22 May 2013
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Tag Archives: Reion
25 Apr 2013
- (abs, pdf) Zackrisson et al., The spectral evolution of the first galaxies. II. Spectral signatures of Lyman continuum leakage from galaxies in the reionization epoch
- (abs, pdf) Narayanan, Star Formation in High-Redshift Starburst Galaxies
- (abs, pdf) Heß et al., Simulating Structure Formation of the Local Universe
18-24 Apr 2013
- (abs, pdf) Johnson et al., The Biggest Explosions in the Universe
- (abs, pdf) Vera-Ciro & Helmi, Constraints on the shape of the Milky Way dark matter halo from the Sagittarius stream
- (abs, pdf) Weber et al., Three-Dimensional Modelling of Ionized Gas. I. Did very massive stars of different metallicities drive the second cosmic reionization?
- (abs, pdf) Parsons et al., New Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IGM at z=7.7
- (abs, pdf) Kirby et al., Segue 2: The Least Massive Galaxy
29 Mar 2013
25 Mar 2013
- (abs, pdf) Pfrommer, Toward a comprehensive model for feedback by active galactic nuclei: new insights from M87 observations by LOFAR, Fermi and H.E.S.S
- (abs, pdf) Fu et al., Star Formation and Metallicity Gradients in Semi-analytic Models of Disk Galaxy Formation
- (abs, pdf) Jensen et al., Probing reionization with LOFAR using 21-cm redshift space distortions
14 Mar 2013
30 Jan 2013
- (abs, pdf) Fernandez & Zaroubi, The End of an Era – The Population III to Population II Transition and the Near Infrared Background
- (abs, pdf) Sobacchi & Mesinger, How does radiative feedback from a UV background impact reionization?
- (abs, pdf) Sobacchi & Mesinger, The depletion of gas in high-redshift dwarf galaxies from an inhomogeneous reionization
- (abs, pdf) Nelson et al., Moving mesh cosmology: tracing cosmological gas accretion
23 Jan 2013
- (abs, pdf) Moller et al., Mass-metallicity relation from z=5 to the present: Mass-metallicity relation from z=5 to the present: Evidence for a transition in the mode of galaxy growth at z=2.6 due to the end of sustained primordial gas infall
- (abs, pdf) Jaacks et al., Impact of H_2-based star formation model on the z>=6 luminosity function and the ionizing photon budget for reionization