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Properties of Lyα emitters at z≃6

Published online by Cambridge University Press:  01 August 2006

Crystal L. Martin ,
Marcin Sawicki ,
Alan Dressler  and
Patrick J. McCarthy
Crystal L. Martin
Affiliation:
Department of Physics, UCSB, Santa Barbara, CA 93106, USA email: [email protected]
Marcin Sawicki
Affiliation:
Department of Physics, UCSB, Santa Barbara, CA 93106, USA email: [email protected]
Alan Dressler
Affiliation:
OCIW, 813 Santa Barbara Street, Pasadena, CA 91101-1292, USA
Patrick J. McCarthy
Affiliation:
OCIW, 813 Santa Barbara Street, Pasadena, CA 91101-1292, USA
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Abstract

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We confirm the redshift of several z≃6 objects discovered by our imacs multislit emission-line survey. Their Lyα luminosities are lower than those of galaxies previously discovered using narrow-band imaging, as expected due to the excellent sky-supression inherent to this technique. Based on the line profiles of these objects, we argue that they are extremely young starbursts and find strong evidence for prominent galactic winds. This population of young galaxies is largely beyond the reach of current large surveys that use continuum selection.

Keywords

galaxies:high-redshiftline: identificationtechniques: miscellaneous
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 253
Copyright
Copyright © International Astronomical Union 2007

References

Hansen, M., & Peng Oh, S. 2006, MNRAS, 367, 979CrossRefGoogle Scholar
Martin, C. L., & Sawicki, M. 2004, ApJ, 603, 414CrossRefGoogle Scholar
Tran, K. H., Lilly, S. J., Crampton, D., & Brodwin, M. 2004, ApJ, 612, 89CrossRefGoogle Scholar
Verhamme, A., Schaerer, D., & Maselli, A. 2006, A&A, 460, 397Google Scholar