UGRK Photometry in the Hubble Deep field region (Hogg+, 2000)

Details UGRK Photometry in the Hubble Deep field region (Hogg+, 2000) UGRK Photometry in the Hubble Deep field region (Hogg+, 2000)

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..21270001h&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/127/1. Originally published in: 2000ApJS..127....1H

Physics

Colors, Galaxies: Photometry, Photometry: Ccd

Scientific paper

For visual data, Un=0.53F300W+0.47F450W-0. G=0.83F450W+0.18F606W-0.07mag, and {R}=0.46F606W+0.54F814W-0.02mag images taken with the COSMIC camera (Kells et al., 1998PASP..110.1487K) at the prime focus of the 200 inch Hale Telescope at the Palomar Observatory were used. The Un, G, and {R} filters are described in Steidel & Hamilton (1993AJ....105.2017S); briefly, they have effective wavelengths of 3570, 4830, and 6930Å, FWHM bandpasses of 700, 1200, and 1500Å, and zero-magnitude flux densities of roughly 1550, 3890, and 2750Jy. These magnitudes are Vega relative, not AB. For near-infrared data, an 8' diameter circular region centered on the HDF was imaged on 1997 March 19 - 21 using a Ks filter with a near-infrared camera (Jarrett et al., 1994) mounted at the prime focus of the 200 inch Hale Telescope. The Ks filter has an effective wavelength of 2.15μm, a FWHM bandpass of 0.3μm, and a zero-magnitude flux density of roughly 708Jy. (3 data files).

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