wiki:arxiv
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wiki:arxiv [2022/06/02 02:41] Cheng Li |
wiki:arxiv [2023/12/04 22:19] (current) Cheng Li |
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| ====== My arXiv notes (since 2020) ====== | ====== My arXiv notes (since 2020) ====== | ||
| - | ==== Userful tools/ref ==== | + | ==== Userful tools ==== |
| * RealSim-IFS: [[https://arxiv.org/abs/2205.15335|Realistic synthetic integral field spectroscopy with RealSim-IFS]] | * RealSim-IFS: [[https://arxiv.org/abs/2205.15335|Realistic synthetic integral field spectroscopy with RealSim-IFS]] | ||
| * The RealSim-IFS Python code is publicly available here: https://github.com/cbottrell/realsim_ifs. | * The RealSim-IFS Python code is publicly available here: https://github.com/cbottrell/realsim_ifs. | ||
| * how to referee papers? [[https://arxiv.org/abs/2205.14270|A Referee Primer for Early Career Astronomers]] | * how to referee papers? [[https://arxiv.org/abs/2205.14270|A Referee Primer for Early Career Astronomers]] | ||
| + | * | ||
| + | |||
| + | ==== Review articles ==== | ||
| + | |||
| + | * [[https://arxiv.org/abs/2206.01548|Dust Formation in Astrophysical Environments: The Importance of Kinetics]] | ||
| + | * [[https://arxiv.org/abs/2206.03510|ALPINE: A Large Survey to Understand Teenage Galaxies]] | ||
| + | |||
| + | ===== 2023 ===== | ||
| + | |||
| ===== 2022 ===== | ===== 2022 ===== | ||
| + | |||
| + | ==== July ==== | ||
| + | |||
| + | * [[https://arxiv.org/abs/2207.05093|Turbulent Cold Flows Gave Birth to the First Quasars]] | ||
| ==== June ==== | ==== June ==== | ||
| + | * [[https://arxiv.org/abs/2206.04521|The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers]] | ||
| + | * [[https://arxiv.org/abs/2206.04522|The stellar halo in Local Group Hestia simulations II. The accreted component]] | ||
| + | * [[https://arxiv.org/abs/2206.00681|Pressure-Regulated, Feedback-Modulated Star Formation In Disk Galaxies]] | ||
| + | * [[https://arxiv.org/abs/2206.00662|The Size-Mass Relation of Post-Starburst Galaxies in the Local Universe]]: post-starburst galaxies in SDSS are found to be smaller than quiescent galaxies of same masses. I'm wondering whether the same effect is seen also in the MaNGA-based sample. | ||
| + | * [[https://arxiv.org/abs/2206.00138|PASSAGES: The Large Millimeter Telescope and ALMA Observations of Extremely Luminous High Redshift Galaxies Identified by the Planck]] | ||
| * [[https://arxiv.org/abs/2206.00098|AGN Feedback in Groups and Clusters of Galaxies]] a review chapter | * [[https://arxiv.org/abs/2206.00098|AGN Feedback in Groups and Clusters of Galaxies]] a review chapter | ||
| * [[https://arxiv.org/abs/2205.15672|Intrinsic shapes of Brightest Cluster Galaxies]] | * [[https://arxiv.org/abs/2205.15672|Intrinsic shapes of Brightest Cluster Galaxies]] | ||
wiki/arxiv.1654137692.txt.gz · Last modified: 2022/06/02 02:41 by Cheng Li
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