SIMBAD references

2000AJ....119.1519H - Astron. J., 119, 1519-1525 (2000/April-0)

3 micron imaging of the Hubble Deep Field.

HOGG D.W., NEUGEBAUER G., COHEN J.G., DICKINSON M., DJORGOVSKI S.G., MATTHEWS K. and SOIFER B.T.

Abstract (from CDS):

Images of the Hubble Deep Field (HDF) at 3.2 µm, taken with the 10 m Keck Telescope, are presented. The images cover a total area of ∼2.5 arcmin2. To a 5 σ limit of [3.2]tot~17.5 mag (Vega relative), 11 sources are detected, nine of which are extragalactic. The integrated galaxy number counts are therefore ∼1.3x104 deg–2 to this depth. The galaxies detected at 3.2 µm have a median redshift of z=0.56. All 3.2 µm sources have 1.6 µm, 1.1 µm, and visual counterparts, all of fairly regular morphology; several also have 6.7 µm, 15 µm, 850 µm, 8.5 GHz, or 1.4 GHz counterparts. No sources are found that are either anomalously red or anomalously blue in their H-[3.2] color, and there are significant detections of most of the known near-infrared HDF sources for which detection in these 3.2 µm data seemed likely.

Abstract Copyright: ∼

Journal keyword(s): Galaxies: Photometry - Galaxies: Statistics - Infrared Radiation - Techniques: Photometric

Nomenclature: Table 2: [HNC2000] JHHMMSS.sss+DDMMSS.ss N=11.

Simbad objects: 12

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