Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-27T00:20:57.840Z Has data issue: false hasContentIssue false
  • English
  • Français

Studies of the Cosmic Infrared Background with the Space Infrared Telescope Facility (SIRTF)

Published online by Cambridge University Press:  13 May 2016

M. W. Werner ,
William T. Reach  and
M. Rieke
M. W. Werner
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, 91109, USA
William T. Reach
Affiliation:
SIRTF Science Center, California Institute of Technology, Pasadena, CA, 91125, USA
M. Rieke
Affiliation:
Steward Observatory, University of Arizona, Tucson, AZ, 85721, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

IRAS, COBE, and ISO have demonstrated the unique importance of a cryogenic infrared telescope in space for studying diffuse infrared backgrounds and for teasing out the individual point sources which contribute to them. This importance results from the extremely high infrared sensitivity of such telescopes, particularly to diffuse radiation. The next cryogenic infrared telescope will be NASA's Space Infrared Telescope Facility (SIRTF), which is currently in the final stages of construction leading to launch in 2002. SIRTF will be the first infrared space observatory to make extensive use - both for imaging and spectroscopy - of large format infrared detector arrays. The sensitivity and spatial and spectral coverage of SIRTF's array-based instruments endow SIRTF with great power for the study of the cosmic infrared background (CIRB) and related scientific issues. This paper reviews the SIRTF mission design and measurement functionality and describes SIRTF's potential studies of the CIRB, drawing examples from the programs planned by the SIRTF Guaranteed Time Observers (GTO's). We also summarize the opportunities for community participation in SIRTF.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 204: The Extragalactic Infrared Background and its Cosmological Implication , 2001 , pp. 439 - 453
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Dermott, S. F., Jayaraman, S., Xu, Y. L., Gustafson, B. A. S., & Liou, J. C. 1994, Nature, 369, 719 Google Scholar
Devriendt, J. E. G., Guiderdoni, B., & Sadat, R. 1999, A&A, 350, 381 Google Scholar
Dwek, E., & Arendt, R. G. 1998, ApJ, 508, L9 CrossRefGoogle Scholar
Fanson, J. L., Fazio, G. G., Houck, J. R., Kelly, T., Rieke, G. H., Tenerelli, D. J., & Whitten, M. 1998, Proc. SPIE, 3356, 478 CrossRefGoogle Scholar
Franceschini, A., Toffolatti, L., Mazzei, P., Danese, L., & De Zotti, G. 1991, A&A Supp. Ser., 89, 285.Google Scholar
Gorjian, V., Wright, E. L., & Chary, R. R. 2000, ApJ, 536, 550 Google Scholar
Hogg, D. W., Neugebauer, G., Cohen, J. G., Dickinson, M., Djorgovski, S. G., Matthews, K., & Soifer, B. T. 2000, AJ, 119, 1519 Google Scholar
Jayaraman, S., Dermott, S., & Werner, M. 1996, in ASP Conf. Ser. Vol. 104, Physics, Chemistry, and Dynamics of Interplanetary Dust, ed. Gustafson, B. & Hanner, M. (San Francisco: ASP), 159 Google Scholar
Lutz, D., Spoon, H. W. W., Rigopoulou, D., Moorwood, A. F. M., & Genzel, R. 1998, ApJ, 505, 105.CrossRefGoogle Scholar
Reach, W. T., Franz, B. A., Weiland, J. L., Hauser, M. G., Kelsall, T. N., Wright, E. L., Rawley, G., Stemwedel, S. W., & Spiesman, W. J. 1995, Nature, 374, 521 CrossRefGoogle Scholar
Sturm, E., Lutz, D., Tran, D., Feuchtgruber, H., Genzel, R., Kunze, D., Moorwood, A. F. M., & Thornley, M. D. 2000, A&A, 358, 481 Google Scholar
Tan, J. C., Silk, J., & Balland, C. 1999, ApJ, 522, 579 Google Scholar
Wright, E. L. 2000, ApJ, submitted.Google Scholar
Wright, E. L., Werner, M., & Rieke, G. 1995, in AIP Conf. Proc. 348, Unveiling the Cosmic Infrared Background, ed. Dwek, E. (New York: AIP), 278 Google Scholar