http://www.cco.caltech.edu/~btsoifer/hdf.html

Near infrared imaging of the Hubble Deep Field with the Keck Telescope

In keeping with the spirit of the Hubble Space Telescope Director's Discretionary Time program, the Hubble Deep Field (HDF; Williams et al 1996), the Caltech Faint Galaxy Consortium is making its K-band images of the HDF available to the public. This page is a companion to Hogg et al (1996, listed below).

Data

• Finding chart (gzipped PostScript) showing the locations of the two images, NIRC-HDF-A and NIRC-HDF-B, relative to the HST/WFPC2 image of the Hubble Deep Field.
• Reduced K-band image (FITS format) of NIRC-HDF-A. The zero-point is 30.48 mag and the pixel scale is 0.15 arcsec.
• Reduced K-band image (FITS format) of NIRC-HDF-B. The zero-point is 30.48 mag and the pixel scale is 0.15 arcsec.

References

• Hogg D. W., Neugebauer G., Armus L., Matthews K., Pahre M. A., Soifer B. T. & Weinberger A. J., 1996, Near infrared imaging of the Hubble Deep Field with the Keck Telescope, Astronomical Journal, in press.
• Williams R. E. et al, 1996, The Hubble Deep Field: Observations, data reduction and galaxy photometry, Astronomical Journal, in press.