Name: Cosmic Radiation Fields - Sources in the early Universe
Start: 2010-11-10T08:00:00+01:00
End: 2010-11-12T18:00:00+01:00
Location: Desy-Campus

Cosmic Radiation Fields - Sources in the early Universe

from Wednesday 10 November 2010 (08:00) to Friday 12 November 2010 (18:00)

Monday 8 November 2010
Tuesday 9 November 2010
Wednesday 10 November 2010

08:30 Registration
Registration
08:30 - 09:15
Room: Auditorium (Building 05)

09:15 Welcome
Welcome
09:15 - 09:30
Room: Auditorium (Building 05)
09:30
09:30 - 11:00
Room: Auditorium (Building 05)
Contributions

09:30 First stars and cosmic reionization - Andrea Ferrara (Scuola Normale Superiore)

10:00 Cosmic reionization and the LOFAR project - Benedetta Ciardi (Max Planck Institute for Astrophysics)

10:30 Pointing the James Webb Space Telescope through lensing clusters - can the first stars and galaxies be detected? - Erik Zackrisson (Stockholm Observatory)
11:00 Coffee break
Coffee break
11:00 - 11:30
Room: Auditorium (Building 05)
11:30
11:30 - 12:30
Room: Auditorium (Building 05)
Contributions

11:30 How the first generations of luminous baryons established the X-ray and UV backgrounds - Andrei Mesinger (Princeton University)

11:50 Observational Signatures of Lyman Alpha Emission from Early Galaxy Formation. - Mark Dijkstra (MPA Garching)

12:10 Dark Matter effects on high-redshift universe - Carmelo Evoli (SISSA/ISAS, Trieste, Italy)
12:30 Lunch break
Lunch break
12:30 - 14:00
Room: Auditorium (Building 05)
14:00
14:00 - 15:20
Room: Auditorium (Building 05)
Contributions

14:00 Formation of the First Galaxies - John Wise (Princeton University)

14:20 The effect of dust cooling in the fragmentation of star-forming clouds for the transition from Pop. III to Pop. II - Gustavo Dopcke (ITA - Universität Heidelberg)

14:40 The role of magnetic fields during primordial star formation - Dominik Schleicher (ALMA ARC node Leiden)

15:00 The generation of strong magnetic fields during the formation of the first stars - Sharanya Sur (Institute for Theoretical Astrophysics (ITA), Univ. of Heidelberg)
15:20 Coffee break
Coffee break
15:20 - 16:00
Room: Auditorium (Building 05)
16:00
16:00 - 17:20
Room: Auditorium (Building 05)
Contributions

16:00 The effects of accretion luminosity from Pop III protostars - Rowan J Smith (ITA, University of Heidelberg)

16:20 The Stellar Initial Mass Function in Low-Metallicity Gas - Simon Glover (Institute for Theoretical Astrophysics, Heidelberg)

16:40 Model atmospheres for Dark Stars - Peter Hauschildt (Hamburger Sternwarte)
Thursday 11 November 2010
09:30
09:30 - 11:00
Room: Auditorium (Building 05)
Contributions

09:30 Dark matter and the first stars - Fabio Iocco (Institut d'Astrophysique de Paris)

10:00 Dark stars: structure, evolution and impacts upon the high-redshift Universe - Pat Scott (McGill University)

10:30 tba - Emanuele Ripamonti (Universita' di Milano-Bicocca)
11:00 Coffe break
Coffe break
11:00 - 11:30
Room: Auditorium (Building 05)
11:30
11:30 - 12:30
Room: Auditorium (Building 05)
Contributions

11:30 The Redshift Evolution of LCDM Halo Parameters - Juan Carlos Munoz Cuartas (Astrophysikalisches Institut Potsdam)

11:50 Thermal decoupling of WIMPS: The link between particle physics properties and the small-scale structure of (dark) matter - Torsten Bringmann (Hamburg University)

12:10 Constraints on dark matter powered stars from the extragalactic background light - Andreas Maurer (Institute for Experimental Physics, University of Hamburg)
12:30 Lunch break
Lunch break
12:30 - 14:00
Room: Auditorium (Building 05)
14:00
14:00 - 15:20
Room: Auditorium (Building 05)
Contributions

14:00 Galaxy Evolution and Background Radiations in the Infrared - Alberto FRANCESCHINI

14:30 Galaxy Build-up and Evolution at z>=7: Early results from ultra-deep WFC3/IR observations over the HUDF and GOODS fields - Rychard Bouwens Bouwens (Leiden University)

15:00 Understanding the Cosmic Infrared Background - Elizabeth Fernandez (Institut d'astrophysique spatiale)
15:20 Coffee break
Coffee break
15:20 - 16:00
Room: Auditorium (Building 05)
16:00
16:00 - 17:30
Room: Auditorium (Building 05)
Contributions

16:00 Measurements of the spectral energy distribution of the cosmic infrared background - Matthieu Bethermin (IAS (Orsay, France))

16:30 The Resolved Near-Infrared Extragalactic Background - Ryan Keenan (University of Wisconsin, Madison)

16:50 Herschel/PEP resolves the far-IR background - Stefano Berta (Max Planck Institut fuer Extraterrestrische Physik)

17:10 AKARI observation of the fluctuation of the near-infrared background - Toshio Matsumoto (Department of Physics and Astronomy, Seoul National University)
Friday 12 November 2010
09:30
09:30 - 10:50
Room: Auditorium (Building 05)
Contributions

09:30 Constraints on the gamma-ray opacity of the Universe with the Fermi-LAT instrument - Anita Reimer (Institut für Theoretische Physik, Universität Innsbruck, Austria)

10:00 Constraints on Extragalactic Background Light using very high energy gamma rays - Daniel Mazin (IFAE, Barcelona)

10:30 Gamma-ray opacity and the high-redshift UV background - Rudy Gilmore (SISSA)
10:50 Coffee break
Coffee break
10:50 - 11:30
Room: Auditorium (Building 05)
11:30
11:30 - 13:00
Room: Auditorium (Building 05)
Contributions

11:30 TeV blazars and their distance - Elisa Prandini (Padova University & INFN)

11:50 Measuring Light from the Epoch of Reionization with CIBER, the Cosmic Infrared Background Experiment - Michael Zemcov (California Institute of Technology/Jet Propulsion Laboratory)

12:10 Conference summary - Martin Raue (Institute for Experimental Physics, University of Hamburg)

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