FORS Deep Field UV to blue photometry (Gabasch+, 2004)

Details FORS Deep Field UV to blue photometry (Gabasch+, 2004) FORS Deep Field UV to blue photometry (Gabasch+, 2004)

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34210041g&link_type=abstract

VizieR On-line Data Catalog: J/A+A/421/41. Originally published in: 2004A&A...421...41G

Physics

Galaxies: Photometry

Scientific paper

We use the very deep and homogeneous I-band selected dataset of the FORS Deep Field (FDF) to trace the evolution of the luminosity function over the redshift range 0.5AB=26.8 misses of the order of 10% of the galaxies that would be detected in a K-band selected survey with magnitude limit KAB=26.3 (like FIRES). Photometric redshifts for 5558 galaxies are estimated based on the photometry in 9 filters (U, B, Gunn g, R, I, SDSS z, J, K and a special filter centered at 834nm).
(1 data file).

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