11 citations · 11 across the 3 of their papers we have counts for
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Rapid quenching and early gas depletion in the core of a galaxy protocluster at z=2.2
C. D'Eugenio, H. Dannerbauer, A. Naufal +6
Understanding how galaxy evolution is affected in forming high-z overdensities is a major open question in modern astrophysics. Here, we present the average properties of the quies…
Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster
J. Nadolny, J. M. Pérez-Martínez, H. Dannerbauer +8
We investigate how the environment affects galaxy structure in the Spiderweb protocluster at using JWST/NIRCam F115W, F182M, and F410M imaging (rest-frame Å to…
JWST/NIRCam Pa narrow-band imaging reveals ordinary dust extinction for H emitters within the Spiderweb protocluster at z=2.16
Jose Manuel Pérez-Martínez, Helmut Dannerbauer, Yusei Koyama +7
We combine JWST/NIRCam and Subaru/MOIRCS dual Pa + H narrow-band imaging to trace the dust attenuation and the star-formation activities of a sample of 43 H$\ma…
Revealing the quiescent galaxy population in the Spiderweb protocluster at z=2.16 with deep HST/WFC3 slitless spectroscopy
Abdurrahman Naufal, Yusei Koyama, Chiara D'Eugenio +6
We report the HST WFC3 G141 grism slitless spectroscopy observation of the core region of the Spiderweb protocluster at . We analyzed the spectra of all objects in a $\sim…