BH
2410.05857
- A new approach to constraining properties of AGN host galaxies by combining image and SED decomposition: testing upon the
relation
2410.06141
- Halo Mergers Enhance the Growth of Massive Black Hole Seeds
AGN
2410.05383
- The Effects of AGN Feedback on the Lyman-
Forest Flux Power Spectrum
2410.06297
- Determining star formation rates in AGN hosts from strong optical emission lines
2410.06960
- Blowing star formation away in AGN Hosts (BAH) -- II. Investigating the origin of the H2 emission excess in nearby galaxies with JWST MIRI
2410.06730
- Systematic collapse of the accretion disc in AGN confirmed by UV photometry and broad line spectra
2410.06853
- Microlensing analysis of 14.5-year light curves in SDSS J1004+4112: Quasar accretion disk size and intracluster stellar mass fraction
2410.06653
- Microquasars to AGNs: An uniform Jet variability
CGM
2410.05392
- A MUSE Source-Blind Survey for Emission from the Circumgalactic Medium
Galaxy
2410.06836
- The warm-hot intergalactic medium (WHIM) in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
2410.06988
- Cosmic Ray-Driven Galactic Winds with Resolved ISM and Ion-Neutral Damping
2410.05397
- Polycyclic Aromatic Hydrocarbon and CO(2-1) Emission at 50-150 pc Scales in 66 Nearby Galaxies
2410.06256
- SDSS IV MaNGA: The impact of the acquisition of gas with opposite angular momentum on the evolution of galaxies
2410.06736
- Photometric Analysis for Predicting Star Formation Rates in Large Galaxies Using Machine Learning and Deep Learning Techniques
2410.06510
- An X-ray Shell Reveals the Supernova Explosion for Galactic Microquasar SS 433
high-z
2410.05867
- Self-Similar Buildup and Inside-Out Growth: Tracing the Evolution of Intermediate to High-Mass Star-Forming Galaxies Since
2410.06505
- Neural network emulator to constrain the high-
IGM thermal state from Lyman-
2410.05891
- Supermassive primordial black holes for the GHZ9 and UHZ1 observed by the JWST
2410.05372
- Cosmic Reionization On Computers: Biases and Uncertainties in the Measured Mean Free Path at the End Stage of Reionization
