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The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: IV. Cosmological Implications

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arxiv astro-ph/9806129 v1 pith:VSEKPPON submitted 1998-06-09 astro-ph

E. Dwek , R. G. Arendt , M. G. Hauser , D. Fixsen , T. Kelsall , D. Leisawitz , Y. C. Pei , E. L. Wright
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J. C. Mather S. H. Moseley N. Odegard R. Shafer R. F. Silverberg J. L. Weiland
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classification astro-ph
keywords backgroundcosmologicalinfraredcobeconstraintscosmicdetectiondiffuse
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In this paper we examine the cosmological constraints of the recent DIRBE and FIRAS detection of the extragalactic background light between 125-5000 microns on the metal and star formation histories of the universe.

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  1. Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements

    astro-ph.CO 2025-05 conditional novelty 6.0 of 10

    Galactic dust bias on CMB lensing amplitude is below 0.3σ for ACT but can exceed 0.3σ for Simons Observatory with wide masks, depending on the dust model.

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