Tag Archives: UDG

07 Aug 2020

  • (abs, pdf) Hayashi et al., Probing Dark Matter Self-interaction with Ultra-faint Dwarf Galaxies
  • (abs, pdf) Greig et al., Exploring reionisation and high-z galaxy observables with recent multi-redshift MWA upper limits on the 21-cm signal
  • (abs, pdf) Ghosh et al., Axion Gegenschein: Probing Back-scattering of Astrophysical Radio Sources Induced by Dark Matter

23 Jul 2020

  • (abs, pdf) Diemer, Fly-bys, orbits, splashback: subhalos and the importance of the halo boundary
  • (abs, pdf) Hemler et al., Gas-phase metallicity gradients of TNG50 star-forming galaxies
  • (abs, pdf) Blaña et al., Dwarfs in the Milky Way halo outer rim: first in-fall or backsplash satellites?
  • (abs, pdf) Aguado et al., The S2 Stream: the shreds of a primitive dwarf galaxy
  • (abs, pdf) Rathi et al., "Observations" of simulated dwarf galaxies: Star-formation histories from color-magnitude diagrams
  • (abs, pdf) Iodice et al., The first detection of ultra-diffuse galaxies in the Hydra I cluster from VEGAS survey

21 Jul 2020

  • (abs, pdf) Diemer, The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
  • (abs, pdf) Lu et al., The Effect of Supernovae on the Turbulence and Dispersal of Molecular Clouds
  • (abs, pdf) Lagos et al., Physical properties and evolution of (Sub-)millimeter selected galaxies in the galaxy formation simulation Shark
  • (abs, pdf) Shin et al., Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations

01 May 2020

  • (abs, pdf) Ayromlou et al., Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
  • (abs, pdf) Piña et al., Robust HI kinematics of gas-rich ultra-diffuse galaxies: hints of a weak-feedback formation scenario
  • (abs, pdf) Simons et al., Figuring Out Gas & Galaxies In Enzo (FOGGIE). IV. The Stochasticity of Ram Pressure Stripping in Galactic Halos
  • (abs, pdf) Gronke et al., Lyman-alpha transmission properties of the intergalactic medium in the CoDaII simulation

27 Apr 2020

  • (abs, pdf) Bonaca et al., Timing the Early Assembly of the Milky Way with the H3 Survey
  • (abs, pdf) Kovacs et al., Ultra-diffuse galaxies in the Coma cluster: Probing their origin and AGN occupation fraction
  • (abs, pdf) Merritt et al., A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
  • (abs, pdf) Santos-Santos et al., Planes of satellites around simulated disc galaxies: I.- Finding high-quality planar configurations from positional information and their comparison to MW/M31 data

22 Apr 2020

  • (abs, pdf) Taylor et al., The Ultraluminous Lyman Alpha Luminosity Function at z=6.6
  • (abs, pdf) Sommovigo et al., Warm dust in high-z galaxies: origin and implications
  • (abs, pdf) Rey et al., EDGE: From quiescent to gas-rich to star-forming low-mass dwarf galaxies
  • (abs, pdf) Lu et al., ALMA Observations of Massive Clouds in the Central Molecular Zone: Jeans Fragmentation and Cluster Formation
  • (abs, pdf) Cardona-Barrero et al., NIHAO XXIV: Rotation or pressure supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics

29 Jan 2020

  • (abs, pdf) Gaikwad et al., Probing the thermal state of the intergalactic medium at $z>5$ with the transmission spikes in high-resolution Ly$\alpha$ forest spectra
  • (abs, pdf) Forbes et al., Globular Clusters in Coma Cluster Ultra Diffuse Galaxies (UDGs): Evidence for Two Types of UDG?
  • (abs, pdf) Woosley et al., The Birth Function for Black Holes and Neutron Stars in Binaries

10 Jan 2020

  • (abs, pdf) Keto et al., A Turbulent-Entropic Instability and the Fragmentation of Star-Forming Clouds
  • (abs, pdf) Trujillo et al., A physically motivated definition for the size of galaxies in an era of ultra-deep imaging
  • (abs, pdf) Chamba et al., Are ultra-diffuse galaxies Milky Way-sized?
  • (abs, pdf) Nanayakkara et al., Reconstructing the observed ionizing photon production efficiency at z~2 using stellar population models
  • (abs, pdf) Shen et al., The Bolometric Quasar Luminosity Function at z = 0-7