NIR Follow-Up of the VVDS 02hr Field

S. Temporin , A. Iovino , H. J. McCracken , M. Bolzonella , M. Scodeggio , D. Bottini , B. Garilli , V. Le Brun

show 41 more authors

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

Authors on Pith no claims yet

classification 🌌 astro-ph

keywords fieldk-bandvvdsarcminassesscatalogueclassescolor

0 comments

read the original 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.

This paper has not been read by Pith yet.

NIR Follow-Up of the VVDS 02hr Field

discussion (0)