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Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 ≤ z ≤ 2.5 in 3D-HST/CANDELS
Shuang Liu, Yizhou Gu, Qirong Yuan, Shiying Lu, Min Bao, Guanwen Fang and Lulu Fan The Astrophysical Journal 923(1) 46 (2021) https://doi.org/10.3847/1538-4357/ac2817
Feedback from Active Galactic Nuclei in Galaxy Groups
Dominique Eckert, Massimo Gaspari, Fabio Gastaldello, Amandine M. C. Le Brun and Ewan O’Sullivan Universe 7(5) 142 (2021) https://doi.org/10.3390/universe7050142
The infrared-radio correlation of star-forming galaxies is stronglyM⋆-dependent but nearly redshift-invariant sincez∼ 4
Observable gravitational waves from tidal disruption events and their electromagnetic counterpart
Hugo Pfister, Martina Toscani, Thomas Hong Tsun Wong, et al. Monthly Notices of the Royal Astronomical Society 510(2) 2025 (2021) https://doi.org/10.1093/mnras/stab3387
Galaxy Stellar Mass Functions from z ∼ 10 to z ∼ 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of Galaxies in the First Gigayear of Cosmic Time
Mauro Stefanon, Rychard J. Bouwens, Ivo Labbé, Garth D. Illingworth, Valentino Gonzalez and Pascal A. Oesch The Astrophysical Journal 922(1) 29 (2021) https://doi.org/10.3847/1538-4357/ac1bb6
Kinematics and star formation of high-redshift hot dust-obscured quasars as seen by ALMA
The distribution and properties of DLAs at z ≤ 2 in the EAGLE simulations
Lilian Garratt-Smithson, Chris Power, Claudia del P Lagos, et al. Monthly Notices of the Royal Astronomical Society 501(3) 4396 (2021) https://doi.org/10.1093/mnras/staa3870