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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…
Feeding and feedback processes in the Spiderweb proto-intracluster medium
M. Lepore, L. Di Mascolo, P. Tozzi +15
We present the detailed analysis of the thermal, diffuse emission of the proto-intracluster medium (ICM) detected in the halo of the Spiderweb Galaxy at z=2.16, within a radius of…
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-MartÃnez, 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 re…
Spider-Webb: JWST Near Infrared Camera resolved galaxy star formation and nuclear activities in the Spiderweb protocluster at z=2.16
Rhythm Shimakawa, Yusei Koyama, Tadayuki Kodama +8
Near-infrared (NIR) emission is less affected by dust than UV and optical emission and is therefore useful for studying the properties of dust-obscured galaxies. Although rest-fram…
ASWDF: Census of the obscured star formation in a galaxy cluster in formation at
Y. H. Zhang, H. Dannerbauer, J. M. Pérez-MartÃnez +13
We report the results of the deep and wide Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm mapping of the Spiderweb protocluster at . The observations were divid…
MeerKAT Observations of Herschel Protocluster Candidates
Y. Ding, D. L. Clements, L. L. Leeuw +9
High-redshift protoclusters consisting of dusty starbursts are thought to play an important role in galaxy evolution. Their dusty nature makes them bright in the FIR/submm but diff…