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Infrared Surveys: A Golden Age of Exploration

Published online by Cambridge University Press:  25 May 2016

C.A. Beichman
C.A. Beichman*
Affiliation:
Infrared Processing and Analysis Center, Jet Propulsion Laboratory, California Institute of Technology

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The next decade promises an explosion of information about the infrared sky from wavelengths from 1 μm to 1,000 μm, in the continuum and in spectral lines. Measurements of objects ranging from comets in the Kuiper Belt to newly-forming galaxies will be useful for almost every branch of astrophysics. The number of catalogued infrared sources will increase a thousand-fold from the 600,000 presently known from IRAS. This talk addresses the compelling scientific interest of the infrared and describes why, years from now, astronomers will view this decade as a golden era for the exploration of the infrared sky.

Type
Part 1. General Sky Survey Reviews
Information
Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 27 - 40
Copyright
Copyright © Kluwer 1998 

References

Abergel, A. et al. 1996. Astron. Astrophys., 308, L5.Google Scholar
Aumann, H.H., Fowler, J.W. and Melnyk, M. 1990. Astron. J., 99, 1674.Google Scholar
Beichman, et al. 1997. in preparation.Google Scholar
Blitz, L. and Spergel, D.N. 1991. Astrophys. J., 379, 631.CrossRefGoogle Scholar
Bogun, S. et al. 1996. Astron. Astrophys., in press.Google Scholar
Boyle, B. J. and diMatteo, T. 1995. Mon. Not. R. astron. Soc., 277, L63.Google Scholar
Cao, Y., Terebey, S. Prince, T.A. and Beichman, C.A. 1996. Astrophys. J., in press.Google Scholar
Cowie, L.L., Gardner, J.P., Hu, E.M., Songaila, A., Hodapp, K.W. and Wainscoat, R.J. 1994. Astrophys. J., 434, 114.Google Scholar
Djorgovski, G. et al. 1995. Astrophys. J., 438, L13.Google Scholar
Elvis, M., Wilkes, B.J., Mcdowell, J.C., Green, R.F., Bechtold, J., et al. 1994. Astrophys. J. Suppl., 95, 1.Google Scholar
Huang, J.-S., Cowie, L. L., Gardner, J.P., Hu, E.M., Songaila, A. and Wainscot, R. J., 1996. preprint.Google Scholar
Kirkpatrick, D., Beichman, C.A., and Skrutskie, M. 1996. Astrophys. J., in press.Google Scholar
Laureijs, et al. 1996. Astron. Astrophys., in press.Google Scholar
Mera, D., Charbier, G., and Baraffe, I., 1996. Astrophys. J., 459, L87.CrossRefGoogle Scholar
Onaka, T., Yamamura, I., Tanabé, T., Roellig, T. L. and Yuen, L., 1996. preprint.Google Scholar
Skrutskie, et al. 1996. in “The Impact of Large Scale Near-Infrared Surveys”.Google Scholar
Webster, R. L., Francis, P.J., Peterson, B.A., Drinkwater, M.J. and Masci, F.J., 1995. Nature, 375, 469.Google Scholar
Weinberg, M.D., 1992. Astrophys. J., 384, 81.Google Scholar
Wright, E. L. et al. 1991. Astrophys. J., 381, 200.Google Scholar