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Table · dataset · 2022

3yrs spectroscopic light curves of PG0026+129

Listed in IVOA Registry (Virtual Observatory)

We report on the results of a new spectroscopic monitoring campaign of the quasar PG 0026+129 at the Calar Alto Observatory 2.2m telescope from 2017 July to 2020 February.

Description

Significant variations in the fluxes of the continuum and broad emission lines, including H{beta} and HeII, were observed in the first and third years, and clear time lags between them are measured. The broad H{beta} line profile consists of two Gaussian components: an intermediate-width H{beta}_IC_ with an FWHM of 1964+/-18km/s and another very broad H{beta}_VBC_ with an FWHM of 7570+/-83km/s.

H{beta}_IC_ has long time lags of ~40-60days in the rest frame, while H{beta}_VBC_ shows nearly zero time delay with respect to the optical continuum at 5100{AA}. The velocity-resolved delays show consistent results: lags of ~30-50days at the core of the broad H{beta} line and roughly zero lags at the wings. H{beta}_IC_ has a redshift of ~400km/s, which seems to be stable for nearly 30yr by comparing with archived spectra, and may originate from an infall.

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The rms spectrum of H{beta}_VBC_ shows a double-peaked profile with brighter blue peak and extended red wing in the first year, which matches the signature of a thin disk. Both the double-peaked profile and the near-zero lag suggest that H{beta}_VBC_ comes from a region associated with the part of the accretion disk that emits the optical continuum. Adopting the FWHM (in the rms spectrum) and the time lag measured for the total H{beta} line, and a virial factor of 1.5, we obtain a virial mass of 2.89_-0.69_^+0.60^x10^7^M_{sun}_ for the central black hole in this quasar.

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