J. P. Gardner

A Wide-Field K-band Survey: The Luminosity Function of Galaxies

We present the first determination of the near-infrared K-band luminosity function of field galaxies from a wide-field K-selected redshift survey. The best-fit Schechter function parameters are M* = -23.12 + 5 log h, α = -0.91, and * = 1.66 × 10-2h3 Mpc-3. We estimate that systematics are no more than 0.1 mag in M* and 0.1 in α, which is comparable to the statistical errors on this measurement.

A wide-field K-band survey — II. Galaxy clustering

We present the first measurement of the angular correlation function in a

The K-Band Luminosity Function of Galaxies

K

A WIDE-FIELD K-BAND SURVEY - I. GALAXY COUNTS IN B, V, I AND K

-selected galaxy survey, from two fields covering almost 10 square degrees. The angular correlation function at small angles is well described by a

Galaxy number counts—IV. Surveying the Herschel Deep Field in the near-infrared

\theta^{-0.8}

K-baml photometry of spectroscopic redshift survey objects

power law, as for optically selected samples. The clustering amplitude is reduced by a factor of

Galaxy Counts, Sizes, Colours and Redshifts in the Hubble Deep Field

\sim 4

The K-band Luminosity Function of Early-Type Galaxies

between galaxies with

A Wide-Field K-band Galaxy Survey: The Color and Surface Brightness Distribution of Nearby Galaxies

K<15

Faint Galaxy Number-Counts

and a fainter magnitude slice with