activity
20222026
most citedSigns of environmental effects on star-forming galaxies in the Spiderweb protocluster at z=2.16

44 citations · 84 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026

Euclid: Quick Data Release (Q1) -- Exploring the detailed visual morphology of galaxies in clusters

P. Mas-Buitrago, S. Kruk, D. O'Ryan +167

Galaxy clusters provide unique laboratories for studying environmental effects on galaxy evolution. The morphology--density (--) and morphology--cluster-centric radius (--…

astro-ph.GA2024★ 10 cited

COALAS III: The ATCA CO(1-0) look at the growth and death of H emitters in the Spiderweb protocluster at z=2.16

J. M. Pérez-Martínez, H. Dannerbauer, B. H. C. Emonts +26

We obtain CO(1-0) molecular gas measurements with ATCA on a sample of 43 spectroscopically confirmed H emitters in the Spiderweb protocluster at and investigate the rel…

astro-ph.GA2023

Enhanced star formation and metallicity deficit in the USS 1558-003 forming protocluster at z=2.53

Jose Manuel Pérez-Martínez, Tadayuki Kodama, Yusei Koyama +6

We use K-band multi-object near-infrared spectroscopy with Keck/MOSFIRE to search for environmental imprints on the gas properties of 27 narrow-band selected H emitters (HAEs) a…

astro-ph.GA2023★ 1 cited

COALAS II. Extended molecular gas reservoirs are common in a distant, forming galaxy cluster

Zhengyi Chen, Helmut Dannerbauer, Matthew Lehnert +24

This paper presents the results of 475 hours of interferometric observations with the Australia Telescope Compact Array towards the Spiderweb protocluster at \(z=2.16\). We search…

astro-ph.GA2023

New insights into the role of AGNs in forming the cluster red sequence

Rhythm Shimakawa, José Manuel Pérez-Martínez, Yusei Koyama +7

As a considerable investment of time from various telescope facilities were dedicated toward studying the Spiderweb protocluster at , it so far remains one of the most exten…

astro-ph.GA2022★ 44 cited

Signs of environmental effects on star-forming galaxies in the Spiderweb protocluster at z=2.16

Jose Manuel Pérez-Martínez, Helmut Dannerbauer, Tadayuki Kodama +11

We use multi-object near-infrared (NIR) spectroscopy with VLT/KMOS to investigate the role of the environment in the evolution of the ionized gas properties of narrow-band selected…

astro-ph.GA2022★ 29 cited

Revealing impacts of stellar mass and environment on galaxy quenching

Zhiying Mao, Tadayuki Kodama, Jose Manuel Pérez-Martínez +3

Galaxy quenching is a critical step in galaxy evolution. In this work, we present a statistical study of galaxy quenching in 17 cluster candidates at 0.5<z<1.0 in the COSMOS field.…