESULTS FROM THE NOAO SURVEY OF THE OUTER LIMITS OF THE MAGELLANIC CLOUDS
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Revealing Substructure in the Galactic Halo: The SEKBO RR Lyrae Survey
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CARBON-ENHANCED METAL-POOR STARS IN THE INNER AND OUTER HALO COMPONENTS OF THE MILKY WAY
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HALO STREAMS IN THE SEVENTH SLOAN DIGITAL SKY SURVEY DATA RELEASE
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The Stellar Content of Galaxy Halos: A Comparison between ΛCDM Models and Observations of M31
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FIRST RESULTS FROM THE NOAO SURVEY OF THE OUTER LIMITS OF THE MAGELLANIC CLOUDS
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The long Galactic bar as seen by UKIDSS Galactic Plane Survey
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THE TILT OF THE HALO VELOCITY ELLIPSOID AND THE SHAPE OF THE MILKY WAY HALO
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On the alleged duality of the Galactic haloPreprint
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THE THREE-DIMENSIONAL VELOCITY STRUCTURE OF THE THICK DISK FROM SPM4 AND RAVE DR2
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Self-citationThe Apache Point Observatory Galactic Evolution Experiment (APOGEE)
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Metadata
- Authors
- Ivezić, Ž., Beers, T. C., & Jurić, M.
- Affiliations
- Harvard University (US)
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2012-09-22
- Volume
- 50
- Issue
- 1
- Pages
- 251-304
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2127189980
- Cited by
- 136
- References
- 225
- Citations by year
- 2026: 2 · 2025: 3 · 2024: 4 · 2023: 5 · 2022: 9 · 2021: 8 · 2020: 6 · 2019: 16 · 2018: 9 · 2017: 10 · 2016: 15 · 2015: 18 · 2014: 17 · 2013: 14
- FWCI
- 1.27
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Annual Review of Astronomy and Astrophysics (publishedVersion)
- arXiv (Cornell University) (publishedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Keywords
- stellar populations, Milky Way formation, galaxy mergers, galactic substructure, Virgo Overdensity, Galactic halo, stellar kinematics, metallicity, wide-field sky survey, LSST, SkyMapper, Pan-STARRS, Gaia
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