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JWST/NIRCam Narrowband Survey of Paβ Emitters in the Spiderweb Protocluster at z = 2.16

We report the initial result of our Pa β narrowband imaging on a protocluster with the JWST Near Infrared Camera (NIRCam). As NIRCam enables deep narrowband imaging of rest-frame near-infrared lines at z > 1, we target one of the most studied protoclusters, the Spiderweb protocluster at z = 2.16, in...

Deskribapen osoa

Gorde:
Egile Nagusiak: Rhythm Shimakawa, J. M. Pérez-Martínez, Helmut Dannerbauer, Yusei Koyama, Tadayuki Kodama, Pablo G. Pérez-González, Chiara D’Eugenio, Yuheng Zhang, Abdurrahman Naufal, Kazuki Daikuhara
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: IOP Publishing 2024-01-01
Saila:The Astrophysical Journal
Gaiak:
Protoclusters
High-redshift galaxy clusters
Emission line galaxies
Near infrared astronomy
Galaxy formation
Galaxy evolution
Sarrera elektronikoa:https://doi.org/10.3847/1538-4357/ad8155
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