NIR Follow-Up of the VVDS 02hr Field
Astrophysics
2017-03-22 v1
Abstract
We present a new K-band survey covering 623 arcmin in the VVDS 0226-0430 deep field down to a limiting magnitude K 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
Cite
@article{arxiv.astro-ph/0611108,
title = {NIR Follow-Up of the VVDS 02hr Field},
author = {S. Temporin and A. Iovino and H. J. McCracken and M. Bolzonella and M. Scodeggio and D. Bottini and B. Garilli and V. Le Brun and O. Le Fevre and D. Maccagni and J. -P. Picat and R. Scaramella and L. Tresse and G. Vettolani and A. Zanichelli and C. Adami and S. Arnouts and S. Bardelli and A. Cappi and S. Charlot and P. Ciliegi and T. Contini and O. Cucciati and S. Foucaud and P. Franzetti and I. Gavignaud and L. Guzzo and O. Ilbert and B. Marano and C. Marinoni and A. Mazure and B. Meneux and R. Merighi and S. Paltani and R. Pello and A. Pollo and L. Pozzetti and M. Radovich and G. Zamorani and E. Zucca and M. Bondi and A. Bongiorno and J. Brinchmann and S. de la Torre and F. Lamareille and Y. Mellier and P. Merluzzi and D. Vergani and C. J. Walcher},
journal= {arXiv preprint arXiv:astro-ph/0611108},
year = {2017}
}
Comments
6 pages, 4 figures. To appear in the Proceedings of the IAU Symposium No. 235, 2006, "Galaxy Evolution across the Hubble Time", F. Combes & J. Palous, eds