Tag Archives: UDG

03 Nov 2022

  • (abs, pdf) Jones et al., Gas-rich, field ultra-diffuse galaxies host few globular clusters
  • (abs, pdf) Hahn et al., ${\rm S{\scriptsize IM}BIG}$: A Forward Modeling Approach To Analyzing Galaxy Clustering
  • (abs, pdf) Capelo et al., Black hole-galaxy co-evolution and the role of feedback
  • (abs, pdf) da Cunha, The dust properties of star-forming galaxies in the first billion years
  • (abs, pdf) Saldana-Lopez et al., The VANDELS survey: the ionizing properties of star-forming galaxies at $3 \leq z \leq 5$ using deep rest-frame ultraviolet spectroscopy

28 Oct 2022

  • (abs, pdf) Di Matteo et al., A vast population of wandering and merging IMBHs at cosmic noon
  • (abs, pdf) Li et al., Beyond Ultra-Diffuse Galaxies I: Mass-Size Outliers Among the Satellites of Milky Way Analogs
  • (abs, pdf) Rácz et al., Complementary Cosmological Simulations
  • (abs, pdf) Rino-Silvestre et al., EmulART: Emulating Radiative Transfer – A pilot study on autoencoder based dimensionality reduction for radiative transfer models
  • (abs, pdf) Roberts-Borsani et al., A shot in the Dark (Ages): a faint galaxy at $z=9.76$ confirmed with JWST

19-23 Sept 2022

  • (abs, pdf) Mugnai & Modirrousta-Galian, RAPOC : the Rosseland and Planck opacity converter. A user-friendly and fast opacity program for Python
  • (abs, pdf) Benavides et al., Origin and evolution of ultra-diffuse galaxies in different environments
  • (abs, pdf) Katz & Krassner, 3 MHz Space Observatory
  • (abs, pdf) Wang et al., Towards Super-resolution via Iterative multi-exposure Coaddition
  • (abs, pdf) Satyavolu et al., The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization
  • (abs, pdf) Choudhury, A Short Introduction to Reionization Physics
  • (abs, pdf) Chang et al., Report of the Topical Group on Cosmic Frontier 5 Dark Energy and Cosmic Acceleration: Cosmic Dawn and Before for Snowmass 2021
  • (abs, pdf) Filion et al., Faint Stars in a Faint Galaxy: II. The Low Mass Stellar Initial Mass Function of the Bo\"otes I Ultrafaint Dwarf Spheroidal Galaxy
  • (abs, pdf) Yamaguchi et al., The extent of metal enrichment from galactic winds during the Cosmic Dawn
  • (abs, pdf) Gültekin et al., Intermediate-mass black holes and the fundamental plane of black hole accretion

24 Aug 2022

  • (abs, pdf) Hu et al., Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback:\\ Lagrangian vs. Eulerian Methods
  • (abs, pdf) Raghuvanshi & Dutta, Simulating the collapse of rotating primordial gas clouds to study the survival possibility of Pop III protostars
  • (abs, pdf) Webb et al., Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
  • (abs, pdf) Sarbadhicary et al., Testing the Momentum-driven Supernova Feedback Paradigm in M31

18 Jul 2022

  • (abs, pdf) van Dokkum et al., Monochromatic globular clusters as a critical test of formation models for the dark matter deficient galaxies NGC1052-DF2 and NGC1052-DF4
  • (abs, pdf) Tang & Turk, Reduced Order Model for Chemical Kinetics: A case study with Primordial Chemical Network
  • (abs, pdf) Sarmento & Scannapieco, The Effects of Radiative Feedback and Supernova Induced Turbulence on Early Galaxies

19 May 2022

  • (abs, pdf) Collins & Read, Observational constraints on stellar feedback in dwarf galaxies
  • (abs, pdf) van Dokkum et al., A trail of dark matter-free galaxies from a bullet dwarf collision
  • (abs, pdf) Bordoloi et al., Resolving the HI in Damped Lyman-{\alpha} systems that power star-formation
  • (abs, pdf) Bisbas et al., The origin of the [CII]-deficit in a simulated dwarf galaxies starburst
  • (abs, pdf) Karpov et al., Physics-Informed Machine Learning for Modeling Turbulence in Supernovae

18 May 2022

  • (abs, pdf) Chiaki & Wise, Triggered Population III star formation: the effect of H$_2$ self-shielding
  • (abs, pdf) Schatz et al., Horizons: Nuclear Astrophysics in the 2020s and Beyond
  • (abs, pdf) Piras et al., Fast and realistic large-scale structure from machine-learning-augmented random field simulations
  • (abs, pdf) Ricotti et al., Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
  • (abs, pdf) Zier & Springel, Simulating cold shear flows on a moving mesh
  • (abs, pdf) Seitova & Pober, The Optical Depth of Foregrounds for the Highest Redshift 21 cm Signals

21 Apr 2022

  • (abs, pdf) Naidu et al., Live Fast, Die $\alpha$-Enhanced: The Mass-Metallicity-$\alpha$ Relation of the Milky Way's Disrupted Dwarf Galaxies
  • (abs, pdf) Collins et al., Pegasus V — a newly discovered ultra-faint dwarf galaxy on the outskirts of Andromeda
  • (abs, pdf) Klepitko et al., Tree-based solvers for adaptive mesh refinement code FLASH — III: a novel scheme for radiation pressure on dust and gas and radiative transfer from diffuse sources

12 Nov 2021

  • (abs, pdf) Connor et al., X-Ray Evidence Against the Hypothesis that the Hyper-Luminous z=6.3 Quasar J0100+2802 is Lensed
  • (abs, pdf) Schaurecker et al., Super-resolving Dark Matter Halos using Generative Deep Learning
  • (abs, pdf) Errani et al., Structure and kinematics of tidally limited satellite galaxies in LCDM
  • (abs, pdf) Gannon et al., Ultra-Diffuse Galaxies in the Perseus Cluster: Comparing Galaxy Properties with Globular Cluster System Richness

23 Sept 2021

  • (abs, pdf) Villaescusa-Navarro et al., Multifield Cosmology with Artificial Intelligence
  • (abs, pdf) García-Vergara et al., ALMA reveals large overdensity and strong clustering of galaxies in quasar environments at $z\sim4$
  • (abs, pdf) Stücker et al., Simulating the complexity of the dark matter sheet II: halo and subhalo mass functions for non-cold dark matter models
  • (abs, pdf) Hopkins et al., First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations
  • (abs, pdf) Keim et al., Tidal Distortions in NGC1052-DF2 and NGC1052-DF4: Independent Evidence for a Lack of Dark Matter
  • (abs, pdf) Husain et al., Detectability of Population III stellar remnants as X-ray binaries from tidal captures in the local Universe