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wiki:arxiv [2022/05/19 13:54]
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 ====
 +
 +  * 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]]
 +  * 
 +
 +==== 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 ====
 +
 +  * [[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/​2205.15325|FIREbox:​ Simulating galaxies at high dynamic range in a cosmological volume]]
  
 ==== May ==== ==== May ====
  
 +  * [[https://​arxiv.org/​abs/​2205.14858|Molecular Gas Structures traced by 13CO Emission in the 18,190 12CO Molecular Clouds from the MWISP Survey]]
 +  * [[https://​arxiv.org/​abs/​2205.12169|Investigating the Dominant Environmental Quenching Process in UVCANDELS/​COSMOS Groups]]
 +  * [[https://​arxiv.org/​abs/​2205.14899|Close Major Merger Pairs at z=0: Bulge-to-Total Ratio and Star Formation Enhancement]] another paper by Cong Xu on S+S and S+E pairs
 +  * [[https://​arxiv.org/​abs/​2205.14417|The driving mode of shock-driven turbulence]]
 +  * [[https://​arxiv.org/​abs/​2205.14378|Possible Systematic Rotation in the Mature Stellar Population of a z=9.1 Galaxy]]
 +  * [[https://​arxiv.org/​abs/​2205.09087|Three-dimensional extinction maps: Inverting inter-calibrated extinction catalogues]]
 +  * [[https://​arxiv.org/​abs/​2205.09069|Influence of Magnetic Fields on the Gas Rotation in the Galaxy NGC6946]]
 +    * magnetic field causes an ascending rotation curve in the outer radii of the galaxy, by ~7-14 km/s
 +    * so magnetic field is not that important
 +  * [[https://​arxiv.org/​abs/​2205.08799|A sparse regression approach for populating dark matter halos and subhalos with galaxies]] (the Durrum team)
 +    * interesting to compare with Yangyao'​s model
 +  * [[https://​arxiv.org/​abs/​2205.08554|Resolving the HI in Damped Lyman-α systems that power star-formation]] (Nature)
 +  * [[https://​arxiv.org/​abs/​2205.08552|A trail of dark matter-free galaxies from a bullet dwarf collision]] (Pieter van Dokkum, Nature)
 +  * [[https://​arxiv.org/​abs/​2205.08543|CLEAR:​ The Evolution of Spatially Resolved Star Formation in Galaxies between 0.5≲z≲1.7 using Hα Emission Line Maps]]
 +    * Ha surface density relative to continuum surface density within 1kpc drops from z~1 to z~0.5. The authors attribute this to inside-out quenching in the wake of inside-out growth. Since galaxy size grows, the lower value at lower redshift could be a result of gradient but not evolution. The 1kpc radius covers out to the disc at z~1 but it is only the central region at lower redshift. Need to check the size-mass relation at different redshifts.
   * [[https://​arxiv.org/​abs/​2205.08424|Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses]]   * [[https://​arxiv.org/​abs/​2205.08424|Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses]]
   * [[https://​arxiv.org/​abs/​2205.08241|How well do local relations predict gas-phase metallicity gradients? Results from SDSS-IV MaNGA]]   * [[https://​arxiv.org/​abs/​2205.08241|How well do local relations predict gas-phase metallicity gradients? Results from SDSS-IV MaNGA]]
wiki/arxiv.1652968473.txt.gz · Last modified: 2022/05/19 13:54 by Cheng Li