Abstract

This paper describes the Sloan Digital Sky Survey photometric system, a new five-color (u‧ g‧ r‧ i‧ z‧) wide-band CCD system with wavelength coverage from 3000 to 11 000 Å. The zero points will be based on an updated version of the spectrophotometric AB<SUB>v</SUB> system. This updated calibration, designated as AB<SUB>95</SUB>, is presented in this paper.

Keywords

PhysicsSkyAstronomyPhotometry (optics)Photometric systemRemote sensingAstrophysicsStarsGeography

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Publication Info

Year
1996
Type
article
Volume
111
Pages
1748-1748
Citations
2795
Access
Closed

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M. Fukugita, Takashi Ichikawa, James E. Gunn et al. (1996). The Sloan Digital Sky Survey Photometric System. The Astronomical Journal , 111 , 1748-1748. https://doi.org/10.1086/117915

Identifiers

DOI
10.1086/117915