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Radio astronomical probes of Cosmic Reionization and the 1 st luminous objects

Radio astronomical probes of Cosmic Reionization and the 1 st luminous objects Chris Carilli March 19, 2007 University of Colorado. Brief introduction to cosmic reionization

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746 views • 64 slides

Radio astronomical probes of Cosmic Reionization and the 1 st luminous objects

Radio astronomical probes of Cosmic Reionization and the 1 st luminous objects Chris Carilli, NRL, April 2008. Brief introduction to cosmic reionization

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710 views • 60 slides

History of IGM

History of IGM. Epoch of Reionization (EoR). bench-mark in cosmic structure formation indicating the first luminous structures. z=5.80. z=5.82. z=5.99. z=6.28. The Gunn Peterson Effect. Fast reionization at z =6.3 => opaque at l _obs <0.9 m m. f(HI) > 0.001 at z = 6.3.

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655 views • 50 slides

A Sub-mm View of Debris Disks: The case for CCAT exploration

A Sub-mm View of Debris Disks: The case for CCAT exploration. ? Corvi Wyatt et al. (2005). 450 ?m. 850 ?m. Sally Dodson-Robinson University of Texas. Spitzer 160 ?m. HD 207129: 16 pc 152-158 mJy HD 10647: 17 pc 451-462 mJy HD 115617 (not shown): 8.5 pc 89-141 mJy

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164 views • 8 slides

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Radio astronomical probes of Cosmic Reionization and the 1 st luminous objects

Radio astronomical probes of Cosmic Reionization and the 1 st luminous objects

History of IGM

A Sub-mm View of Debris Disks: The case for CCAT exploration