Copertina

JWST observations and a model for the extremely luminous obscured quasar W2246-0526 at z=4.6

Fuente: arXiv

Salvato in:

Dettagli Bibliografici
Autori principali:	Varnava, Charalambia, Efstathiou, Andreas, Díaz-Santos, Tanio, Farrah, Duncan
Natura:	Preprint
Pubblicazione:	2026
Soggetti:	Astrophysics of Galaxies
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi

Exploring the properties of the obscured hyperluminous quasar COS-87259 at z=6.853
di: Varnava, Charalambia, et al.
Pubblicazione: (2024)

Constraints on the active galactic nucleus and starburst activity of local ultraluminous infrared galaxies from a broad range of torus models
di: Varnava, Charalambia, et al.
Pubblicazione: (2025)

Ly$α$ imaging around the hyperluminous dust-obscured quasar W2246$-$0526 at $z=4.6$
di: Luo, Yibin, et al.
Pubblicazione: (2024)

SMART: spectral energy distributions Markov chain analysis with radiative transfer models
di: Varnava, Charalambia, et al.
Pubblicazione: (2024)

Resolving the black hole sphere of influence in a hyper-luminous obscured quasar at redshift 4.6
di: Liao, Mai, et al.
Pubblicazione: (2025)

A benchmark for extreme conditions of the multiphase interstellar medium in the most luminous hot dust-obscured galaxy at z = 4.6
di: Aranda, Román Fernández, et al.
Pubblicazione: (2024)

Resolving turbulence drivers in two luminous obscured quasars with JWST/NIRSpec IFU
di: Chen, Mandy C., et al.
Pubblicazione: (2024)

JWST IFU observations uncover host galaxy continua in extremely red and obscured quasars
di: Chen, Yu-Ching, et al.
Pubblicazione: (2025)

Powerful nuclear outflows and circumgalactic medium shocks driven by the most luminous known obscured quasar in the Universe
di: Vayner, Andrey, et al.
Pubblicazione: (2024)

A comparative study of galaxy evolution with four different active galactic nucleus torus models and two different host geometries
di: Papadopoulos, Michail, et al.
Pubblicazione: (2025)

HYPERION. Interacting companion and outflow in the most luminous $z>6$ quasar
di: Tripodi, R., et al.
Pubblicazione: (2023)

How accurately can obscured galaxy luminosities be measured using spectral energy distribution fitting of near- through far-infrared observations?
di: Farrah, Duncan, et al.
Pubblicazione: (2025)

Clumpy star formation and an obscured nuclear starburst in the luminous dusty z=4 galaxy GN20 seen by MIRI/JWST
di: Bik, A., et al.
Pubblicazione: (2023)

Escape fractions from unattenuated Ly$α$ emitters around luminous $z>6$ quasars
di: Yue, Minghao, et al.
Pubblicazione: (2025)

A deep X-ray look to the most obscured quasar at z~3.6 and its environment
di: Villani, I., et al.
Pubblicazione: (2025)

Simulated host galaxy analogs of high-z quasars observed with JWST
di: Berger, Sabrina, et al.
Pubblicazione: (2024)

Molecular gas excitation and outflow properties of obscured quasars at z$\sim$0.1
di: Audibert, A., et al.
Pubblicazione: (2025)

JWST UNCOVER: The Overabundance of Ultraviolet-luminous Galaxies at $z>9$
di: Chemerynska, Iryna, et al.
Pubblicazione: (2023)

Merging gas-rich galaxies that harbor low-luminosity twin quasars at z = 6.05: a promising progenitor of the most luminous quasars
di: Izumi, Takuma, et al.
Pubblicazione: (2024)

Multi-phase investigation of outflows in the circumgalactic and interstellar media of luminous quasars at z~5
di: Brazzini, Matilde, et al.
Pubblicazione: (2025)

MEOW: The increase in the obscured AGN fraction in mid-infrared from 0 < z < 6 with JWST MIRI
di: Bulichi, Teodora-Elena, et al.
Pubblicazione: (2026)

A lack of LAEs within 5Mpc of a luminous quasar in an overdensity at z=6.9: potential evidence of quasar negative feedback at protocluster scales
di: Lambert, Trystan S., et al.
Pubblicazione: (2024)

JWST's PEARLS: A z=6 quasar in a train-wreck galaxy merger system
di: Marshall, Madeline A., et al.
Pubblicazione: (2025)

The Soltan argument at $z=6$: UV-luminous quasars contribute less than 10% to early black hole mass growth
di: Jahnke, Knud
Pubblicazione: (2024)

Quantifying biases in stellar masses of JWST high-z quasar host galaxies caused by quasar subtraction
di: Berger, Sabrina, et al.
Pubblicazione: (2025)

Discovery and characterization of 25 new quasars at 4.6 < z < 6.9 from wide-field multi-band surveys
di: Belladitta, Silvia, et al.
Pubblicazione: (2025)

The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z=4-6
di: Mitsuhashi, Ikki, et al.
Pubblicazione: (2023)

Molecular Gas Heating, Star Formation Rate Relations, and AGN Feedback in Infrared-luminous Galaxy Mergers
di: Farrah, Duncan, et al.
Pubblicazione: (2025)

Very bright, very blue, and very red: JWST CAPERS analysis of highly luminous galaxies with extreme UV slopes at $\mathbf{z = 10}$
di: Donnan, Callum T., et al.
Pubblicazione: (2025)

NOEMA reveals the true nature of luminous red JWST z>10 galaxy candidates
di: Meyer, R. A., et al.
Pubblicazione: (2023)

The radio properties of z>3.5 quasars: Are most high-redshift radio-loud active galactic nuclei obscured?
di: Capetti, Alessandro, et al.
Pubblicazione: (2024)

Evidence for universal gas depletion in a sample of 41 luminous Type 1 quasars at z $\sim$ 2
di: Molyneux, S. J., et al.
Pubblicazione: (2025)

JWST observes the assembly of a massive galaxy at z~4
di: Saxena, Aayush, et al.
Pubblicazione: (2025)

The BoRG-$JWST$ Survey: Analogs at $z\sim8$ to the UV-luminous Galaxy Population at $z\gtrsim10$
di: Rojas-Ruiz, Sofía, et al.
Pubblicazione: (2025)

The role of environment in triggering AGN -- evidence for a change at $z\sim$1
di: Reeves, Jason, et al.
Pubblicazione: (2025)

Monster radio jet (>66 kpc) observed in quasar at z$\sim$5
di: Gloudemans, Anniek J., et al.
Pubblicazione: (2024)

A hidden population of active galactic nuclei can explain the overabundance of luminous $z>10$ objects observed by JWST
di: Hegde, Sahil, et al.
Pubblicazione: (2024)

Infrared fine-structure lines at high redshift
di: Decarli, Roberto, et al.
Pubblicazione: (2025)

Halfway to the Peak: ice absorption bands at $z\approx0.5$ with JWST MIRI/MRS
di: Sajina, Anna, et al.
Pubblicazione: (2025)

Deciphering the JWST spectrum of a 'little red dot' at $z \sim 4.53$: An obscured AGN and its star-forming host
di: Killi, Meghana, et al.
Pubblicazione: (2023)