Imagen de Portada

The brightest X-ray AGNs at redshift $3\lesssim z \lesssim 6$

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Heather, Cameron, Chantavat, Teeraparb, Chongchitnan, Siri, Chainakun, Poemwai
Formato:	Preprint
Publicado:	2025
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Extreme-value modelling of the brightest galaxies at $z\gtrsim9$
por: Heather, Cameron, et al.
Publicado: (2024)

Extreme Values of Black Hole to Stellar Mass Ratio for High-Redshift Galaxies
por: Heather, Cameron, et al.
Publicado: (2026)

NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at $3\lesssim z\lesssim 6$
por: Zhuang, Ming-Yang, et al.
Publicado: (2025)

Chronicling the reionization history at $6\lesssim z \lesssim 7$ with emergent quasar damping wings
por: Ďurovčíková, Dominika, et al.
Publicado: (2024)

Lyman Continuum Emission from AGN at 2.3$\lesssim$z$\lesssim$3.7 in the UVCANDELS Fields
por: Smith, Brent M., et al.
Publicado: (2024)

Angular correlation functions of bright Lyman-break galaxies at $\mathbf{3 \lesssim z \lesssim 5}$
por: Ye, Isabelle, et al.
Publicado: (2025)

JWST/NIRSpec Observations of Ly$α$ Emission in Star Forming Galaxies at $6.5\lesssim z\lesssim13$
por: Tang, Mengtao, et al.
Publicado: (2024)

The Lyman Continuum Escape Fraction of Star-forming Galaxies at $2.4\lesssim z\lesssim3.0$ from UVCANDELS
por: Wang, Xin, et al.
Publicado: (2023)

Age and metal gradients in massive quiescent galaxies at $0.6 \lesssim z \lesssim 1.0$: implications for quenching and assembly histories
por: Cheng, Chloe M., et al.
Publicado: (2024)

A 3D view on the local gravitational instability of cold gas discs in star-forming galaxies at $0 \lesssim \mathrm{z} \lesssim 5$
por: Bacchini, C., et al.
Publicado: (2024)

The MAGPI Survey: co-evolution of baryons and dark matter in star-forming disk-like galaxies at $0.1 \lesssim z \lesssim 0.85$
por: Sharma, Gauri, et al.
Publicado: (2026)

Early Results from GLASS-JWST. XXV. Electron Density in the Interstellar Medium at $0.7\lesssim z\lesssim 9.3$ with NIRSpec High-resolution Spectroscopy
por: Li, Sijia, et al.
Publicado: (2024)

Constraining $z\lesssim 2$ ultraviolet emission with the upcoming ULTRASAT satellite
por: Libanore, Sarah, et al.
Publicado: (2024)

The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning $0.2 \lesssim z \lesssim 15$
por: Wang, Bingjie, et al.
Publicado: (2023)

Clues to inside-out quenching in quiescent galaxies at $1.2\lesssim z\lesssim2.2$: Age, Fe-, and Mg-abundance gradients from JWST-SUSPENSE
por: Cheng, Chloe M., et al.
Publicado: (2025)

Clumps in spiral galaxies at $z \lesssim 3$: Disentangling two spatial modes of star formation
por: Chugunov, Ilia V., et al.
Publicado: (2026)

The Evolution of Size and Merger Fraction of Submillimeter Galaxies across $1 < z \lesssim 6$ as Observed by JWST
por: Ren, Jian, et al.
Publicado: (2025)

The Cosmic Ultraviolet Baryon Survey (CUBS) VII: on the warm-hot circumgalactic medium probed by O VI and Ne VIII at 0.4 $\lesssim$ z $\lesssim$ 0.7
por: Qu, Zhijie, et al.
Publicado: (2024)

Less Wound and More Asymmetric: JWST Confirms the Evolution of Spiral Structure in Galaxies at $z \lesssim 3$
por: Chugunov, Ilia V., et al.
Publicado: (2025)

Extending the Frontier of Spatially-Resolved Supermassive Black Hole Mass Measurements to at $1\lesssim z\lesssim2$: Simulations with ELT/MICADO High-Resolution Mass Models and HARMONI Integral-Field Stellar Kinematics
por: Nguyen, Dieu D., et al.
Publicado: (2025)

Morphological evolution of disk galaxies and their concentration, asymmetry and clumpiness (CAS) properties in simulations across Toomre's $Q$ parameter
por: Chantavat, Teeraparb, et al.
Publicado: (2024)

The Size Evolution and the Size-Mass Relation of Lyman-Alpha Emitters across $3 \lesssim z < 7$ as Observed by JWST
por: Song, Qi, et al.
Publicado: (2025)

A Survey of H I and O VI Absorption Lines in the Outskirts of $z\lesssim0.3$ Galaxy Clusters
por: Luna, Priscilla Holguin, et al.
Publicado: (2024)

Eddington Ratios of Dust-obscured Quasars at $z \lesssim 1$: Evidence Supporting Dust-obscured Quasars as Young Quasars
por: Kim, Dohyeong, et al.
Publicado: (2024)

Extraction method for response functions from X-ray light curves of AGN by optimization algorithm
por: Deesamutara, Sanhanat, et al.
Publicado: (2026)

JWST + ALMA ubiquitously discover companion systems within $\lesssim18\,$kpc around four $z$$\approx$3.5 luminous radio-loud AGN
por: Wang, Wuji, et al.
Publicado: (2025)

Gas content and evolution of a sample of YSO associations at $d \lesssim$ 3.5 kpc from the Sun
por: Zhou, Ji-Xuan, et al.
Publicado: (2024)

The Magellan M2FS spectroscopic survey of high-redshift galaxies: the brightest Lyman-break galaxies at $z \sim 6$
por: Fu, Shuqi, et al.
Publicado: (2024)

Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion
por: Inayoshi, Kohei, et al.
Publicado: (2024)

The Halo Occupation Distribution Modeling of the X-ray-selected AGNs at 0.6 < z < 2.6 in the COSMOS field
por: Ikeda, Hiroyuki, et al.
Publicado: (2025)

Cosmic Chance Superpositions: Largest Catalog of Quasar-Galaxy Pairs at a Projected Separation of $D \lesssim 20$ kpc
por: Guha, Labanya Kumar, et al.
Publicado: (2026)

Parameter dependency on the public X-ray reverberation models kynxilrev and kynrefrev
por: Khanthasombat, K., et al.
Publicado: (2024)

Identifying AGNs from X-ray detections-I: Metallicity calibrations in AGNs with X-ray luminosity as the primary input parameter
por: Armah, Mark, et al.
Publicado: (2026)

Properties of the brightest young stellar clumps in extremely lensed galaxies at redshifts 4 to 5
por: Messa, Matteo, et al.
Publicado: (2024)

Identifying Compton-thick AGNs in the COSMOS. I. Among X-ray AGNs with Low Photon Counts
por: Guo, Xiaotong, et al.
Publicado: (2025)

Low-ionization Metal Absorption at $0.7 \lesssim z \lesssim 2$ Confronting Cosmological Simulations with Observations
por: Rapoport, Ivan, et al.
Publicado: (2026)

Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\lesssim$100 parsec in nearby star-forming galaxies from PHANGS
por: Jing, Tao, et al.
Publicado: (2025)

AGNfitter-rx: Modelling the radio-to-X-ray SEDs of AGNs
por: Martínez-Ramírez, L. N., et al.
Publicado: (2024)

Widespread AGN feedback in a forming brightest cluster galaxy at $z=4.1$ unveiled by JWST
por: Saxena, Aayush, et al.
Publicado: (2024)

Molecular gas properties of star-forming brightest group galaxies at $z \sim 0.3$
por: Toni, Greta, et al.
Publicado: (2026)