Results 111 to 120 of about 512 (214)

The Influence of Microlensing on Time Delay Determinations in Double‐imaged Quasars

open access: yesThe Astrophysical Journal, 1998
The lag associated with the main peak of the cross-correlation function of the two light curves arriving from a double-imaged quasar is usually identified with the time delay between the components. However, short-timescale microlensing events can independently modify the light curve of each component, and when strong microlensing is present, the ...
Luis Julian Goicoechea   +4 more
openaire   +1 more source

Active Galactic Nuclei and Host Galaxies in COSMOS-Web. II. First Look At the Kiloparsec-scale Dual and Offset AGN Population

open access: yesThe Astrophysical Journal
Kiloparsec-scale dual and offset active galactic nuclei (AGNs) are signposts of accreting supermassive black holes (SMBHs) triggered during late-stage galaxy mergers, offering crucial insights into the coevolution of SMBHs and galaxies. However, robustly
Junyao Li   +5 more
doaj   +1 more source

The Gamma-Ray Luminosity Function of Flat-spectrum Radio Quasars

open access: yesThe Astrophysical Journal
We have utilized the largest sample of gamma-ray-selected Fermi flat-spectrum radio quasars (FSRQs) ever used (519 sources) to construct the luminosity function and its evolution through cosmic history. In addition to spanning large redshift (0 
Garima Rajguru   +4 more
doaj   +1 more source

The Role of Galaxies and Quasars in Reionising the High Redshift Intergalactic Medium [PDF]

open access: yes, 2020
Only one billion years after the Big Bang, the neutral hydrogen in the intergalactic medium had been completely ionised. This last phase transition of the Universe known as the epoch of reionisation is one of the frontiers in astrophysics.
Meyer, Romain A.
core  

Coherence of Supermassive Black Hole Binary Demographics with the nHz Stochastic Gravitational-wave Background

open access: yesThe Astrophysical Journal
We present a refined estimation of the stochastic gravitational-wave background (SGWB) based on observed dual active galactic nuclei (AGNs) together with AGN X-ray luminosity functions, in light of recent Pulsar Timing Array (PTA) detections of an nHz ...
Katsunori Kusakabe   +2 more
doaj   +1 more source

VODKA-JWST: A 3.8 kpc Dual Quasar at Cosmic Noon in a Powerful Starburst Galaxy with JWST/MIRI Integral Field Unit

open access: yesThe Astrophysical Journal
Dual quasars—two active supermassive black holes at galactic scales—represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation rate (SFR) within their host galaxies, particularly at cosmic noon when SFR ...
Yu-Ching Chen   +14 more
doaj   +1 more source

Discovery of 19 strongly lensed, dual, or projected quasars in DESI-LS

open access: yes
We report the results of a follow-up spectroscopic confirmation of two lensed quasars, six dual quasars, and eleven projected quasars that had previously been identified as lensed-quasar candidates in our earlier work.
Nan Li   +7 more
core   +1 more source

VODKA-JWST: Synchronized Growth of Two Supermassive Black Holes in a Massive Gas Disk? A 3.8 kpc Separation Dual Quasar at Cosmic Noon with the NIRSpec Integral Field Unit

open access: yesThe Astrophysical Journal
The search for dual supermassive black holes (SMBHs) is of immense interest in modern astrophysics. Galaxy mergers may fuel and produce SMBH pairs. Actively accreting SMBH pairs are observed as dual quasars, which are vital probes of SMBH growth.
Yuzo Ishikawa   +12 more
doaj   +1 more source

Quasars vs. Microquasars: Scaling and Particle Acceleration

open access: yes
Quasars and microquasars both contain accreting black holes and power nonthermal radio sources but differ in more than their scales: Quasars are proportionally much more efficient accelerators of energetic electrons.
Katz, J. I.
core  

High-resolution images of five radio quasars at early cosmological epochs

open access: yes, 2010
Context. Until now, there have only been seven quasars at z > 4.5 whose the high-resolution radio structure had been studied in detail with Very Long Baseline Interferometry (VLBI) imaging. Aims.
L. I. Gurvits   +4 more
core   +1 more source

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