Empirical constraints on the first stars and quasars

Haiman Z, Loeb A. 1999. Empirical constraints on the first stars and quasars. AIP Conference Proceedings. 470(1), 34–47.

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Abstract
Empirical studies of the first generation of stars and quasars in the Universe will likely become feasible over the next decade. The Next Generation Space Telescope will provide direct imaging and photometry of sub-galactic objects at (math formular) while microwave anisotropy experiments, such as MAP or Planck, will set constraints on the ionization history of the intergalactic medium due to these sources. We describe the expected signals that will be detectable with these future instruments.
Publishing Year
Date Published
1999-04-27
Journal Title
AIP Conference Proceedings
Publisher
AIP Publishing
Volume
470
Issue
1
Page
34-47
IST-REx-ID

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Haiman Z, Loeb A. Empirical constraints on the first stars and quasars. AIP Conference Proceedings. 1999;470(1):34-47. doi:10.1063/1.58620
Haiman, Z., & Loeb, A. (1999). Empirical constraints on the first stars and quasars. AIP Conference Proceedings. AIP Publishing. https://doi.org/10.1063/1.58620
Haiman, Zoltán, and A. Loeb. “Empirical Constraints on the First Stars and Quasars.” AIP Conference Proceedings. AIP Publishing, 1999. https://doi.org/10.1063/1.58620.
Z. Haiman and A. Loeb, “Empirical constraints on the first stars and quasars,” AIP Conference Proceedings, vol. 470, no. 1. AIP Publishing, pp. 34–47, 1999.
Haiman Z, Loeb A. 1999. Empirical constraints on the first stars and quasars. AIP Conference Proceedings. 470(1), 34–47.
Haiman, Zoltán, and A. Loeb. “Empirical Constraints on the First Stars and Quasars.” AIP Conference Proceedings, vol. 470, no. 1, AIP Publishing, 1999, pp. 34–47, doi:10.1063/1.58620.
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