246 citations · 6k across the 111 of their papers we have counts for
11 papers · 1 filter
Theoretical strong line metallicity diagnostics for the JWST era
Prerak Garg, Desika Narayanan, Ryan L. Sanders +5
The ratios of strong rest-frame optical emission lines are the dominant indicator of metallicities in high-redshift galaxies. Since typical strong-line based metallicity indicators…
: Modeling a Universe of Molecular Line Luminosities in Hydrodynamical Simulations
Karolina Garcia, Desika Narayanan, Gergö Popping +3
We present {\sc slick} (the Scalable Line Intensity Computation Kit), a software package that calculates realistic CO, [\ion{C}{1}], and [\ion{C}{2}] luminosities for clouds and ga…
Galaxy mergers in Subaru HSC-SSP: a deep representation learning approach for identification and the role of environment on merger incidence
Kiyoaki Christopher Omori, Connor Bottrell, Mike Walmsley +7
We take a deep learning-based approach for galaxy merger identification in Subaru HSC-SSP, specifically through the use of deep representation learning and fine-tuning, with the ai…
Faint [CI](1-0) emission in z 3.5 radio galaxies
S. Kolwa, C. De Breuck, J. Vernet +6
We present Atacama Large Millimeter/sub-millimeter Array (ALMA) neutral carbon, [C I](1-0), line observations that probe molecular hydrogen gas (H) within seven radio galaxies…
Emulating Radiative Transfer with Artificial Neural Networks
Snigdaa S. Sethuram, Rachel K. Cochrane, Christopher C. Hayward +4
Forward-modeling observables from galaxy simulations enables direct comparisons between theory and observations. To generate synthetic spectral energy distributions (SEDs) that inc…
IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
Connor Bottrell, Hassen M. Yesuf, Gergö Popping +13
At fixed galaxy stellar mass, there is a clear observational connection between structural asymmetry and offset from the star forming main sequence, SFMS. Herein, we use the TNG…
The IR Compactness of Dusty Galaxies Set Star-formation and Dust Properties at z~0-2
Jed McKinney, Alexandra Pope, Allison Kirkpatrick +9
Surface densities of gas, dust and stars provide a window into the physics of star-formation that, until the advent of high-resolution far-infrared/sub-millimeter observations, has…
ALMA High-Level Data Products: Submillimetre counterparts of SDSS quasars in the ALMA footprint
A. Wong, E. Hatziminaoglou, A. Borkar +5
The Atacama Large Millimetre/submillimetre Array (ALMA) is the world's most advanced radio interferometric facility, producing science data with an average rate of about 1 TB per d…
ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at
Seiji Fujimoto, Kotaro Kohno, Masami Ouchi +40
We present a statistical study of 180 dust continuum sources identified in 33 massive cluster fields by the ALMA Lensing Cluster Survey (ALCS) over a total of 133 arcmin area…
A NOEMA molecular line scan of the Hubble Deep Field North: Improved constraints on the CO luminosity functions and cosmic density of molecular gas
Leindert A. Boogaard, Roberto Decarli, Fabian Walter +9
We present measurements of the CO luminosity functions (LFs) and the evolution of the cosmic molecular gas density out to z~6 based on an 8.5 arcmin^2 spectral scan survey at 3mm o…
MusE GAs FLOw and Wind (MEGAFLOW) IX. The impact of gas flows on the relations between the mass, star formation rate and metallicity of galaxies
I. Langan, J. Zabl, N. F. Bouche +13
We study the link between gas flow events and key galaxy scaling relations: the relations between star formation rate (SFR) and stellar mass (the main sequence, MS), gas metallicit…