From the 1 of 11 linked papers with an AI index.
11 papers
Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster
J. Nadolny, J. M. Pérez-MartÃnez, H. Dannerbauer +8
The paper uses JWST/NIRCam imaging to study how galaxy sizes and structures in the Spiderweb protocluster at z=2.16 depend on environment, finding distinct mass‑size relations for…
Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa narrow-band imaging
Kazuki Daikuhara, Tadayuki Kodama, Yusei Koyama +10
Understanding the role of the environment in galaxy evolution is key to revealing the physical processes that regulate galaxy growth. We study the star formation activity of \pab\…
Spider-Webb: Spatially-Resolved Evidence of Inside-Out Quenching in the Spiderweb Protocluster at
Ronaldo Laishram, Yusei Koyama, Abdurrahman Naufal +6
We present a spatially-resolved analysis of galaxy quenching within the Spiderweb Protocluster at , combining deep imaging from the James Webb Space Telescope (JWST) a…
JWST reveals extended stellar disks for ALMA-bright dusty star-forming galaxies in the Spiderweb protocluster
Y. H. Zhang, H. Dannerbauer, J. M. Pérez-MartÃnez +14
We present JWST/NIRCam imaging of dusty star-forming galaxies (DSFGs) detected by Atacama Large Millimeter/submillimeter Array (ALMA) in the Spiderweb protocluster at . We…
The Stellar Morphology & Size of X-ray-selected Active Galactic Nuclei Host Galaxies Revealed by JWST
Bovornpratch Vijarnwannaluk, Zhen-Kai Gao, Wei-Hao Wang +19
We investigate the stellar shape and size-mass relationship of X-ray selected Active Galactic Nuclei (AGN) host galaxies using the high-angular resolution and deep sensitivity in t…
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…