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Chemo-Kinematic Survey of z ∼ 1 Star Forming Galaxies using Keck OSIRIS LGS-AO

Published online by Cambridge University Press:  09 February 2015

Etsuko Mieda ,
Shelley A. Wright ,
James E. Larkin ,
Lee Armus  and
Stephanie Juneau
Etsuko Mieda
Affiliation:
Department of Astronomy and Astrophysics, University of Toronto, ON, Canada, M5S3H4 email: mieda@astro.utoronto
Shelley A. Wright
Affiliation:
Department of Astronomy and Astrophysics, University of Toronto, ON, Canada, M5S3H4 email: mieda@astro.utoronto Dunlap Institute for Astronomy & Astrophysics, Toronto, ON, Canada, M5S3H4
James E. Larkin
Affiliation:
Department of Physics and Astronomy, University of California, Los Angeles, CA, USA, 90095
Lee Armus
Affiliation:
Spitzer Science Center, California Institute of Technology, Pasadena, CA, 91125
Stephanie Juneau
Affiliation:
CEA Saclay, DSM/IRFU/Sap.F-91191Gif-sur-Yvette, France
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Abstract

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We present first results from the Intermediate Redshift OSIRIS Chemo-Kinematic Survey (IROCKS) of z ∼ 1 star forming galaxies (Mieda et al. in prep). We have targeted Hα and [NII] emission lines in J-band and have spatially resolved the galaxies at sub-kilo parsec scale. We have combined our sample with deep HST continuum images, and are able to reveal the dynamics, morphologies, metallicity distribution, emission-line diagnostics, and star formation rates of galaxies spanning this crucial z ∼ 1 epoch.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 362
Copyright
Copyright © International Astronomical Union 2015 

References

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