activity
20162025
most citedAn Atlas of Color-selected Quiescent Galaxies at in Public Fields

204 citations · 533 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.GA202515 cited

Clumps as multiscale structures in cosmic noon galaxies

Boris S Kalita, Tomoko L Suzuki, Daichi Kashino +31

Star-forming clumps have been found to significantly influence the star formation of gas-rich galaxies. Using public data from JWST/NIRCam (COSMOS-Web) and ALMA (FMOS-COSMOS)…

astro-ph.GA20252 cited

A multi-wavelength investigation of spiral structures in galaxies with JWST

Boris S. Kalita, Si-Yue Yu, John D. Silverman +18

Recent JWST observations have revealed the prevalence of spiral structures at . Unlike in the local Universe, the origin and the consequence of spirals at this epoch remain…

astro-ph.GA20245 cited

Behind the dust veil: A panchromatic view of an optically dark galaxy at z=4.82

Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis +30

Optically dark dusty star-forming galaxies (DSFGs) play an essential role in massive galaxy formation at early cosmic time, however their nature remains elusive. Here we present a…

astro-ph.GA20242 cited

SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web

Jed McKinney, Caitlin M. Casey, Arianna S. Long +36

JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In…

astro-ph.GA202432 cited

The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas

F. Rizzo, C. Bacchini, M. Kohandel +8

The gas in the interstellar medium (ISM) of galaxies is supersonically turbulent. Measurements of turbulence typically rely on cold gas emission lines for low-z galaxies and warm i…

astro-ph.GA20243 cited

A massive, neutral gas reservoir permeating a galaxy proto-cluster after the reionization era

Kasper E. Heintz, Jake S. Bennett, Pascal A. Oesch +21

Galaxy clusters are the most massive, gravitationally-bound structures in the Universe, emerging through hierarchical structure formation of large-scale dark matter and baryon over…