Zre良

UV 2411.14532[https://arxiv.org/abs/2411.14532] Hitting the slopes: A spectroscopic vie...

Zre良

2411.08485[https://arxiv.org/abs/2411.08485] The circumgalactic medium traced by Mg II ...

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TDE 2410.19047[https://arxiv.org/abs/2410.19047] Ultra-High-Energy Cosmic Rays from Neu...

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CGM 2410.17252[https://arxiv.org/abs/2410.17252] Cosmic Ray Mediated Thermal Fronts in ...

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AGN 2410.16018[https://arxiv.org/abs/2410.16018] Size and kinematics of the low-ionizat...

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AGN 2410.14291[https://arxiv.org/abs/2410.14291] First results from the JWST Early Rele...

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BH 2410.13406[https://arxiv.org/abs/2410.13406] Distinguishability of a naked singulari...

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Galaxy 2410.12911[https://arxiv.org/abs/2410.12911] Resonant Capture of Stars by Black ...

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CGM 2410.10993[https://arxiv.org/abs/2410.10993] Direct High-resolution Observation of ...

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TDE 2410.09720[https://arxiv.org/abs/2410.09720] Recurring tidal disruption events a de...

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Artifical Neural Networks 2410.08369[https://arxiv.org/abs/2410.08369] Estimating Cosmo...

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BH 2410.07342[https://arxiv.org/abs/2410.07342] An Intermediate Mass Black Hole Hidden ...

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BH 2410.05857[https://arxiv.org/abs/2410.05857] A new approach to constraining properti...

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AGN 2408.15934[https://arxiv.org/abs/2408.15934] Windy or not: Radio pc-scale evidence ...

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AGN 2408.15229[https://arxiv.org/abs/2408.15229] Why are optical coronal lines faint in...

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AGN 2408.13841[https://arxiv.org/abs/2408.13841] Bipolar blobs as evidence of hidden AG...

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AGN 2408.12770[https://arxiv.org/abs/2408.12770] An automated method for finding the mo...

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BH 2408.12017[https://arxiv.org/abs/2408.12017] Radiation Hydrodynamic Simulations of M...

Zre良

BH 2408.11098[https://arxiv.org/abs/2408.11098] Supermassive black holes from inflation...