(abs , pdf ) Warren, 2HOT: An Improved Parallel Hashed Oct-Tree N-Body Algorithm for Cosmological Simulation
(abs , pdf ) Novak, Local Black Hole Scaling Relations Imply Compton Thick or Super Eddington Accretion
(abs , pdf ) Angulo et al., Extending the halo mass resolution of $N$-body simulations
(abs , pdf ) Hopkins et al., The Meaning and Consequences of Star Formation Criteria in Galaxy Models with Resolved Stellar Feedback
(abs , pdf ) Turk, How to Scale a Code in the Human Dimension
(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
(abs , pdf ) Almgren et al., Nyx: A Massively Parallel AMR Code for Computational Cosmology
(abs , pdf ) Habib et al., The Universe at Extreme Scale: Multi-Petaflop Sky Simulation on the BG/Q
(abs , pdf ) Ibgui et al., IRIS: A Generic Three-Dimensional Radiative Transfer Code
(abs , pdf ) Hassan et al., Tera-scale Astronomical Data Analysis and Visualization
(abs , pdf ) Whalen et al., Finding the First Cosmic Explosions I: Pair-Instability Supernovae
(abs , pdf ) Silk & Mamon, The Current Status of Galaxy Formation
(abs , pdf ) Geisler et al., The Unique Na:O Abundance Distribution in NGC 6791: The First Open(?) Cluster with Multiple Populations
(abs , pdf ) Farris et al., Binary black hole mergers in magnetized disks: simulations in full general relativity
(abs , pdf ) Francis et al., The chemical composition of Ultracompact Dwarf Galaxies in the Virgo and Fornax Clusters
(abs , pdf ) de Barros et al., Properties of z ~ 3 to z ~ 6 Lyman Break Galaxies. I. Impact of nebular emission at high redshift
(abs , pdf ) Mitra et al., Constraining the escape fraction of ionizing photons from high redshift galaxies using data-constrained reionization models
(abs , pdf ) Zhang et al., CASTRO: A New Compressible Astrophysical Solver. III. Multigroup Radiation Hydrodynamics
(abs , pdf ) Shimizu et al., Sub-millimetre galaxies in cosmological hydrodynamic simulations: Source number counts and the spatial clustering
(abs , pdf ) Wang et al., Probing Pre-galactic Metal Enrichment with High-Redshift Gamma-Ray Bursts
(abs , pdf ) Hallenbeck et al., Gas-Bearing Early-Type Dwarf Galaxies in Virgo: Evidence for Recent Accretion
(abs , pdf ) Romanowsky & Fall, Angular momentum and galaxy formation revisited
(abs , pdf ) Simmons et al., Galaxy Zoo: Bulgeless Galaxies With Growing Black Holes
(abs , pdf ) Law et al., High Velocity Dispersion in A Rare Grand Design Spiral Galaxy at Redshift z=2.18
(abs , pdf ) Ren et al., A Search for Metal-poor Stars Pre-enriched by Pair-instability Supernovae I. A Pilot Study for Target Selection from Sloan Digital Sky Survey (SDSS)
(abs , pdf ) Bryan et al., The impact of baryons on the spins and shapes of dark matter haloes
(abs , pdf ) Brammer et al., 3D-HST Grism Spectroscopy of a Gravitationally Lensed, Low-metallicity Starburst Galaxy at z=1.847
(abs , pdf ) Rafelski et al., Metallicity Evolution of Damped Lyman-alpha Systems out to z~5
(abs , pdf ) Vanzella et al., Probing ionizing radiation of L<~0.1L* star-forming galaxies at z>~3 with strong lensing
(abs , pdf ) Laporte et al., The bright-end of the luminosity function at z~9
(abs , pdf ) Hogg, Data analysis recipes: Probability calculus for inference
(abs , pdf ) Peirani et al., Evolution of the baryon fraction in the Local Group: accretion versus feedback at low and high z
(abs , pdf ) Tanvir et al., Star formation in the early universe: beyond the tip of the iceberg
(abs , pdf ) Rafikov, Structure and evolution of circumbinary disks around supermassive black hole (SMBH) binaries
(abs , pdf ) Zheng et al., A highly magnified candidate for a young galaxy seen when the Universe was 500 Myrs old
(abs , pdf ) Dehnen & Aly, New Kernels for SPH
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