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Table · dataset · 2015

SEAMBHs IV. H{beta} time lags

Listed in IVOA Registry (Virtual Observatory)

We have completed two years of photometric and spectroscopic monitoring of a large number of active galactic nuclei (AGNs) with very high accretion rates.

Description

In this paper, we report on the result of the second phase of the campaign, during 2013-2014, and the measurements of five new H{beta} time lags out of eight monitored AGNs. All five objects were identified as super-Eddington accreting massive black holes (SEAMBHs).

The highest measured accretion rates for the objects in this campaign are dM/dt>~200, where dM/dt=dM/dt_{dot}_/L_Edd_C^-2^, dM/dt_{dot}_ is the mass accretion rates, L_Edd_ is the Eddington luminosity and c is the speed of light.

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Catalogue records · 2

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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/apj/806/2215 d agoJSON v1
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access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
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updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0