Category Archives: astro-ph

Here are the papers from astro-ph that I find interesting. I tend to update daily, so if there is a day missing, I probably didn’t find any papers relevant to our group.

GPU Papers

  • (abs, pdf) Fluke et al., Astrophysical Supercomputing with GPUs: Critical Decisions for Early Adopters
  • (abs, pdf) Schive et al., GAMER: a GPU-Accelerated Adaptive Mesh Refinement Code for Astrophysics
  • (abs, pdf) Wang et al., Adaptive Mesh Fluid Simulations on GPU
  • (abs, pdf) Jonsson & Primack, Accelerating Dust Temperature Calculations with Graphics Processing Units
  • (abs, pdf) Bédorf et al., A sparse octree gravitational N-body code that runs entirely on the GPU processor

07 Sept 2011

  • (abs, pdf) Kruijssen et al., The dynamical state of stellar structure in star-forming regions
  • (abs, pdf) Revaz & Jablonka, The Dynamical and Chemical Evolution of Dwarf Spheroidal Galaxies with GEAR
  • (abs, pdf) Robertson & Ellis, Connecting the Gamma Ray Burst Rate and the Cosmic Star Formation History: Implications for Reionization and Galaxy Evolution
  • (abs, pdf) Bouwens et al., UV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observations: Discovery of a well-defined UV-color magnitude relationship for z>=4 star-forming galaxies
  • (abs, pdf) Nayakshin et al., Are SMBHs shrouded by “Super-Oort” clouds of comets and asteroids?

02 Sept 2011

  • (abs, pdf) Riebe et al., The MultiDark Database: Release of the Bolshoi and MultiDark Cosmological Simulations
  • (abs, pdf) de la Rosa et al., The link between the Star Formation History and [alpha/Fe]
  • (abs, pdf) Hibon et al., Search for z~6.96 Ly-alpha emitters with Magellan/IMACS in the COSMOS field
  • (abs, pdf) Jiang et al., Keck Spectroscopy of Lyman-break Galaxies and its Implications for the UV-continuum and Ly_alpha Luminosity Functions at z>6
  • (abs, pdf) Li et al., Cosmological evolution of supermassive black holes. I. mass function at 0<z<2
  • (abs, pdf) Forero-Romero et al., Modelling the fraction of Lyman Break Galaxies with strong Lyman alpha emission at 5 < z < 7