Hostname: page-component-745bb68f8f-5r2nc Total loading time: 0 Render date: 2025-01-13T11:00:34.927Z Has data issue: false hasContentIssue false
  • English
  • Français

Future Cosmic Microwave and Cosmic Infrared Background Measurements

Published online by Cambridge University Press:  25 May 2016

John C. Mather
John C. Mather*
Affiliation:
Code 685, Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771, 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.

Cosmic microwave and infrared background radiation (CMBR and CIBR) measurements in the near future have the potential to greatly advance our knowledge of the early universe. New instrument and space technology will soon enable much better measurements of both.

Type
Part I: Invited Reviews
Information
Symposium - International Astronomical Union , Volume 168: Examining the Big Bang and the Diffuse Background Radiations , 1996 , pp. 419 - 421
Copyright
Copyright © Kluwer 1996 

References

Bennett, C. L. et al., 1992, ApJ, 396, L7.Google Scholar
Bennett, C. L., et al., 1994, ApJ, 436, 423–442.CrossRefGoogle Scholar
Dwek, E., and Slavin, J., 1994, ApJ, 436, 696–704.Google Scholar
Mather, J. C. et al., 1994, ApJ, 420, 439–444.CrossRefGoogle Scholar
Smoot, G. F. et al., 1992, ApJ, 396, L1.Google Scholar
Stecker, F.W., & Dejager, O.C., 1993, ApJ, 415, L71.CrossRefGoogle Scholar
Wright, E. L. et al., 1992, ApJ, 396, L13.Google Scholar