activity
19942026
most citedCoevolution (Or Not) of Supermassive Black Holes and Host Galaxies

4.2k citations · 53.7k across the 547 of their papers we have counts for

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303 papers · 1 filter

astro-ph.GA2026

Searching for Nearby Supermassive Black Hole Binaries with GRAVITY

GRAVITY Collaboration, K. Abd El Dayem, N. Aimar +82

We present a systematic interferometric search for close supermassive black hole (SMBH) binaries in 20 nearby type 1 active galactic nuclei (AGN) observed with VLTI/\grav. We inves…

astro-ph.GA2025

Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XII. Reverberation Mapping Results for 15 PG Quasars from a Long-Duration High-Cadence Campaign

Chen Hu, Sha-Sha Li, Sen Yang +15

We present the first results from long-term high-cadence spectroscopic monitoring of 15 PG quasars with relatively strong Fe II emission as a part of a broader reverberation mappin…

astro-ph.GA2023

Star Formation in Self-gravitating Disks in Active Galactic Nuclei. III. Efficient Production of Iron and Infrared Spectral Energy Distributions

J. -M. Wang, S., Zhai +7

Strong iron lines are a common feature of the optical spectra of active galactic nuclei (AGNs) and quasars from to the local Universe, and [Fe/Mg] ratios do not show co…

astro-ph.GA2023★ 1 cited

The Structure and Morphology of Galaxies during the Epoch of Reionization Revealed by JWST

Wen Sun, Luis C. Ho, Ming-Yang Zhuang +3

We analyze 347 galaxies at redshift using JWST observations from the CEERS program by fitting a two-dimensional parametric model simultaneously to the seven-filter NIRCam…

astro-ph.GA2023

VLBI Observations of a sample of Palomar-Green quasars II: characterising the parsec-scale radio emission

Ailing Wang, Tao An, Yingkang Zhang +4

This study uses multi-frequency Very Long Baseline Interferometry (VLBI) to study the radio emission from 10 radio-quiet quasars (RQQs) and four radio-loud quasars (RLQs). The dive…

astro-ph.GA2023

On the dominant role of wind in the quasar feedback mode in the late stage evolution of massive elliptical galaxies

Bocheng Zhu, Feng Yuan, Suoqing Ji +2

In this paper we investigate the role of AGN feedback on the late stage evolution of elliptical galaxies by performing high-resolution hydrodynamical simulation in the {\it MACER}…

astro-ph.GA2023★ 12 cited

White Dwarf--White Dwarf collisions in AGN discs via close encounters

Yan Luo, Xiao-Jun Wu, Shu-Rui Zhang +3

White dwarfs (WDs) in active galactic nucleus (AGNs) discs might migrate to the inner radii of the discs and form restricted three-body systems with two WDs moving around the centr…

astro-ph.GA2023★ 65 cited

Evolutionary Paths of Active Galactic Nuclei and Their Host Galaxies

Ming-Yang Zhuang, Luis C. Ho

The tight correlations between the masses of supermassive black holes (BHs) and the properties of their host galaxies suggest that BHs coevolve with galaxies. However, what is the…

astro-ph.GA2023

Photometric Selection of Unobscured QSOs in the Ecliptic Poles: KMTNet in the South Field and Pan-STARRS in the North Field

Woowon Byun, Minjin Kim, Yun-Kyeong Sheen +18

We search for quasi-stellar objects (QSOs) in a wide area of the south ecliptic pole (SEP) field, which has been and will continue to be intensively explored through various space…

astro-ph.GA2023★ 11 cited

The Subtle Effects of Mergers on Star Formation in Nearby Galaxies

Yang A. Li, Luis C. Ho, Jinyi Shangguan

Interactions and mergers play an important role in regulating the physical properties of galaxies, such as their morphology, gas content, and star formation rate (SFR). Controversy…

astro-ph.GA2023★ 13 cited

Panchromatic Photometry of Low-redshift, Massive Galaxies Selected from SDSS Stripe 82

Yang A. Li, Luis C. Ho, Jinyi Shangguan +2

The broadband spectral energy distribution of a galaxy encodes valuable information on its stellar mass, star formation rate (SFR), dust content, and possible fractional energy con…

astro-ph.GA2023★ 19 cited

Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission

Joel Bregman, Renyue Cen, Yang Chen +51

The Hot Universe Baryon Surveyor (HUBS) is a proposed space-based X-ray telescope for detecting X-ray emissions from the hot gas content in our universe. With its unprecedented spa…

astro-ph.GA2023

Deficit of Hot Dust in Low-redshift Active Galactic Nuclei

Suyeon Son, Minjin Kim, Luis C. Ho

We assemble a broad-band spectral energy distribution (SED) ranging from optical to mid-infrared of nearby active galactic nuclei at . SED fitting analysis is performed us…

astro-ph.GA2023★ 1 cited

Galaxy Light profile neural Networks (GaLNets). II. Bulge-Disc decomposition in optical space-based observations

Chen Qiu, Nicola R. Napolitano, Rui Li +12

Bulge-disk (B-D) decomposition is an effective diagnostic to characterize the galaxy morphology and understand its evolution across time. So far, high-quality data have allowed det…

astro-ph.GA2023

Nobeyama 45-m CO J=1-0 Observations of Luminous Type 1 AGNs at

Tomonari Michiyama, Ming-Yang Zhuang, Jinyi Shangguan +3

We have performed CO J =1-0 observations of ten galaxies hosting luminous () type 1 active galactic nuclei (AGNs) with the Nobeyama 45-m r…

astro-ph.GA2023★ 10 cited

Mildly Relativistic Motion in the Radio Quiet Quasar PG 1351+640

Ailing Wang, Tao An, Shaoguang Guo +8

Measuring the proper motion of the emission component in radio-quiet quasars (RQQs) could help to distinguish between the origins of the radio emission and to understand whether th…

astro-ph.GA2023★ 5 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Key Results

Yue Shen, Catherine J. Grier, Keith Horne +44

We present the final data from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project, a precursor to the SDSS-V Black Hole Mapper Reverberation Mapping program. This…

astro-ph.GA2023★ 1 cited

Radio Polarization: A Powerful Resource for Understanding the Blazar Divide

Janhavi Baghel, P. Kharb, Silpa S. +2

With high-sensitivity kiloparsec-scale radio polarimetry, we can examine the jet-medium interactions and get a better understanding of the blazar divide in radio-loud (RL) AGN. We…

astro-ph.GA2023★ 10 cited

Lack of Correlations between Cold Molecular Gas and AGN Properties in Type 1 AGNs at

Juan Molina, Jinyi Shangguan, Ran Wang +3

We present new NOrthern Extended Millimeter Array (NOEMA) observations of the CO(2--1) emission in eight of the brightest Palomar-Green quasars at to investigate t…

astro-ph.GA2023★ 15 cited

FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group

Xuchen Lin, Jing Wang, Virginia Kilborn +27

Combining new HI data from a synergetic survey of ASKAP WALLABY and FAST with the ALFALFA data, we study the effect of ram pressure and tidal interactions in the NGC 4636 group. We…

astro-ph.GA2023★ 24 cited

Diverse Molecular Structures Across The Whole Star-Forming Disk of M83: High fidelity Imaging at 40pc Resolution

Jin Koda, Akihiko Hirota, Fumi Egusa +23

We present high-fidelity CO(1-0) imaging of molecular gas across the full star-forming disk of M83, using ALMA's 12m, 7m, and TP arrays and the MIRIAD package. The data have a mass…

astro-ph.GA2023★ 7 cited

Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow

Bocheng Zhu, Feng Yuan, Suoqing Ji +4

The cosmological inflow of a galaxy is speculated to be able to enter the galaxy and enhance the star formation rate (SFR) and black hole accretion rate (BHAR). In this paper, by p…

astro-ph.GA2023★ 7 cited

Dynamics of Molecular Gas in the Central Region of the Quasar IZwicky1

Qinyue Fei, Ran Wang, Juan Molina +4

We present a study of the molecular gas distribution and kinematics in the cicumnuclear region (radii kpc) of the quasar IZwicky1 using a coll…

astro-ph.GA2023★ 21 cited

Testing Super-Eddington Accretion onto a Supermassive Black Hole: Reverberation Mapping of PG 1119+120

Fergus R. Donnan, Juan V. Hernández Santisteban, Keith Horne +11

We measure the black hole mass and investigate the accretion flow around the local () quasar PG 1119+120. Spectroscopic monitoring with Calar Alto provides H lags and…