Revealing the Quiescent Galaxy Population in the Spiderweb Protocluster at z = 2.16 with Deep HST/WFC3 Slitless Spectroscopy

Revealing the Quiescent Galaxy Population in the Spiderweb Protocluster at z = 2.16 with Deep HST/WFC3 Slitless Spectroscopy

We report the Hubble Space Telescope Wide Field Camera 3 G141 grism slitless spectroscopy observation of the core region of the Spiderweb protocluster at z = 2.16. We analyzed the spectra of all objects in a $\sim 2\times 2\,{\mathrm{arcmin}}^{2}$ field of view and identified 40 protocluster members...

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Bibliographic Details
Main Authors: Abdurrahman Naufal, Yusei Koyama, Chiara D’Eugenio, Helmut Dannerbauer, Rhythm Shimakawa, Jose Manuel Pérez-Martínez, Tadayuki Kodama, Yuheng Zhang, Kazuki Daikuhara
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Protoclusters
Quenched galaxies
High-redshift galaxy clusters
Galaxy evolution
Online Access:https://doi.org/10.3847/1538-4357/ad8dcf
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https://doi.org/10.3847/1538-4357/ad8dcf

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