Near Infrared Imaging of the Hubble Deep Field with The Keck Telescope

Details Near Infrared Imaging of the Hubble Deep Field with The Keck Telescope Near Infrared Imaging of the Hubble Deep Field with The Keck Telescope

1996-11-08

arxiv.org/abs/astro-ph/9611070v2

AJ 113 474 (plus erratum AJ in press)

Astronomy and Astrophysics

Astrophysics

Replaced with slightly revised source positions and corrected V-I magnitudes (which were incorrect in the Tables and Figure 5)

Scientific paper

10.1086/118269

Two deep K-band ($2.2 \mu m$) images, with point-source detection limits of $K=25.2$ mag (one sigma), taken with the Keck Telescope in subfields of the Hubble Deep Field, are presented and analyzed. A sample of objects to K=24 mag is constructed and $V_{606}-I_{814}$ and $I_{814}-K$ colors are measured. By stacking visually selected objects, mean $I_{814}-K$ colors can be measured to very faint levels; the mean $I_{814}-K$ color is constant with apparent magnitude down to $V_{606}=28$ mag.

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