2024-W08-2

Accretion disk

2402.10969

  • Reevaluating LSST's Capability for Time Delay Measurements in Quasar Accretion Discs

AGN

2402.11188

  • AGN properties of ~1 million member galaxies of galaxy groups and clusters at z < 1.4 based on the Subaru Hyper Suprime-Cam survey

2402.11665

  • Fast Outflows and Luminous He II Emission in Dwarf Galaxies with AGN

2402.11817

  • EMU/GAMA: A Technique for Detecting Active Galactic Nuclei in Low Mass Systems

2402.12054

  • The transient event in NGC 1566 from 2017 to 2019. I. An eccentric accretion disk and a turbulent, disk-dominated broad-line region unveiled by double-peaked Ca II and O I lines

2402.12063

  • To test R_{NLRs}~-~L_{O3} relation for narrow emission line regions of AGN through low redshift Type-2 AGN in SDSS

BH

2402.11018

  • Merger-Driven Growth of Intermediate-mass Black Holes: Constraints from Hubble Space Telescope Imaging of Hyper-luminous X-Ray Sources

2402.11019

  • Could long-period transients be powered by primordial black hole capture?

2402.11033

  • The Primordial Black Hole Abundance: The Broader, the Better

2402.12325

  • What Is the Black Hole Spin in Cyg X-1?

Cosmos

2402.11220

  • Peering into cosmic reionization: the Lyα visibility evolution from galaxies at z = 4.5-8.5 with JWST

2402.11688

  • Evidence for Episodic Black Hole Growth of Reionization-Era Quasars observed with Magellan/FIRE

2402.12016

  • A Distinct Radial Acceleration Relation across Brightest Cluster Galaxies and Galaxy Clusters

Galaxy

2402.12367

  • The first all-sky survey of star-forming galaxies with eROSITA: Scaling relations and a population of X-ray luminous starbursts

Review

2402.10996

  • A review of 70 years with astrometry
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