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NIR Follow-Up of the VVDS 02hr Field

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arxiv astro-ph/0611108 v1 pith:BD6F3ZEI submitted 2006-11-03 astro-ph

S. Temporin , A. Iovino , H. J. McCracken , M. Bolzonella , M. Scodeggio , D. Bottini , B. Garilli , V. Le Brun
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O. Le Fevre D. Maccagni J.-P. Picat R. Scaramella L. Tresse G. Vettolani A. Zanichelli C. Adami S. Arnouts S. Bardelli A. Cappi S. Charlot P. Ciliegi T. Contini O. Cucciati S. Foucaud P. Franzetti I. Gavignaud L. Guzzo O. Ilbert B. Marano C. Marinoni A. Mazure B. Meneux R. Merighi S. Paltani R. Pello A. Pollo L. Pozzetti M. Radovich G. Zamorani E. Zucca M. Bondi A. Bongiorno J. Brinchmann S. de la Torre F. Lamareille Y. Mellier P. Merluzzi D. Vergani C. J. Walcher
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classification astro-ph
keywords fieldk-bandvvdsarcminassesscatalogueclassescolor
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abstract

We present a new K-band survey covering 623 arcmin$^2$ in the VVDS 0226-0430 deep field down to a limiting magnitude K$_{\rm{Vega}}$ $\leq$ 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.

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