Blue Monsters at $z>10$. Where has all their dust gone?
Fuente:
arXiv
Guardado en:
| Autores principales: | Ferrara, A., Pallottini, A., Sommovigo, L. |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
por: Pallottini, A., et al.
Publicado: (2024)
por: Pallottini, A., et al.
Publicado: (2024)
Beyond the first galaxies primordial black holes shine
por: Matteri, Antonio, et al.
Publicado: (2025)
por: Matteri, Antonio, et al.
Publicado: (2025)
Can primordial black holes explain the overabundance of bright super-early galaxies?
por: Matteri, Antonio, et al.
Publicado: (2025)
por: Matteri, Antonio, et al.
Publicado: (2025)
The eventful life of GS-z14-0, the most distant galaxy at redshift $z=14.32$
por: Ferrara, Andrea
Publicado: (2024)
por: Ferrara, Andrea
Publicado: (2024)
Dynamically cold disks in the early Universe: myth or reality?
por: Kohandel, Mahsa, et al.
Publicado: (2023)
por: Kohandel, Mahsa, et al.
Publicado: (2023)
Survival of dust in super-dusty galaxies at redshifts $z \approx 5-8$
por: Shchekinov, Yuri A., et al.
Publicado: (2025)
por: Shchekinov, Yuri A., et al.
Publicado: (2025)
Constraints on CMBR flux due to high-z dust emission
por: Lopez-Corredoira, Martin
Publicado: (2026)
por: Lopez-Corredoira, Martin
Publicado: (2026)
Learning the Universe: physically-motivated priors for dust attenuation curves
por: Sommovigo, Laura, et al.
Publicado: (2025)
por: Sommovigo, Laura, et al.
Publicado: (2025)
Inefficient dust production in a massive, metal-rich galaxy at $z=7.13$ uncovered by JWST and ALMA
por: Heintz, Kasper E., et al.
Publicado: (2025)
por: Heintz, Kasper E., et al.
Publicado: (2025)
Where are all the dark galaxies? Predicting galaxy/halo locations from their bright neighbors
por: Chen, Alice, et al.
Publicado: (2025)
por: Chen, Alice, et al.
Publicado: (2025)
High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
por: Kostyuk, Ivan, et al.
Publicado: (2025)
por: Kostyuk, Ivan, et al.
Publicado: (2025)
A$^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4 < z < 5$
por: Magnelli, Benjamin, et al.
Publicado: (2024)
por: Magnelli, Benjamin, et al.
Publicado: (2024)
Studying [CII] Emission in Low-mass Galaxies at z ~ 7
por: Glazer, Kelsey, et al.
Publicado: (2023)
por: Glazer, Kelsey, et al.
Publicado: (2023)
Strong Balmer break objects at z ~ 7-10 uncovered with JWST
por: Kuruvanthodi, A., et al.
Publicado: (2024)
por: Kuruvanthodi, A., et al.
Publicado: (2024)
Resolving the dusty star-forming galaxy GN20 at z=4.055 with NOEMA and JWST: A similar distribution of stars, gas and dust despite distinct apparent profiles
por: Boogaard, Leindert A., et al.
Publicado: (2025)
por: Boogaard, Leindert A., et al.
Publicado: (2025)
Is GN-z11 powered by a super-Eddington massive black hole?
por: Bhatt, Maulik, et al.
Publicado: (2024)
por: Bhatt, Maulik, et al.
Publicado: (2024)
Evolution of Massive Red Galaxies in Clusters from z=1.0 to z=0.3
por: Lin, Yen-Ting, et al.
Publicado: (2025)
por: Lin, Yen-Ting, et al.
Publicado: (2025)
Simulated [CII] in high-z galaxies
por: Muñoz-Elgueta, N., et al.
Publicado: (2024)
por: Muñoz-Elgueta, N., et al.
Publicado: (2024)
JWST-JADES. Possible Population III signatures at z=10.6 in the halo of GN-z11
por: Maiolino, Roberto, et al.
Publicado: (2023)
por: Maiolino, Roberto, et al.
Publicado: (2023)
The cosmic web's Lyman-$α$ glow at $z \approx 2.5$; varying hydrodynamic models, dust, and wide-field, narrow-band imaging detection
por: Sokoliuk, Oleksii, et al.
Publicado: (2025)
por: Sokoliuk, Oleksii, et al.
Publicado: (2025)
Redshift evolution of Lyman continuum escape fraction after JWST
por: Ferrara, A., et al.
Publicado: (2025)
por: Ferrara, A., et al.
Publicado: (2025)
The search for Population III: Confirmation of a HeII emitter with no metal lines at z=10.6
por: Maiolino, Roberto, et al.
Publicado: (2026)
por: Maiolino, Roberto, et al.
Publicado: (2026)
Pushing JWST to the extremes: search and scrutiny of bright galaxy candidates at z$\simeq$15-30
por: Castellano, M., et al.
Publicado: (2025)
por: Castellano, M., et al.
Publicado: (2025)
Improved measurements of the age of JWST galaxies at z=6-10
por: Lopez-Corredoira, M., et al.
Publicado: (2026)
por: Lopez-Corredoira, M., et al.
Publicado: (2026)
A 15 Mpc rotating galaxy filament at redshift z = 0.032
por: Tudorache, Madalina N., et al.
Publicado: (2025)
por: Tudorache, Madalina N., et al.
Publicado: (2025)
JWST NIRSpec spectroscopy of the triply-lensed $z = 10.17$ galaxy MACS0647$-$JD
por: Hsiao, Tiger Yu-Yang, et al.
Publicado: (2023)
por: Hsiao, Tiger Yu-Yang, et al.
Publicado: (2023)
Photometrically Selected Protocluster Candidates at z~9-10 in the JWST COSMOS-Web field
por: Wu, Cossas K. -W., et al.
Publicado: (2025)
por: Wu, Cossas K. -W., et al.
Publicado: (2025)
First direct carbon abundance measured at $z>10$ in the lensed galaxy MACS0647$-$JD
por: Hsiao, Tiger Yu-Yang, et al.
Publicado: (2024)
por: Hsiao, Tiger Yu-Yang, et al.
Publicado: (2024)
Stochastic star formation and the abundance of $z>10$ UV-bright galaxies
por: Kravtsov, Andrey, et al.
Publicado: (2024)
por: Kravtsov, Andrey, et al.
Publicado: (2024)
Ly$α$ visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z $\sim$ 7
por: Napolitano, L., et al.
Publicado: (2025)
por: Napolitano, L., et al.
Publicado: (2025)
JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
por: Polletta, M., et al.
Publicado: (2024)
por: Polletta, M., et al.
Publicado: (2024)
Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBE
por: Gjerløw, E., et al.
Publicado: (2026)
por: Gjerløw, E., et al.
Publicado: (2026)
Cosmoglobe DR2. VII. Towards a concordance model of large-scale thermal dust emission for microwave and infrared frequencies
por: Gjerløw, E., et al.
Publicado: (2026)
por: Gjerløw, E., et al.
Publicado: (2026)
Ubiquitous radio emission in quasars: predominant AGN origin and a connection to jets, dust and winds
por: Calistro-Rivera, G., et al.
Publicado: (2023)
por: Calistro-Rivera, G., et al.
Publicado: (2023)
Primordial black holes as supermassive black holes seeds
por: Ziparo, Francesco, et al.
Publicado: (2024)
por: Ziparo, Francesco, et al.
Publicado: (2024)
Using dust to constrain dark matter models
por: Ussing, Adam, et al.
Publicado: (2024)
por: Ussing, Adam, et al.
Publicado: (2024)
Magnetised CGM Gas at z~1 revealed by SPICE-RACS
por: Malik, Sunil, et al.
Publicado: (2026)
por: Malik, Sunil, et al.
Publicado: (2026)
Spectroscopic confirmation of the galaxy clusters CARLA J0950+2743 at z=2.363, and CARLA-Ser J0950+2743 at z=2.243
por: Grishin, Kirill A., et al.
Publicado: (2024)
por: Grishin, Kirill A., et al.
Publicado: (2024)
Stretch to stretch, dust to dust: lower-value local $H_{0}$ measurement from two-population modelling of type Ia supernovae
por: Wojtak, Radosław, et al.
Publicado: (2025)
por: Wojtak, Radosław, et al.
Publicado: (2025)
Statistical signatures of interstellar turbulence in dust polarization maps
por: Ho, Ka Wai, et al.
Publicado: (2024)
por: Ho, Ka Wai, et al.
Publicado: (2024)
Ejemplares similares
-
The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
por: Pallottini, A., et al.
Publicado: (2024) -
Beyond the first galaxies primordial black holes shine
por: Matteri, Antonio, et al.
Publicado: (2025) -
Can primordial black holes explain the overabundance of bright super-early galaxies?
por: Matteri, Antonio, et al.
Publicado: (2025) -
The eventful life of GS-z14-0, the most distant galaxy at redshift $z=14.32$
por: Ferrara, Andrea
Publicado: (2024) -
Dynamically cold disks in the early Universe: myth or reality?
por: Kohandel, Mahsa, et al.
Publicado: (2023)