wiki:arxiv
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wiki:arxiv [2022/06/01 13:52] 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]] | ||
| + | * 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/2205.15672|Intrinsic shapes of Brightest Cluster Galaxies]] | ||
| + | * We show that these objects are strongly triaxial, with triaxiality parameters 0.39 ≤T≤ 0.72, have on average axis ratios <p(r)>= 0.84 and <q(r)>= 0.68, and are more spherical in the central regions but flatten out at large radii. | ||
| + | * Measured shapes in the outskirts agree well with the shapes found for simulated massive galaxies and their dark matter halos from both the IllustrisTNG and the Magneticum simulations, possibly probing the nature of dark matter. In contrast, both simulations fail to reproduce the observed inner regions of BCGs, producing too flattened objects. | ||
| + | * [[https://arxiv.org/abs/2205.15388|The UV luminosity functions of Bright z>8 Galaxies: Determination from ~0.41 deg2 of HST Observations along ~300 independent sightlines]] | ||
| * [[https://arxiv.org/abs/2205.15328|Impact of the cosmic background radiation on the initial mass function of metal-poor stars]] | * [[https://arxiv.org/abs/2205.15328|Impact of the cosmic background radiation on the initial mass function of metal-poor stars]] | ||
| * [[https://arxiv.org/abs/2205.15325|FIREbox: Simulating galaxies at high dynamic range in a cosmological volume]] | * [[https://arxiv.org/abs/2205.15325|FIREbox: Simulating galaxies at high dynamic range in a cosmological volume]] | ||
wiki/arxiv.1654091574.txt.gz · Last modified: 2022/06/01 13:52 by Cheng Li
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