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Muti-Color Imaging of Clusters of Galaxies with Mosaic CCD Cameras

  • S. Okamura (a1), M. Doi (a1), N. Kashikawa (a2), W. Kawasaki (a1), Y. Komiyama (a1), M. Sekiguchi (a2), K. Shimasaku (a1), M. Yagi (a1) and N. Yasuda (a1)...

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At present, the photometric data for clusters at z ≲ 0.2 mainly come from photographic photometry. The lack of CCD data for such clusters is simply due to the fact that no CCD camera had been available until recently that covers the wide extension of clusters within a reasonable amount of observing time. We have developed a large mosaic CCD camera and conducted multicolor imaging observations of z ≲ 0.2 clusters using the 40-inch Swope telescope at Las Campanas Observatory.

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References

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Doi, M., Fukugita, M., & Okamura, S. 1993, Mon. Not. R. astron. Soc., 264, 832.
Kashikawa, N. et al. 1995a, in “Scientific and Engineering Frontiers for 8–10m Telescopes,” eds. Iye, M. and Nishimura, T. (Tokyo: Universal Academy Press), pp. 105110.
Kashikawa, N. et al. 1995b, Astrophys. J., 452, L99.
Sekiguchi, M. et al. 1992, Publ. Astron. Soc. Pacific, 104, 744.

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