Accès ouvert
2026
article
OpenAlex
M. V. Legnardi, F. Muratore, A. P. Milone, G. Cordoni et autres
Nearby galaxies such as the Large Magellanic Cloud (LMC) offer an ideal laboratory to test the initial mass function under different physical conditions, but previous works have been limited by photometric depth and have therefore poorly constrained the low-mass regime. Here, we …
it, au, ae, us, kr, cn
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Accès ouvert
2026
article
OpenAlex
Matteo Messa, Anita Zanella, A. Bolamperti, M Castellano et autres
We report the discovery of a faint (M 1700 ≃ −12.2), oxygen-deficient, strongly lensed ionizing source – dubbed Lensed And Pristine 2 (LAP2) – at a spectroscopic redshift of z = 4.19. LAP2 appears to be isolated and lies very close to …
it, de, gb, se, us
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Accès ouvert
2025
article
OpenAlex
F. Calura, R. Pascale, Oscar Agertz, Eric P. Andersson et autres
Star clusters stand at the crossroads between galaxies and single stars. Resolving the formation of star clusters in cosmological simulations represents an ambitious and challenging goal, since modelling their internal properties requires very high resolution. This paper is the third of a …
Accès ouvert
2025
article
OpenAlex
A. Bolamperti, S.J. Chang, Jean-Louis Vernet, A. Zanella et autres
Lyman-α (Lyα) emission is the intrinsically strongest tracer of recombining ionized hydrogen in young star-forming galaxies, but its origin is still debated. Lyα arises when emitted photons scatter in neutral hydrogen, with each scattering event changing their propagation direction and frequency. So …
de, it, nl
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Accès ouvert
2025
preprint
OpenAlex
A. Bolamperti, S.J. Chang, Jean-Louis Vernet, A. Zanella et autres
Ly$α$ emission is the strongest tracer of recombining ionized hydrogen in young, star-forming galaxies, but its origin is still debated. Ly$α$ arises when emitted photons scatter in neutral hydrogen and, so far, observational efforts have mostly focused on the Ly$α$ surface brightness …
Accès ouvert
2024
preprint
OpenAlex
F. Calura, R. Pascale, Oscar Agertz, Eric P. Andersson et autres
Star clusters stand at the crossroads between galaxies and single stars. Resolving the formation of star clusters in cosmological simulations represents an ambitious and challenging goal, since modelling their internal properties requires very high resolution. This paper is the third of a …
it, se, us, fr
(code pays fourni par la source)
Accès ouvert
2024
article
OpenAlex
Eros Vanzella, F. Loiacono, Matteo Messa, M Castellano et autres
We report the serendipitous discovery of a faint (M UV > −12.2), low-metallicity (Z ∼ 0.02 Z⊙) ionizing source, dubbed T2c, with a spectroscopic redshift of z = 6.146. T2c is part of a larger structure amplified by the Hubble Frontier Field …
Accès ouvert
2024
preprint
OpenAlex
E. Vanzella, F. Loiacono, Matteo Messa, M Castellano et autres
We report the serendipitous discovery of a faint (M_UV > -12.2), low-metallicity (Z ~ 0.02 Zsun), ionizing source (dubbed T2c) with a spectroscopic redshift of z=6.146. T2c is part of a larger structure amplified by the Hubble Frontier Field galaxy cluster MACSJ0416, …
Accès ouvert
2024
preprint
OpenAlex
Y. Mellier, J.A. Acevedo Barroso, A. Achúcarro, Jiřı́ Adámek et autres
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015-2025 programme of the European Space Agency …
fr, us, ch, nl, es, it, gb, pt, de, be, ca, au
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Accès ouvert
2022
article
OpenAlex
S. E. van Mierlo, K. I. Caputi, M. Ashby, Hakim Atek et autres
A&A, 666, A200 (2022), https://doi.org/10.1051/0004-6361/202243950
nl, us, fr, it, gb, dk, es, pt, ch, de, ca, no, fi
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Accès ouvert
2022
preprint
OpenAlex
E. Vanzella, M. Castellano, P. Bergamini, Tommaso Treu et autres
We investigate the blue and optical rest-frame sizes (lambda~2300A-4000A) of three compact star-forming regions in a galaxy at z=4 strongly lensed (x30, x45, x100) by the Hubble Frontier Field galaxy cluster A2744 using GLASS-ERS JWST/NIRISS imaging at 1.15um, 1.50mu and 2.0mu with …