Astrophysics from the Highly-Redshifted 21 cm Line

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dc.creatorFurlanetto, Steven
dc.creatorLidz, Adam
dc.creatorLoeb, Abraham
dc.creatorMcQuinn, Matthew
dc.creatorPritchard, Jonathan
dc.creatorAguirre, James
dc.creatorAlvarez, Marcelo
dc.creatorBacker, Donald
dc.creatorBowman, Judd
dc.creatorBurns, Jack
dc.creatorCarilli, Chris
dc.creatorCen, Renyue
dc.creatorCooray, Asantha
dc.creatorGnedin, Nickolay
dc.creatorGreenhill, Lincoln
dc.creatorHaiman, Zoltan
dc.creatorHewitt, Jacqueline
dc.creatorLazio, Joseph
dc.creatorMesinger, Andrei
dc.creatorMadau, Piero
dc.creatorMorales, Miguel
dc.creatorOh, S. Peng
dc.creatorPeterson, Jeffrey
dc.creatorPihlstrom, Ylva
dc.creatorShapiro, Paul
dc.creatorTegmark, Max
dc.creatorTrac, Hy
dc.creatorZahn, Oliver
dc.creatorZaldarriaga, Matias
dc.date2009-02-17
dc.date.accessioned2026-07-07T12:43:25Z
dc.date.available2026-07-07T12:43:25Z
dc.descriptionThe cosmic dark ages and the epoch of reionization, during which the first generations of stars and galaxies formed, are among the most compelling frontiers of extragalactic astrophysics and cosmology. Here we describe an exciting new probe of these eras: the 21 cm line of neutral hydrogen, which will allow us to map the neutral intergalactic medium throughout the era of first galaxy formation. In this white paper, we describe how these studies can answer two key questions about galaxy formation: What were the properties of high-redshift galaxies? How did they affect the Universe around them?
dc.description8 pages, 5 figures, science white paper submitted to the US Astro2010 Decadal Survey "Galaxies across Cosmic Time" Science Frontier Panel
dc.identifierhttps://arxiv.org/abs/0902.3011
dc.identifierhttp://arxiv.org/abs/0902.3011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/220416
dc.subjectCosmology and Nongalactic Astrophysics
dc.titleAstrophysics from the Highly-Redshifted 21 cm Line
dc.typetext

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