August 19, 2024

Lead: Annika Peter

Breaking the cosmological invariance of the dark matter halos shape as a new probe of modified gravity theory
Dark matter cooling during early matter-domination boosts sub-earth halos
On the Origin of Star Formation Quenching of Galaxies in Group Environments using the NewHorizon simulation
DIISC-IV: DIISCovery of Anomalously Low Metallicity H II Regions in NGC 99: Indirect Evidence of Gas Inflows
From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
Constraining SN Ia Progenitors from the Observed Fe-peak Elemental Abundances in the Milky Way Dwarf Galaxy Satellites
Study of the motion of Globular Clusters relative to the plane and center of the Galaxy based on Gaia and HST data
Denser Environments Cultivate Larger Galaxies: A Comprehensive Study Beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies
Globular cluster counts around 700 nearby galaxies
Systematically Measuring Ultra-Diffuse Galaxies. VII. The HI Survey Overview
The Anisotropic Circumgalactic Medium of Sub-L∗ Galaxies
Quantifying Bursty Star Formation in Dwarf Galaxies
Segue 2 Recently Collided with the Cetus-Palca Stream: New Opportunities to Constrain Dark Matter in an Ultra-Faint Dwarf
Euclid: The Early Release Observations Lens Search Experiment
Free Streaming in Warm Wave Dark Matter
Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
Probing the nature of dark matter using strongly lensed gravitational waves from binary black holes
Gas-rich "ultra-diffuse" galaxies are consistent with the baryonic Tully-Fisher relation and with Milgromian dynamics
Large dark matter content and steep metallicity profile predicted for Ultra-Diffuse Galaxies formed in high-spin halos
Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with Star Formation Histories

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