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- A Steep-Extinction Quasi-stellar Object at z=4.6: JWST Evidence for Abundant Small Dust Grains
- Episodic super-Eddington accretion as a clue to overmassive black holes in the early Universe
- FASHI DR2: A Catalog of 132 Low-Redshift HI 21 cm Absorption Systems
- Extended components of little red dots in the rest-frame optical
- Cosmic evolution of the [C II]-to-dense neutral gas relation
- MIAO-ALMA: Shocks and Protostellar Outflows in 70 μm-dark clumps with L/M < 1 L⊙/M⊙
- Little red dots host black hole stars: a unified family of gas-reddened AGN revealed by JWST /NIRSpec spectroscopy
- A first GLIMPSE into star-cluster populations across cosmic time
- Changing-look Active Galactic Nuclei from SDSS, LAMOST and DESI Surveys
- A Cross-Band (X-ray × Optical) Periodicity Search for Supermassive Black Hole Binaries: A Null Result and the First Completeness-Corrected Constraint
- Ejecta clumps revealed by study of reverse-shocked ejecta through MUSE integral field spectroscopy of SNR 0509-67.5
- XP-TEAL: Gaia XP Tool for Emission and Absorption Lines II. Gaia-HELIX catalogue of Hα emitters in Gaia BP/RP spectra
- A novel data-driven approach to extract stellar population properties from galaxy spectra using absorption indices
- Exact black hole solutions with semi-symmetric vectorial torsion
- Theoretical emission lines and metallicity calibrations of H II regions in ASTRID simulation
- Ghostly DLAs in SDSS DR16
- Improved constraints on the Milky Way potential using the M68 stream and DESI spectroscopic data
- Observing Co-Located Neutral and Ionized Gas-Phase Iron Depletion in the Magellanic Clouds
- Trace the Self-Gravitating Gas Using CO Isotopologues
- Testing Covarying Coupling Constants (CCC) against the full SPARC rotation-curve sample: a like-for-like comparison with MOND and NFW
- The Delay Time Distribution of Quasi-Periodic Eruptions
- Evidence for the First Globular Cluster Stellar Stream beyond the Milky Way
- A gas-enshrouded and gas-reddened black hole at cosmic dawn
- The little blue and red dot Rosetta stones
- Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots