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A Survey of Surveys

Published online by Cambridge University Press:  25 May 2016

S. M. Kent
S. M. Kent*
Affiliation:
Fermi National Accelerator Laboratory, MS 127, P. O. Box 500, Batavia, IL 60510 USA †

Abstract

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A new era for the field of Galactic structure is about to be opened with the advent of wide-area digital sky surveys. In this article, I will review the status and prospects for research for 3 new ground-based surveys: the Sloan Digital Sky Survey (SDSS), the Deep Near-Infrared Survey of the Southern Sky (DENIS) and the Two Micron All Sky Survey (2MASS). These surveys will permit detailed studies of Galactic structure and stellar populations in the Galaxy with unprecedented detail. Extracting the information, however, will be challenging.

Type
Chapter 1: Are the Disk and Halo Axisymmetric?
Information
Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 47 - 55
Copyright
Copyright © Kluwer 1996 

References

Bahcall, J.N., and Soneira, R.M. (1980) Astrophys. J. Suppl. 44, 73 CrossRefGoogle Scholar
Blitz, L., and Spergel, D. (1991) Astrophys. J. , 379, 631 CrossRefGoogle Scholar
Boggess, N.W., Mather, J.C., Weiss, R., Bennett, C.L., Cheng, E.S., Dewk, E., Gulkis, S., Hauser, M.G., Janssen, M.A., Kelsall, T., Meyer, S.S., Moseley, S.H., Murdock, T.L., Shafer, R.A., Silverberg, R.F., Smoot, G.F., Wilkinson, D.T., and Wright, E.L. (1992) Astrophys. J. , 397, 420 CrossRefGoogle Scholar
Gilmore, G.F., and Reid, I.N. (1983) Mon. Not. Roy. Astron. Soc. , 202, 1025 CrossRefGoogle Scholar
Habing, H. Astron. Astrophys. , 200, 40 Google Scholar
Hauser, M. (1992) In AIP conference Back to the Galaxy , 201 Google Scholar
Hayakawa, S., Matsumoto, T., Murakami, H., Uyama, K., Thomas, J.A., and Yamagami, T. (1981) Astron. Astrophys. , 100, 116 Google Scholar
Karawa, K., Kozasa, T., and Sato, S. (1982) Publ. Astron. Jap. 34, 389 Google Scholar
Kent, S.M., Dame, T.M., and Fazio, G. (1991) Astrophys. J. , 378, 131.CrossRefGoogle Scholar
Kron, R.G. (1980) Astrophys. J. Suppl. , 43, 305 CrossRefGoogle Scholar
Ortiz, R., and Lepine, R.D. (1993) Astron. Astrophys. , 279, 90 Google Scholar
Paczynski, B., Stanek, K.Z., Udalski, A., Szymanski, M., Kaluzny, J., Kubiak, M., Mateo, M., and Krzeminski, W. (1994) preprint Google Scholar
Reid, N., and Majewski, S.R. (1993) Astrophys. J. , 409, 635 CrossRefGoogle Scholar
Robin, A.C., and Creze, M. (1986) Astron. Astrophys. , 157, 71 Google Scholar
Ruelas-Mayora, R.A. (1991a) Rev. Mexicana Astron. Astrophys , 22, 27 Google Scholar
Ruelas-Mayora, R.A. (1991b) Rev. Mexicana Astron. Astrophys , 22, 43 Google Scholar
Wainscoat, R.J., Cohen, M., Volk, K., Walker, H.J., and Schwartz, D.E. (1992) Astrophysical Journal Supplement 83, 111 CrossRefGoogle Scholar
Weinberg, M. (1992) Astrophys. J. , 384, 81 CrossRefGoogle Scholar