Sfoglia per Autore
From simulations to observations: Methodology and data release of mock TNG50 galaxies at 0.3 < z < 0.7 for WEAVE-StePS
2025 Ikhsanova, A; Costantin, L; Pizzella, A; Corsini, E; Morelli, L; Ditrani, F; Ferré-Mateu, A; Gabarra, L; Gullieuszik, M; Haines, C; Iovino, A; Longhetti, M; Mercurio, A; Ragusa, R; Sánchez-Blázquez, P; Tortora, C; Vulcani, B; Zhou, S; Gafton, E; Pistis, F
Automated quasar continuum estimation using neural networks
2025 Pistis, F; Fumagalli, M; Fossati, M; Berg, T; Mangola, E; Dutta, R; Grespan, M; Iovino, A; Malek, K; Morrison, S; Murphy, D; Pearson, W; Perez-Rafols, I; Pieri, M; Pollo, A; Vergani, D
Attenuation proxy hidden in surface brightness - colour diagrams: A new strategy for the LSST era
2024 Malek, K; Junais, ; Pollo, A; Boquien, M; Buat, V; Salim, S; Brough, S; Demarco, R; Graham, A; Hamed, M; Mullaney, J; Romano, M; Sifon, C; Aravena, M; Benavides, J; Busa, I; Donevski, D; Dorey, O; Hernandez-Toledo, H; Nanni, A; Pearson, W; Pistis, F; Ragusa, R; Riccio, G; Roman, J
A comparative study of the fundamental metallicity relation: The impact of methodology on its observed evolution
2024 Pistis, F; Pollo, A; Figueira, M; Vergani, D; Hamed, M; Malek, K; Durkalec, A; Donevski, D; Salim, S; Iovino, A; Pearson, W; Romano, M; Scodeggio, M
Influence of star-forming galaxy selection on the galaxy main sequence
2023 Pearson, W; Pistis, F; Figueira, M; Małek, K; Moutard, T; Vergani, D; Pollo, A
Decoding the IRX-β dust attenuation relation in star-forming galaxies at intermediate redshift
2023 Hamed, M; Pistis, F; Figueira, M; Malek, K; Nanni, A; Buat, V; Pollo, A; Vergani, D; Bolzonella, M; Junais, ; Krywult, J; Takeuchi, T; Riccio, G; Moutard, T
X-ray luminosity-star formation rate scaling relation: Constraints from the eROSITA Final Equatorial Depth Survey (eFEDS)
2023 Riccio, G; Yang, G; Malek, K; Boquien, M; Junais, ; Pistis, F; Hamed, M; Grespan, M; Paolillo, M; Torbaniuk, O
The fundamental metallicity relation from SDSS (z ∼0) to VIPERS (z ∼0.7): Data selection or evolution
2022 Pistis, F; Pollo, A; Scodeggio, M; Figueira, M; Durkalec, A; Malek, K; Iovino, A; Vergani, D; Salim, S
SFR estimations from z = 0 to z = 0.9: A comparison of SFR calibrators for star-forming galaxies
2022 Figueira, M; Pollo, A; Malek, K; Buat, V; Boquien, M; Pistis, F; Cassara, L; Vergani, D; Hamed, M; Salim, S
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