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The quiescent population at $0.5\le z \le 0.9$: Environmental impact on the mass-size relation
Free accessArXiv | 2024| -
A comparative study of the fundamental metallicity relation
Free accessThe impact of methodology on its observed evolution⋆EDP Sciences | 2024| -
The ALPINE-ALMA [CII] Survey: Dust emission effective radius up to 3 kpc in the Early Universe
Free accessArXiv | 2024| -
Euclid preparation
Free accessXXXIX. The effect of baryons on the halo mass functionEDP Sciences | 2024| -
Euclid preparation
Free accessXXXVII. Galaxy colour selections with Euclid and ground photometry for cluster weak-lensing analysesEDP Sciences | 2024| -
Euclid preparation
Free accessXXXVIII. Spectroscopy of active galactic nuclei with NISP⋆EDP Sciences | 2024| -
Euclid preparation. Measuring detailed galaxy morphologies for Euclid with Machine Learning
Free accessArXiv | 2024| -
Influence of star-forming galaxy selection on the galaxy main sequence
Free accessEDP Sciences | 2023| -
Decoding the IRX–β dust attenuation relation in star-forming galaxies at intermediate redshift
Free accessEDP Sciences | 2023| -
Decoding the IRX-\beta\ dust attenuation relation in star-forming galaxies at intermediate redshift
Free accessArXiv | 2023| -
The ALMA-ALPINE [CII] survey: sub-kpc morphology of 3 main-sequence galaxy systems at z~4.5 revealed by ALMA
Free accessArXiv | 2023| -
Stellar metallicity from optical and UV spectral indices: Test case for WEAVE-StePS
Free accessEDP Sciences | 2023| -
Stellar metallicity from optical and UV spectral indices: Test case for WEAVE-StePS
Free accessArXiv | 2023|
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