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On Valency

published · living versions
W_nm4r9yd4·v1 · currentpublished
Cosmic evolution and metal aversion in super-luminous supernova host galaxies
with S. Schulze, T. Krühler, G. Leloudas, J. Gorosabel +19
1 version

Preprints & journals

131 papers in the corpus · 2002–2026
Probing IMF Variations in High-Redshift Early-Type Galaxies with SHARP2606.31189v1 · F. La Barbera, G. De Lucia, F. Ditrani et al.2026 · 0 citationsarXiv
A big step forward with SHARP: spatially resolved stellar population properties in passive galaxies at z > 1.52606.31628v1 · A. Gargiulo, C. Mancini, F. R. Ditrani et al.2026 · 1 citation2026NewA..12702578G
Fueling and feedback mechanisms at the nodes of the cosmic web2606.31671v1 · M. Polletta, G. De Lucia, A.R. Gallazzi et al.2026 · 0 citations2026, New Astronomy, Volume 127, id. 102561
SHARP -- A spectrograph proposal to fully exploit ELT capabilities and look beyond JWST2606.30721v1 · P. Saracco, P. Conconi, C. Arcidiacono et al.2026 · 1 citationarXiv
A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon2606.30763v1 · Chiara Mancini, Adriana Gargiulo, Alvio Renzini et al.2026 · 1 citation2026, NewA, 127, 102580
A novel data-driven approach to extract stellar population properties from galaxy spectra using absorption indices2606.13791v2 · Zahra Sharbaf, Ignacio Ferreras, Anna R. Gallazzi et al.2026 · 0 citationsMon Not R Astron Soc (2026)
Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing2604.01828v1 · Quirino D'Amato, Filippo Mannucci, Alessandro Sonnenfeld et al.2026 · 0 citationsNat Astron (2026)
There and back again? Neutral outflows in z~3.5 quiescent galaxies2602.17767v2 · Pengpei Zhu, Kei Ito, Francesco Valentino et al.2026 · 2 citationsA&A, 712, A169 (2026)
Decomposing the growth mechanisms of galaxies over the last 10 billion years2601.14666v1 · Luke J. M. Davies, Annagrazia Puglisi, Marcella Longhetti et al.2026 · 0 citationsarXiv
Archaeological investigation of galaxies' evolutionary history in the cosmic middle ages2512.16998v1 · Anna R. Gallazzi, Stefano Zibetti, Mark Sargent et al.2025 · 0 citationsarXiv
The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at z∼1z\sim12512.10383v2 · Angelos Nersesian, Yasha Kaushal, Marco Martorano et al.2025 · 1 citationA&A 705, A153 (2026)
LEGA-C stellar populations scaling relations. I: Chemo-archaeological downsizing trends at z~0.72512.07952v1 · Anna R. Gallazzi, Stefano Zibetti, Arjen van der Wel et al.2025 · 3 citationsA&A 708, A289 (2026)
Re-assessing the stellar population scaling relations of the galaxies in the Local Universe2509.04570v1 · D. Mattolini, S. Zibetti, A. R. Gallazzi et al.2025 · 7 citationsA&A 703, A5 (2025)
ChemicalUniverseMachine I: Uncovering the Cosmic Evolution of Metals in the Galaxy-ISM-CGM Ecosystem2503.10999v2 · Moka Nishigaki, Peter Behroozi, Masami Ouchi et al.2025 · 0 citationsarXiv
Gas outflows in two recently quenched galaxies at z = 4 and 72503.01990v3 · F. Valentino, K.E. Heintz, G. Brammer et al.2025 · 36 citationsA&A 699, A358 (2025)
More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector2502.03021v2 · Angelos Nersesian, Arjen van der Wel, Anna R. Gallazzi et al.2025 · 17 citationsA&A 695, A86 (2025)
From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function2408.12442v2 · Dingyi Zhao, Yingjie Peng, Yipeng Jing et al.2024 · 9 citationsApJ 979 42 (2025)
SHARP -- A near-IR multi-mode spectrograph conceived for MORFEO@ELT2407.06264v3 · P. Saracco, P. Conconi, C. Arcidiacono et al.2024 · 5 citationsarXiv
From Halos to Galaxies. IX. Estimate of Halo Assembly History for SDSS Galaxy Groups2407.03409v1 · Cheqiu Lyu, Yingjie Peng, Yipeng Jing et al.2024 · 5 citationsarXiv
Retrieval of the physical parameters of galaxies from WEAVE-StePS-like data using machine learning2406.11748v1 · J. Angthopo, B.R. Granett, F. La Barbera et al.2024 · 5 citationsarXiv
The Wide-field Spectroscopic Telescope (WST) Science White Paper2403.05398v2 · Vincenzo Mainieri, Richard I. Anderson, Jarle Brinchmann et al.2024 · 15 citationsarXiv
On the maximum age resolution achievable through stellar population synthesis models2401.07335v1 · Stefano Zibetti, Edoardo Rossi, Anna R. Gallazzi2024 · 15 citationsarXiv
Stars, gas, and star formation of distant post-starburst galaxies2308.08681v1 · Po-Feng Wu, Rachel Bezanson, Francesco D'Eugenio et al.2023 · 16 citationsarXiv
Stellar metallicity from optical and UV spectral indices: Test case for WEAVE-StePS2308.02635v1 · F. R. Ditrani, M. Longhetti, F. La Barbera et al.2023 · 6 citationsA&A 677, A93 (2023)
The large molecular gas fraction of post-starburst galaxies at z > 12306.08120v1 · A. Zanella, F. Valentino, A. Gallazzi et al.2023 · 16 citationsarXiv
The Gas-Phase Mass--Metallicity Relation for Massive Galaxies at z∼0.7z\sim0.7 with the LEGA-C Survey2304.12343v1 · Zach J. Lewis, Brett H. Andrews, Rachel Bezanson et al.2023 · 2 citationsarXiv
An Atlas of Color-selected Quiescent Galaxies at z>3z>3 in Public JWSTJWST Fields2302.10936v1 · Francesco Valentino, Gabriel Brammer, Katriona M. L. Gould et al.2023 · 215 citationsarXiv
WEAVE-StePS. A stellar population survey using WEAVE at WHT2302.07366v1 · A. Iovino, B. M. Poggianti, A. Mercurio et al.2023 · 20 citationsA&A 672, A87 (2023)
LEGA-C: analysis of dynamical masses from ionized gas and stellar kinematics at z~0.82203.06194v1 · Caroline M.S. Straatman, Arjen van der Wel, Josha van Houdt et al.2022 · 7 citationsarXiv
REQUIEM-2D: A diversity of formation pathways in a sample of spatially-resolved massive quiescent galaxies at z~22203.04979v1 · Mohammad Akhshik, Katherine E. Whitaker, Joel Leja et al.2022 · 24 citationsarXiv
Stellar mass as the "glocal" driver of galaxies' stellar population properties2202.03975v1 · Stefano Zibetti, Anna R. Gallazzi2022 · 18 citationsarXiv
Ubiquitous [OII] Emission in Quiescent Galaxies at z ~ 0.852110.00009v1 · Michael V. Maseda, Arjen van der Wel, Marijn Franx et al.2021 · 18 citationsarXiv
Career total: at least 238 works. 131 are in this corpus.Showing the 50 most recent.

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