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NIR Follow-Up of the VVDS 02hr Field: First Results

Published online by Cambridge University Press:  01 August 2006

S. Temporin ,
A. Iovino ,
H. J. McCracken ,
M. Bolzonella  and
M. Scodeggio
S. Temporin
Affiliation:
INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20121 Milano, Italy
A. Iovino
Affiliation:
INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20121 Milano, Italy
H. J. McCracken
Affiliation:
Institut d'Astrophysique de Paris, UMR 7095, 98 bis Bvd Arago, 75014 Paris, France Observatoire de Paris, LERMA, 61 Avenue de l'Observatoire, 75014 Paris, France
M. Bolzonella
Affiliation:
INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, Bologna, Italy
M. Scodeggio
Affiliation:
INAF-IASF, Via Bassini 11, Milano, Italy
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Abstract

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We present a new K-band survey covering 623 arcmin2 in the VVDS 0226-0430 deep field down to a limiting magnitude KVega ≤ 20.5. We use the spectroscopic sample extracted from this new K-band catalogue to assess the effectiveness of optical-near infrared color selections in identifying extreme classes of objects at high redshift.

Keywords

Infrared: galaxiessurveysgalaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 432 - 437
Copyright
Copyright © International Astronomical Union 2007

References

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