Maxime Tarrasse
A5073195612- Astronomy and Astrophysical Research
- Galaxies: Formation, Evolution, Phenomena
- Stellar, planetary, and galactic studies
- Particle physics theoretical and experimental studies
- Astrophysical Phenomena and Observations
- Adaptive optics and wavefront sensing
- Computational Physics and Python Applications
- Astrophysics and Cosmic Phenomena
Université Paris-Saclay
2023-2025
Université Paris Cité
2023-2025
Astrophysique, Instrumentation et Modélisation
2023-2025
Centre National de la Recherche Scientifique
2023-2025
CEA Paris-Saclay
2023-2025
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
2023-2025
In recent years, observations have uncovered a population of massive galaxies that are invisible or very faint in deep optical/near-infrared (near-IR) surveys but brighter at longer wavelengths. However, the nature these optically dark (OFGs; one several names given to objects) is highly uncertain. this work, we investigate drivers dust attenuation JWST era. particular, study role stellar mass, size, and orientation obscuring star-forming (SFGs) $3 < z 7.5$, focusing on question why OFGs...
The James Webb Space Telescope (JWST) is revolutionizing our understanding of the Universe by unveiling faint, near-infrared dropouts previously beyond reach, ranging from exceptionally dusty sources to galaxies up redshift $z \sim 14$. In this paper, we identify F200W-dropout objects in Cosmic Evolution Early Release Science (CEERS) survey which are absent existing catalogs. Our selection method can effectively obscured low-mass ($\log \text{M}_* \leq 9$) at 6$, massive dust-rich 12$, and...
Abstract We have not yet observed the epoch at which disc galaxies emerge in Universe. While high-z measurements of large-scale features such as bars and spiral arms trace evolution galaxies, methods cannot directly quantify featureless discs early Here we identify a substantial population apparently Cosmic Evolution Early Release Science (CEERS) survey by combining quantitative visual morphologies ∼7000 from Galaxy Zoo JWST CEERS project with public catalogue expert parametric morphologies....
The combined capabilities of the James Webb Space Telescope/Near Infrared Camera (NIRCam) and Hubble Telescope/Advanced for Surveys (ACS) instruments provide high-angular-resolution imaging from ultraviolet to near-infrared (UV/NIR), offering unprecedented insight into inner structure star-forming galaxies (SFGs) even when they are shrouded in dust. In particular, it is now possible spatially resolve study a population highly attenuated massive red SFGs (rm RedSFGs) at z∼4 rest-frame...
In recent years, observations have uncovered a population of massive galaxies that are invisible or very faint in deep optical/near-infrared (near-IR) surveys but brighter at longer wavelengths. However, the nature these optically dark (OFGs; one several names given to objects) is highly uncertain. this work, we investigate drivers dust attenuation JWST era. particular, study role stellar mass, size, and orientation obscuring star-forming (SFGs) $3 < z 7.5$, focusing on question why OFGs...
During the last decade, studies about highly attenuated and massive red star-forming galaxies (RedSFGs) at $z \sim 4$ have suggested that they could constitute a crucial population for unraveling mechanisms driving transition from vigorous star formation to quiescence high redshifts. Since such seems be linked morphological transformation, studying properties of these RedSFGs is essential our understanding galaxy evolution. To this end, we are using JWST/NIRCam images CEERS survey assemble...