GCs of dwarf galaxies in Perseus cluster
T. Saifollahi, A. Lançon, Michele Cantiello, Jean‐Charles Cuillandre et autres
fr, it, es, gb, de, at, ca, fi, pt, us, in, ch, no, nl, dk (code pays fourni par la source)
Informations fournies par OpenAlex. Research Africa ne déduit ni nationalité, ni poste, ni coordonnées personnelles.
T. Saifollahi, A. Lançon, Michele Cantiello, Jean‐Charles Cuillandre et autres
fr, it, es, gb, de, at, ca, fi, pt, us, in, ch, no, nl, dk (code pays fourni par la source)
Francine R. Marleau, Cuillandre J.-C., Cantiello M., Carollo D. et autres
at, fr, it, ch, fi, nl, gb, de, ca, es, pt, in, no, us, dk (code pays fourni par la source)
Jean‐Charles Cuillandre, Bolzonella M., Boselli A., Marleau F.R. et autres
Mondelin M., S. Codis, J.-C. Cuillandre, C. Laigle et autres
The discovery of the large-scale structure of the Universe has fundamentally reshaped our understanding of galaxy formation and evolution. Filaments of the cosmic web act as privileged environments, guiding the growth of structures. Motivated by predictions from cosmological simulations, we investigate the …
Mondelin M., S. Codis, J.-C. Cuillandre, C. Laigle et autres
The discovery of the large-scale structure of the Universe has fundamentally reshaped our understanding of galaxy formation and evolution. Filaments of the cosmic web act as privileged environments, guiding the growth of structures. Motivated by predictions from cosmological simulations, we investigate the …
Mondelin M., S. Codis, J. -C. Cuillandre, R. Paviot et autres
Intrinsic alignments of galaxy shapes are a major systematic for weak gravitational lensing and provide insight into how galaxies acquire orientations within the cosmic web. Most studies rely on large statistical samples; here, we probe this signal in a single nearby superstructure, …
Mondelin M., S. Codis, J. -C. Cuillandre, R. Paviot et autres
Intrinsic alignments of galaxy shapes are a major systematic for weak gravitational lensing and provide insight into how galaxies acquire orientations within the cosmic web. Most studies rely on large statistical samples; here, we probe this signal in a single nearby superstructure, …
S. Martocchia, A. Boselli, J.-C. Cuillandre, Mondelin M. et autres
The Euclid Early Release Observations (ERO) programme targeted the Perseus galaxy cluster in its central region over 0.7 deg2. We combined the exceptional image quality and depth of the ERO-Perseus with FUV and NUV observations from GALEX and AstroSat/UVIT, as well as …
fr, it, gb, be, es, de, ca (code pays fourni par la source)
S. Martocchia, A. Boselli, J.-C. Cuillandre, Mondelin M. et autres
The Euclid Early Release Observations (ERO) programme targeted the Perseus galaxy cluster in its central region over 0.7 deg 2 . We combined the exceptional image quality and depth of the ERO-Perseus with FUV and NUV observations from GALEX and AstroSat/UVIT, as …
fr, it, gb, be, es, de, ca, nl, us, ch, no, dk, fi (code pays fourni par la source)
S. Martocchia, A. Boselli, J. -C. Cuillandre, Mondelin M. et autres
The Euclid Early Release Observations (ERO) programme targeted the Perseus galaxy cluster in its central region over 0.7deg$^2$. We combined the exceptional image quality and depth of the ERO-Perseus with FUV and NUV observations from GALEX and AstroSat/UVIT, as well as $ugrizHα$ …
Mondelin M., F. Bournaud, J.-C. Cuillandre, S. Codis et autres
The Perseus field captured by Euclid as part of its Early Release Observations provides a unique opportunity to study cluster environment ranging from outskirts to dense regions. Leveraging unprecedented optical and near-infrared depths, we investigate the stellar structure of massive disc galaxies …
Jean‐Charles Cuillandre, M. Bolzonella, A. Boselli, F.R Marleau et autres
The Euclid Early Release Observations (ERO) programme targeted the Perseus cluster of galaxies, gathering deep data in the central region of the cluster over 0.7 deg2, including the cluster core up to 0.25 r200. The dataset reaches a point-source depth of IE …
fr, it, at, de, ca, es, pt, gb, nl, ch, be, fi (code pays fourni par la source)
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