Detection of stellar light from quasar host galaxies at redshifts above 6

X Ding, M Onoue, JD Silverman, Y Matsuoka, T Izumi… - Nature, 2023 - nature.com
The detection of starlight from the host galaxies of quasars during the reionization epoch (z>
6) has been elusive, even with deep Hubble Space Telescope observations,. The current …

A preferential growth channel for supermassive black holes in elliptical galaxies at z≲ 2

D Farrah, S Petty, KS Croker, G Tarlé… - The Astrophysical …, 2023 - iopscience.iop.org
The assembly of stellar and supermassive black hole (SMBH) mass in elliptical galaxies
since z∼ 1 can help to diagnose the origins of locally observed correlations between SMBH …

The Stellar Mass–Black Hole Mass Relation at z ∼ 2 down to Determined by HETDEX

Y Zhang, M Ouchi, K Gebhardt, C Liu… - The Astrophysical …, 2023 - iopscience.iop.org
The Stellar Mass–Black Hole Mass Relation at z ∼ 2 down to Determined by HETDEX -
IOPscience Skip to content IOP Science home Accessibility Help Search Journals Journals …

The eROSITA final equatorial-depth survey (eFEDS): host-galaxy demographics of X-ray AGNs with Subaru Hyper Suprime-Cam

J Li, JD Silverman, A Merloni, M Salvato… - Monthly Notices of …, 2024 - academic.oup.com
We investigate the physical properties, such as star-forming activity, disc versus bulge
nature, galaxy size, and obscuration of 3811 SRG/eROSITA-detected AGNs at 0.2< z< 0.8 in …

The Sloan Digital Sky Survey Reverberation Mapping Project: The Black Hole Mass–Stellar Mass Relations at 0.2≲ z≲ 0.8

I Jennifer, H Li, Y Shen, LC Ho, WN Brandt… - The Astrophysical …, 2023 - iopscience.iop.org
We measure the correlation between black hole mass M BH and host stellar mass M* for a
sample of 38 broad-line quasars at 0.2≲ z≲ 0.8 (median redshift z med= 0.5). The black hole …

The miniJPAS survey: AGN and host galaxy coevolution of X-ray-selected sources

IE López, M Brusa, S Bonoli, F Shankar… - Astronomy & …, 2023 - aanda.org
Studies indicate strong evidence of a scaling relation in the local Universe between the
supermassive black hole mass (M BH) and the stellar mass of their host galaxies (M⋆). They …

The black hole mass function across cosmic time. II. heavy seeds and (super) massive black holes

A Sicilia, A Lapi, L Boco, F Shankar… - The Astrophysical …, 2022 - iopscience.iop.org
This is the second paper in a series aimed at modeling the black hole (BH) mass function
from the stellar to the (super) massive regime. In the present work, we focus on (super) …

Active Galactic Nuclei and Host Galaxies in COSMOS-Web. I. NIRCam Images, Point-spread-function Models and Initial Results on X-Ray-selected Broad-line AGNs …

MY Zhuang, J Li, Y Shen - The Astrophysical Journal, 2024 - iopscience.iop.org
We present detailed and comprehensive data reduction and point-spread-function (PSF)
model construction for all public JWST NIRCam imaging data from the COSMOS-Web …

Morphological asymmetries of quasar host galaxies with Subaru Hyper Suprime-Cam

S Tang, JD Silverman, HM Yesuf, X Ding… - Monthly Notices of …, 2023 - academic.oup.com
How does the host galaxy morphology influence a central quasar or vice versa? We address
this question by measuring the asymmetries of 2424 SDSS quasar hosts at 0.2< z< 0.8 using …

Tracing the rise of supermassive black holes-A panchromatic search for faint, unobscured quasars at z≳ 6 with COSMOS-Web and other surveys

IT Andika, K Jahnke, M Onoue, JD Silverman… - Astronomy & …, 2024 - aanda.org
We report the identification of 64 new candidates of compact galaxies, potentially hosting
faint quasars with bolometric luminosities of L bol= 10 43–10 46 erg s− 1, residing in the …