11 papers
A GLIMPSE of the 99%: a census of the faintest galaxies during the epoch of reionization and its implications for galaxy formation models
Hakim Atek, Iryna Chemerynska, Lukas J. Furtak +19
We present a comprehensive study of the galaxy UV luminosity function (UVLF) at leveraging deep JWST observations from the GLIMPSE survey. Thanks to gravitational lensing,…
The SPHINX public data release. II. Using low-ionisation absorption lines and dust attenuation to predict Lyman continuum escape
Valentin Mauerhofer, Jérémy Blaizot, Thibault Garel +11
Low-ionisation state (LIS) absorption lines, such as SiII 1526, are widely used to trace the properties of the interstellar medium (ISM) in galaxies. These lines provide crucial in…
ARCHITECTS II: Impact of subgrid physics on the observable properties of the circumgalactic medium
Maxime Rey, Jérémy Blaizot, Taysun Kimm +3
Galaxy evolution is driven by star formation and stellar feedback on scales unresolved by current high-resolution cosmological simulations, requiring robust subgrid models. However…
ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
Maxime Rey, Jérémy Blaizot, Taysun Kimm +2
Galaxy evolution is shaped by star formation and stellar feedback at scales unresolved by current high-resolution cosmological simulations. Precise subgrid models are thus necessar…
Radiation hydrodynamic simulation of the Haro 11 galaxy: the escape of LyC and Ly in a dwarf galaxy merger
Timmy Ejdetjärn, Göran Ãstlin, Joakim Rosdahl +2
The Haro 11 galaxy merger is the closest known Lyman Continuum (LyC) leaker and a strong Lyman- (Ly) emitter, making it an important analogue of the high- galaxies that…
The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
Claudia Di Cesare, Jorryt Matthee, Rohan P. Naidu +17
Galaxies exhibit a tight correlation between their star-formation rate and stellar mass over a wide redshift range known as the star-forming main sequence (SFMS). With JWST, we can…