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The GALAH survey

Published online by Cambridge University Press:  06 January 2014

B. Anguiano ,
K. Freeman ,
J. Bland-Hawthorn ,
G. De Silva ,
M. Asplund ,
D. Carollo ,
V. D'Orazi ,
S. Keller ,
S. Martell  and
S. Sharma
...Show all authors
B. Anguiano
Affiliation:
Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109Australia; Research Centre for Astronomy, Astrophysics and Astrophotonics, Macquarie University, Sydney, NSW 2109Australia
K. Freeman
Affiliation:
Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, ANU, Canberra, Australia
J. Bland-Hawthorn
Affiliation:
Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia
G. De Silva
Affiliation:
Australian Astronomical Observatory, 105 Delhi Rd, NSW 2113, Australia
M. Asplund
Affiliation:
Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, ANU, Canberra, Australia
D. Carollo
Affiliation:
Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109Australia; Research Centre for Astronomy, Astrophysics and Astrophotonics, Macquarie University, Sydney, NSW 2109Australia
V. D'Orazi
Affiliation:
Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109Australia; Research Centre for Astronomy, Astrophysics and Astrophotonics, Macquarie University, Sydney, NSW 2109Australia
S. Keller
Affiliation:
Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, ANU, Canberra, Australia
S. Martell
Affiliation:
Australian Astronomical Observatory, 105 Delhi Rd, NSW 2113, Australia
S. Sharma
Affiliation:
Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia
C. Sneden
Affiliation:
Department of Astronomy, University of Texas, Austin, USA
L. Wylie de Boer
Affiliation:
Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, ANU, Canberra, Australia
D. Zucker
Affiliation:
Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109Australia; Research Centre for Astronomy, Astrophysics and Astrophotonics, Macquarie University, Sydney, NSW 2109Australia
T. Zwitter
Affiliation:
University of Ljubljana, Faculty of Mathematics and Physics, Ljubljana, Slovenia; Center of excellence SPACE-SI, Ljubljana, Slovenia
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Abstract

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HERMES is a new high-resolution multi-object spectrograph on the Anglo Australian Telescope. The primary science driver for HERMES is the GALAH survey, GALactic Archaeology with HERMES. We are planning a spectroscopic survey of about a million stars, aimed at using chemical tagging techniques to reconstruct the star-forming aggregates that built up the disk, the bulge and halo of the Galaxy. This project will benefit greatly from the stellar distances and transverse motions from the Gaia mission.

Keywords

instrumentation: spectrographssurveysstars: abundancesGalaxy: evolutionGalaxy: kinematics and dynamicsGalaxy: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 322 - 325
Copyright
Copyright © International Astronomical Union 2014 

References

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