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20112026
most citedFast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8

170 citations · 1.4k across the 56 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.GA2023

Structure and Color Gradients of Ultra-diffuse Galaxies in Distant Massive Galaxy Clusters

Pinsong Zhao, Fengshan Liu, Qifan Cui +2

We have measured structural parameters and radial color profiles of 108 ultra-diffuse galaxies (UDGs), carefully selected from six distant massive galaxy clusters in the Hubble Fro…

astro-ph.GA2023

Galaxy mergers in Subaru HSC-SSP: a deep representation learning approach for identification and the role of environment on merger incidence

Kiyoaki Christopher Omori, Connor Bottrell, Mike Walmsley +7

We take a deep learning-based approach for galaxy merger identification in Subaru HSC-SSP, specifically through the use of deep representation learning and fine-tuning, with the ai…

astro-ph.GA2023★ 55 cited

IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation

Connor Bottrell, Hassen M. Yesuf, Gergö Popping +13

At fixed galaxy stellar mass, there is a clear observational connection between structural asymmetry and offset from the star forming main sequence, SFMS. Herein, we use the TNG…

astro-ph.GA2023

HINOTORI I: The Nature of Rejuvenation Galaxies

Takumi S. Tanaka, Kazuhiro Shimasaku, Sandro Tacchella +4

We present the HINOTORI (star formation History INvestigatiOn TO find RejuvenatIon) project to reveal the nature of rejuvenation galaxies (RGs), which are galaxies that restarted t…

astro-ph.GA2023

Nobeyama 45-m CO J=1-0 Observations of Luminous Type 1 AGNs at

Tomonari Michiyama, Ming-Yang Zhuang, Jinyi Shangguan +3

We have performed CO J =1-0 observations of ten galaxies hosting luminous () type 1 active galactic nuclei (AGNs) with the Nobeyama 45-m r…

astro-ph.GA2023

Morphological asymmetries of quasar host galaxies with Subaru Hyper Suprime-Cam

Shenli Tang, John D. Silverman, Hassen M. Yesuf +7

How does the host galaxy morphology influence a central quasar or vice versa? We address this question by measuring the asymmetries of 2424 SDSS quasar hosts at using b…