Tag Archives: Bfield

18 Oct 2017

  • (abs, pdf) Kocevski et al., CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z~2
  • (abs, pdf) Metzger, Welcome to the Multi-Messenger Era! Lessons from a Neutron Star Merger and the Landscape Ahead
  • (abs, pdf) Su et al., Stellar feedback strongly alters the amplification and morphology of galactic magnetic fields
  • (abs, pdf) Hogg & Foreman-Mackey, Data analysis recipes: Using Markov Chain Monte Carlo
  • (abs, pdf) Behrens et al., The impact of Lyman-$\alpha$ radiative transfer on large-scale clustering in the Illustris simulation

29 Aug 2017

  • (abs, pdf) Grand et al., Origin of chemically distinct discs in the Auriga cosmological simulations
  • (abs, pdf) Faisst et al., Are high redshift Galaxies hot? – Temperature of z > 5 Galaxies and Implications on their Dust Properties
  • (abs, pdf) Mao et al., Detection of microgauss coherent magnetic fields in a galaxy five billion years ago
  • (abs, pdf) Villanueva-Domingo et al., Warm Dark Matter and Cosmic Reionization

13 Jul 2017

  • (abs, pdf) Nelson et al., First results from the IllustrisTNG simulations: the galaxy color bimodality
  • (abs, pdf) Marinacci et al., First results from the IllustrisTNG simulations: radio haloes and magnetic fields
  • (abs, pdf) Springel et al., First results from the IllustrisTNG simulations: matter and galaxy clustering
  • (abs, pdf) Naiman et al., First results from the IllustrisTNG simulations: A tale of two elements — chemical evolution of magnesium and europium
  • (abs, pdf) Pillepich et al., First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
  • (abs, pdf) Hirata et al., Detecting primordial gravitational waves with circular polarization of the redshifted 21 cm line: I. Formalism
  • (abs, pdf) Mishra & Hirata, Detecting primordial gravitational waves with circular polarization of the redshifted 21 cm line: II. Forecasts
  • (abs, pdf) Byun et al., Benchmarking Data Analysis and Machine Learning Applications on the Intel KNL Many-Core Processor

21 Apr 2017

  • (abs, pdf) Rieder & Teyssier, A small-scale dynamo in feedback-dominated galaxies – II. The saturation phase and the final magnetic configuration
  • (abs, pdf) Puschnig et al., The Lyman Continuum Escape and ISM properties in Tololo 1247-232 – New Insights from HST and VLA
  • (abs, pdf) Mould et al., Detection of a possible superluminous supernova in the epoch of reionization
  • (abs, pdf) Ono et al., Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z \sim 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ Sky
  • (abs, pdf) Sakurai et al., Formation of Intermediate-Mass Black Holes through Runaway Collisions in the First Star Clusters

02 Mar 2017

  • (abs, pdf) Ng et al., Offsets between member galaxies and dark matter in clusters: a test with the Illustris simulation
  • (abs, pdf) Turner et al., A comparison of observed and simulated absorption from HI, CIV, and SiIV around $z\approx2$ star-forming galaxies suggests redshift-space distortions are due to inflows
  • (abs, pdf) Parker et al., The response of relativistic outflowing gas to the inner accretion disk of a black hole
  • (abs, pdf) Grazian et al., The Lyman Continuum escape fraction of faint galaxies at z~3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC
  • (abs, pdf) Thompson, Tiny Electromagnetic Explosions
  • (abs, pdf) Thompson, Giant Primeval Magnetic Dipoles

22 Feb 2017

  • (abs, pdf) Gallerani et al., Physical properties of the first quasars
  • (abs, pdf) Weisz & Boylan-Kolchin, Local Group Ultra-Faint Dwarf Galaxies in the Reionization Era
  • (abs, pdf) Mocz et al., Moving mesh simulations of star forming cores in magneto-gravo-turbulence
  • (abs, pdf) Vijayaraghavan & Ricker, The Co-Evolution of a Magnetized Intracluster Medium and Hot Galactic Coronae: Magnetic Field Amplification and Turbulence Generation
  • (abs, pdf) Hopkins et al., FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation