UltraVISTA: a new ultra-deep near-infrared survey in COSMOS

In this paper we describe the first data release of the UltraVISTA near-infrared imaging survey of the COSMOS field. We summarise the key goals and design of the survey and provide a detailed description of our data reduction techniques. We provide stacked, sky-subtracted images in YJHKs and narrow-...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2012-08, Vol.544, p.A156
Hauptverfasser: McCracken, H. J., Milvang-Jensen, B., Dunlop, J., Franx, M., Fynbo, J. P. U., Le Fèvre, O., Holt, J., Caputi, K. I., Goranova, Y., Buitrago, F., Emerson, J. P., Freudling, W., Hudelot, P., López-Sanjuan, C., Magnard, F., Mellier, Y., Møller, P., Nilsson, K. K., Sutherland, W., Tasca, L., Zabl, J.
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Sprache:eng
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Zusammenfassung:In this paper we describe the first data release of the UltraVISTA near-infrared imaging survey of the COSMOS field. We summarise the key goals and design of the survey and provide a detailed description of our data reduction techniques. We provide stacked, sky-subtracted images in YJHKs and narrow-band filters constructed from data collected during the first year of UltraVISTA observations. Our stacked images reach 5σAB depths in an aperture of 2″ diameter of  ~25 in Y and  ~24 in JHKs bands and all have sub-arcsecond seeing. To this 5σ limit, our Ks catalogue contains 216 268 sources. We carry out a series of quality assessment tests on our images and catalogues, comparing our stacks with existing catalogues. The 1σ astrometric rms in both directions for stars selected with 17.0 
ISSN:0004-6361
1432-0746
1432-0756
DOI:10.1051/0004-6361/201219507