2025ApJ...983...55K


Query : 2025ApJ...983...55K

2025ApJ...983...55K - Astrophys. J., 983, 55 (2025/April-2)

JWST Spectroscopic View of a Rapidly Growing, Dust-obscured Quasar at z ∼ 4: Effect of Dust Extinction Correction on Black Hole Mass and Eddington Ratio Estimation.

KIM D. and IM M.

Abstract (from CDS):

In the merger-driven galaxy evolution scenario, the central supermassive black holes (SMBHs) in dust-obscured galaxies grow rapidly. Interestingly, a recent work on a dust-obscured galaxy, LID-568 at z = 3.965, has shown that its SMBH is growing extremely fast at about 40 times the Eddington-limited accretion rate (i.e., super-Eddington accretion). However, the heavy dust extinction of the host galaxy could affect the result if not corrected properly. Here, we analyze James Webb Space Telescope (JWST) NIRSpec integral field unit (IFU) and MIRI spectra of LID-568. By measuring its bolometric luminosity (Lbol) and black hole (BH) mass (MBH) using an extinction-free estimator based on mid-infrared spectra, we obtain Lbol = 1046.83±0.07 erg s–1 and MBH = 108.43±0.15M⊙. The measured Eddington ratio (λEdd) is 1.97 ± 0.88, consistent with the accretion rate at the Eddington limit; in other words, it is not super-Eddington in a significant manner. This result underscores challenges and the importance of carefully considering dust extinction when analyzing the BH growth in dust-obscured quasars.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Galaxy evolution - Early universe - Supermassive black holes - Quasars - James Webb Space Telescope - Infrared astronomy

Simbad objects: 1

goto Full paper

goto View the references in ADS

Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 COSMOS2015 943473 AGN 09 58 44.116 +02 44 06.57           ~ 6 0

Query : 2025ApJ...983...55K

Basic data :
COSMOS2015 943473 -- Active Galaxy Nucleus
Other object types:
otypes_help
AGN (2019ApJ), G (2016ApJ), X ([CMC2016])
ICRS coord. (ep=J2000) :
09 58 44.116 +02 44 06.57 (Optical) [ ] C 2016ApJ...817...34M
FK4 coord. (ep=B1950 eq=1950) :
09 56 08.674 +02 58 28.85 [ ]
Gal coord. (ep=J2000) :
235.901463 +42.071077 [ ]
Radial velocity / Redshift / cz :
V(km/s) 276418 [~] / z(spectroscopic) 3.965 [~] / cz 1188677 [~]
   (NIR) D 2025NatAs...9..271S
Fluxes (1) :
i (AB) 26.50 [0.27] C 2016ApJ...817...34M
SIMBAD within arcmin
Overlay Simbad points in this preview
Back
All CDSPortal (CDSPortal)

Send to sendBySAMP sendBySAMP

sedIcon
within arcsec sed-help-icon

Identifiers (2) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

COSMOS2015 943473 [CMC2016] lid 568

References (6 between 1850 and 2026) (Total 6)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
Follow new references on this object
                Reference summaries :

                from: to:

                 or select by : (not exhaustive, explanation here)


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Search by coordinates in Vizier (radius: 5 arcsec)


Annotations :
Annotations allow a user to add a note or report an error concerning the astronomical object and its data. It requires registration to post a note. See description .
Please, have a look at Best practices. The list of all annotations to SIMBAD objects can be found here .

The annotation server is currently not available. Sorry for any inconvenience


To bookmark this query, right click on this link: simbad:objects in 2025ApJ...983...55K and select 'bookmark this link' or equivalent in the popup menu