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JHK Photometry of Extragalactic Sources Using an Infrared Array Camera

Published online by Cambridge University Press:  07 August 2017

I. S. McLean
Affiliation:
Department of Physics and Astronomy, UCLA
T. Liu
Affiliation:
Department of Physics and Astronomy, UCLA
H. Teplitz
Affiliation:
Department of Physics and Astronomy, UCLA

Abstract

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The UCLA two-channel IR camera has been used to perform crowded-field photometry in two distinct classes of extragalactic objects. DAOPHOT was used to reduce images of M 33 and provide JHK color-magnitude diagrams of over 1,700 stars. Galaxy photometry in crowded clusters, e.g. Abell 370, was obtained in JHK and analyzed using FOCAS. In both cases, extensive reductions were performed using synthetic aperture photometry for comparison. Methods and results are summarized.

Type
Section II — Poster Papers
Copyright
Copyright © Kluwer 1995 

References

McLean, I. S., Becklin, E. E., Brims, G., Canfield, J., Casement, L. S., Figer, D. F., Henriquez, F., Huang, A., Liu, T., Macintosh, B. and Teplitz, H. 1993 Proc. SPIE 1946, Infrared Detectors and Instrumentation, Fowler, A. M., ed., p. 513.Google Scholar
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