86 citations · 608 across the 30 of their papers we have counts for
9 papers · 1 filter
Virgo Filaments IV: Using WISE to Measure the Modification of Star-Forming Disks in the Extended Regions Around the Virgo Cluster
Kim Conger, Gregory Rudnick, Rose A. Finn +14
Recent theoretical work and targeted observational studies suggest that filaments are sites of galaxy preprocessing. The aim of the WISESize project is to directly probe galaxies o…
An Indication of Gas Inflow in Clumpy Star-Forming Galaxies near : Lower Gas-Phase Metallicities in Clumpy Galaxies Compared to Non-Clumpy Galaxies
Visal Sok, Adam Muzzin, Pascale Jablonka +5
Despite the ubiquity of clumpy star-forming galaxies at high-redshift, the origin of clumps are still largely unconstrained due to the limited observations that can validate the me…
Virgo Filaments. III. The gas content of galaxies in filaments as predicted by the GAEA semi-analytic model
D. Zakharova, B. Vulcani, G. De Lucia +8
Galaxy evolution depends on the environment in which galaxies are located. The various physical processes (ram-pressure stripping, tidal interactions, etc.) that can affect the gas…
Ground-based image deconvolution with Swin Transformer UNet
Utsav Akhaury, Pascale Jablonka, Jean-Luc Starck +1
As ground-based all-sky astronomical surveys will gather millions of images in the coming years, a critical requirement emerges for the development of fast deconvolution algorithms…
Euclid: Early Release Observations -- Dwarf galaxies in the Perseus galaxy cluster
F. R. Marleau, J. -C. Cuillandre, M. Cantiello +193
We make use of the unprecedented depth, spatial resolution, and field of view of the Euclid Early Release Observations of the Perseus galaxy cluster to detect and characterise the…
Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions
J. -C. Cuillandre, M. Bolzonella, A. Boselli +199
The Euclid ERO programme targeted the Perseus cluster of galaxies, gathering deep data in the central region of the cluster over 0.7 square degree, corresponding to approximately 0…