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UC Irvine Center for Cosmology –

UC Irvine Center for Cosmology. High redshift galaxy spectra unveiling the nature of galaxy formation are available via the world's most powerful telescopes at the Keck Observatory. Set in the Antarctic, ARIANNA is an exciting new experiment that pushes the boundaries of ultra-high energy neutrino physics to new limits, attempting to understand some of the most fundamental characteristics of our universe. Particle Physics and Cosmology. The Center for Cosmology is devoted to unlocking the mysteries of ou...

http://cosmology.uci.edu/

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UC Irvine Center for Cosmology – | cosmology.uci.edu Reviews
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UC Irvine Center for Cosmology. High redshift galaxy spectra unveiling the nature of galaxy formation are available via the world's most powerful telescopes at the Keck Observatory. Set in the Antarctic, ARIANNA is an exciting new experiment that pushes the boundaries of ultra-high energy neutrino physics to new limits, attempting to understand some of the most fundamental characteristics of our universe. Particle Physics and Cosmology. The Center for Cosmology is devoted to unlocking the mysteries of ou...
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UC Irvine Center for Cosmology – | cosmology.uci.edu Reviews

https://cosmology.uci.edu

UC Irvine Center for Cosmology. High redshift galaxy spectra unveiling the nature of galaxy formation are available via the world's most powerful telescopes at the Keck Observatory. Set in the Antarctic, ARIANNA is an exciting new experiment that pushes the boundaries of ultra-high energy neutrino physics to new limits, attempting to understand some of the most fundamental characteristics of our universe. Particle Physics and Cosmology. The Center for Cosmology is devoted to unlocking the mysteries of ou...

INTERNAL PAGES

cosmology.uci.edu cosmology.uci.edu
1

Science Magazine: Rogue stars outside galaxies may be everywhere

http://cosmology.uci.edu/2014/11/06/science-magazine-rogue-stars-outside-galaxies-may-be-everywhere

UC Irvine Center for Cosmology. Science Magazine: Rogue stars outside galaxies may be everywhere. November 6, 2014. By Kevork N. ABAZAJIAN. Reports in an article. On UCI Prof. Asantha Cooray. And CalTech Prof. Jamie Bock. 8216;s Cosmic Infrared Background ExpeRiment (CIBER). Experiment’s result finding extragalactic background light from plenty of rogue stars lighting up the space between galaxies. Cosmology Center Graduate Student Receives Burke Postdoctoral Fellow at CalTech. X000B7; Log in.

2

Alumni

http://cosmology.uci.edu/alumni

UC Irvine Center for Cosmology. Past Postdoctoral Scholars include. CGE Fellow 2010-13) – Faculty at University of Texas, Austin. McCue Fellow 2013-15) – Faculty at University of Texas, Austin. Hubble Fellow 2010-12) – Faculty at University of California, Irvine. McCue Fellow 2006-09) – ARC Future Fellow at Swinburne. 2011-13) – Faculty at University of Iowa. JSPS Fellow / McCue Fellow 2012-14) – Faculty at Virginia Tech. CGE Fellow 2012-14) – Faculty at CalTech. Rachel Kuzio de Naray. Bright light may n...

3

McCue Fellows

http://cosmology.uci.edu/mccue-fellows

UC Irvine Center for Cosmology. As a McCue Fellow, Shunsaku performed research on high-energy astrophysics and its interface with particle physics. He worked on high-energy signatures of supernova explosions and particle dark matter annihilation. He also explored the detectability of such signatures with astronomical observations. Shunsaku’s work as a McCue Fellow helped him secure a faculty position at Virginia Tech. Where he started as an Assistant Professor in 2014. 2010 – 2012. Alex studied the polar...

4

People

http://cosmology.uci.edu/people

UC Irvine Center for Cosmology. UCI’s Cosmology Center is guided by our Executive Board. Play a central role. McCue Postdoctoral Research Fellows. Graduate and Postdoctoral Alumni. Cosmology Center Graduate Student Receives Burke Postdoctoral Fellow at CalTech. Bright light may not be dark matter’s smoking gun after all New Scientist features UCI Center for Cosmology work. Postdoc(s) in Theoretical Particle Physics, Astroparticle Physics and Cosmology at UC Irvine. X000B7; Log in.

5

APS PRL Viewpoint: X-Ray Line May Have Dark Matter Origin

http://cosmology.uci.edu/2014/12/15/aps-prl-viewpoint-x-ray-line-may-have-dark-matter-origin

UC Irvine Center for Cosmology. APS PRL Viewpoint: X-Ray Line May Have Dark Matter Origin. December 15, 2014. By Kevork N. ABAZAJIAN. Prof Abazajian wrote a general physics perspective viewpoint. On the two groups that have detected an unidentified 3.5 keV X-ray line that is consistent with dark matter decay. One group, Bulbul et al. (2014),. Has detected the line in two independent. XMM-Newton X-ray Space Telescope. Stacked cluster observations, and in the Perseus cluster with. X000B7; Log in.

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Michael C. Cooper

http://localgroup.ps.uci.edu/cooper

Michael C. Cooper. University of California Irvine. Michael C. Cooper. Department of Physics and Astronomy. University of California Irvine. Office: 2123 Reines Hall. Cooper -at- uci.edu. Center for Galaxy Evolution. DEEP2 Data Release 1. DEEP2 Data Release 2. DEEP2 Data Release 3. DEEP2 Data Release 4. DEEP3 Preliminary Data Release. Arizona CDFS Environment Survey. IMACS Spectroscopy of UDS/COSMOS. DEEP2 DEIMOS Data Pipeline.

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UC Irvine Center for Cosmology –

UC Irvine Center for Cosmology. High redshift galaxy spectra unveiling the nature of galaxy formation are available via the world's most powerful telescopes at the Keck Observatory. Set in the Antarctic, ARIANNA is an exciting new experiment that pushes the boundaries of ultra-high energy neutrino physics to new limits, attempting to understand some of the most fundamental characteristics of our universe. Particle Physics and Cosmology. The Center for Cosmology is devoted to unlocking the mysteries of ou...

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This is the home of the UCSD cosmology research group. We currently do research on the cosmic microwave background (CMB) and the near-infrared background (NIRB). For a list of the projects we are working on, go to the projects. Brian Keating and Kam Arnold's Cosmology Group. This material is based upon work supported by the following foundations. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect their views.

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