Discovery of a binary quasar at z~0.2 with 430 pc separation indicating a bound SMBH pair each >4e8 Msun, with 2.5 Gyr upper limit on merger timescale and implications for the PTA gravitational wave background.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
verdicts
UNVERDICTED 4representative citing papers
AGN with black-hole masses above 10^8.5 solar masses may occupy halos ~0.4 dex more massive than matched control galaxies, though the difference remains consistent with uncertainties.
X-ray AGN at intermediate redshifts live in dark matter halos of mass ~10^13 solar masses with no significant dependence on black hole mass, Eddington ratio or X-ray luminosity.
Calculations show current pulsar timing arrays have poor prospects for detecting gravitational wave memory, but LISA is likely to see 1-10 events with SNR exceeding 5 in its 4-year mission.
citing papers explorer
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Discovery of a close-separation binary quasar at the heart of a z~0.2 merging galaxy and its implications for low-frequency gravitational waves
Discovery of a binary quasar at z~0.2 with 430 pc separation indicating a bound SMBH pair each >4e8 Msun, with 2.5 Gyr upper limit on merger timescale and implications for the PTA gravitational wave background.
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Black hole mass, host galaxy mass, and dark matter halos: Testing the environmental connection
AGN with black-hole masses above 10^8.5 solar masses may occupy halos ~0.4 dex more massive than matched control galaxies, though the difference remains consistent with uncertainties.
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Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos
X-ray AGN at intermediate redshifts live in dark matter halos of mass ~10^13 solar masses with no significant dependence on black hole mass, Eddington ratio or X-ray luminosity.
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Prospects for Memory Detection with Low-Frequency Gravitational Wave Detectors
Calculations show current pulsar timing arrays have poor prospects for detecting gravitational wave memory, but LISA is likely to see 1-10 events with SNR exceeding 5 in its 4-year mission.