2024-W30-4

AGN

2407.17243

  • A second view on the X-ray polarization of NGC 4151 with IXPE

2407.17116

  • Discovery of a Damped Lyα Absorber in the Circumnuclear Zone of the FeLoBAL Quasar SDSS J083942.11+380526.3

2407.16971

  • Lyα imaging around the hyperluminous dust-obscured quasar W2246-0526 at z=4.6

BH

2407.16745

  • She's Got Her Mother's Hair: End-to-End Collapsar Simulations Unveil the Origin of Black Holes' Magnetic Field

CGM

2407.16784

  • A Sub-solar Fe/O, logT~7.5 Gas Component Permeating the Milky Way's CGM

Galaxy

2407.17410

  • Strong Balmer break objects at z ~ 7-10 uncovered with JWST

2407.17110

  • The Extreme Low-mass End of the Mass-Metallicity Relation at z\sim7

2407.17359

  • Simulated [CII] in high-z galaxies

2407.16755

  • The stellar distribution in ultra-faint dwarf galaxies suggests deviations from the collision-less cold dark matter paradigm

2407.16749

  • Analytic model for the statistics of ultra-high magnification events

Cosmology

2407.16744

-Evaluating Cosmological Biases using Photometric Redshifts for Type Ia Supernova Cosmology with the Dark Energy Survey Supernova Program

IM

2407.17288

  • What is your favorite transient event? SOXS is almost ready to observe!

2407.17288

  • What is your favorite transient event? SOXS is almost ready to observe!

2407.16759

  • X-ray speed reading with the MCRC: prototype success and next-generation upgrades

2407.16757

  • The XOC X-ray Beamline: Probing Colder, Quieter, and Softer

2407.16973

  • Simulation study of the performance of the Very Large Area gamma-ray Space Telescope

2407.16761

  • Continued developments in X-ray speed reading: fast, low noise readout for next-generation wide-field imagers
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