:: Library Catalog

Image de couverture de livre

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Scharré, Lucie, Hirschmann, Michaela, Plat, Adèle, Charlot, Stephane, Somerville, Rachel S., Curtis-Lake, Emma, De Lucia, Gabriella, Dessauges-Zavadsky, Miroslava, Feltre, Anna, Farcy, Marion, Lahén, Natalia, Vijayan, Aswin P., Wilkins, Stephen M.
Format:	Preprint
Publié:	2026
Sujets:	Astrophysics of Galaxies
Accès en ligne:	https://arxiv.org/abs/2605.06769
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9
par: Cleri, Nikko J., et autres
Publié: (2026)

Characterising the z $\sim$ 7.66 Type-II AGN candidate SMACS S06355 using BEAGLE-AGN and JWST NIRSpec/NIRCam
par: Silcock, M. S., et autres
Publié: (2024)

On the origin of star formation quenching in massive galaxies at $z \gtrsim 3$ in the cosmological simulations IllustrisTNG
par: Kurinchi-Vendhan, Shalini, et autres
Publié: (2023)

Probing the dawn of galaxies: star formation and feedback in the JWST era through the GAEA model
par: Cantarella, Sebastiano, et autres
Publié: (2025)

Significant Evidence of an AGN Contribution in GHZ2 at z = 12.34
par: Ortiz, Oscar A. Chavez, et autres
Publié: (2025)

Properties of the brightest young stellar clumps in extremely lensed galaxies at redshifts 4 to 5
par: Messa, Matteo, et autres
Publié: (2024)

First Light and Reionization Epoch Simulations (FLARES) -- XVIII: the ionising emissivities and hydrogen recombination line properties of early AGN
par: Wilkins, Stephen M., et autres
Publié: (2025)

Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
par: Sinigaglia, Francesco, et autres
Publié: (2024)

Signatures of Very Massive Stars in the Epoch of Reionization
par: Marques-Chaves, Rui, et autres
Publié: (2026)

The Origins of Gas Accreted by Supermassive Black Holes: the Importance of Recycled Gas
par: Choi, Ena, et autres
Publié: (2023)

Semi-empirical constraints on the HI mass function of star-forming galaxies and $Ω_{\rm HI}$ at $z\sim 0.37$ from interferometric surveys
par: Sinigaglia, Francesco, et autres
Publié: (2025)

Reinterpreting the puzzling properties of z>6 galaxies within a variable IMF framework
par: Fontanot, Fabio, et autres
Publié: (2026)

Galactic bars are already mature at Cosmic Noon: bar strength and flatness at z ~ 1.5
par: Kalita, Boris S., et autres
Publié: (2025)

Do z>6 quasars reside in protoclusters?
par: Fontanot, Fabio, et autres
Publié: (2025)

Ly$α$ Emission Line Profiles of Extreme [OIII] Emitting Galaxies at $z\gtrsim2$: Implications for Ly$α$ Visibility in the Reionization Era
par: Tang, Mengtao, et autres
Publié: (2024)

What Builds and Quenches the Most Massive Galaxies in the Early Universe?
par: Xiao, Mengyuan, et autres
Publié: (2025)

The Effects of Stellar and AGN Feedback on the Cosmic Star Formation History in the Simba Simulations
par: Scharré, Lucie, et autres
Publié: (2024)

An innovative alternative to traditional funding streams for extragalactic astronomy
par: Wilkins, Stephen M., et autres
Publié: (2026)

Tracing star formation across cosmic time at tens of parsec-scales in the lensing cluster field Abell 2744
par: Claeyssens, Adélaïde, et autres
Publié: (2024)

Stellar Morphology of Optically Dark or Faint Galaxies at $z>3$ with JWST
par: Ganguly, Arpita, et autres
Publié: (2025)

Radio-astronomical Image Reconstruction with Conditional Denoising Diffusion Model
par: Drozdova, Mariia, et autres
Publié: (2024)

SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at $z=9.3$
par: Chen, Zuyi, et autres
Publié: (2026)

Like a candle in the wind: The embers of once aflame, now smouldering galaxies at $5 < z < 8$
par: Trussler, James, et autres
Publié: (2024)

The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
par: Turner, Jack C., et autres
Publié: (2025)

Cosmic quenching
par: De Lucia, Gabriella, et autres
Publié: (2025)

Where Giants Dwell: Probing the Environments of Early Massive Quiescent Galaxies
par: De Lucia, Gabriella, et autres
Publié: (2025)

Tracing the Quenching Journey across Cosmic Time
par: De Lucia, Gabriella, et autres
Publié: (2024)

Comité sobre Cuestiones Forestales del Mediterr neo de la FAO-Silva Mediterranea : revisión y perspectivas para 2020
par: Farcy, C
Publié: (2020)

Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim0.5$ and Quenching at All Radii Simultaneously at $z\sim1$
par: de la Vega, Alexander, et autres
Publié: (2025)

The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies
par: Partmann, Christian, et autres
Publié: (2024)

Leptonycteris nivalis
par: Hensley, Adele Pfrimmer, et autres
Publié: (1988)

Variation of the stellar initial mass function in semi-analytical models III: testing the cosmic ray regulated integrated galaxy-wide initial mass function
par: Fontanot, Fabio, et autres
Publié: (2023)

Unveiling dust, molecular gas, and high star formation efficiency in extremely UV bright star-forming galaxies at $z\sim 2.1-3.6$
par: Dessauges-Zavadsky, M., et autres
Publié: (2024)

Synthesizer: a Software Package for Synthetic Astronomical Observables
par: Lovell, Christopher C., et autres
Publié: (2025)

Efecto de una a amilasa (ec 3.2.1.1) en el patrón de consumo y eficiencia productiva de corderos alimentados con una dieta alta en concentrado
par: FX Plat
Publié: (2015)

Self-Supervised Learning on MeerKAT Wide-Field Continuum Images
par: Lastufka, Erica, et autres
Publié: (2024)

JWST/NIRSpec Observations of High Ionization Emission Lines in Galaxies at High Redshift
par: Tang, Mengtao, et autres
Publié: (2025)

Tau in Alzheimer's disease: Shaping the future patient journey
par: Douglas W. Scharre
Publié: (2025)

Dust evolution across cosmic times as seen through DUSTY-GAEA
par: Osman, Omima, et autres
Publié: (2025)

The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
par: Xie, Lizhi, et autres
Publié: (2025)