Timing Analysis of Light Curves in the Tartarus Active Galactic Nuclei Database

Paul M. O'Neill; Kirpal Nandra; Iossif E. Papadakis; T. Jane Turner

doi:10.1063/1.1781024

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arXiv · astro-ph/0403569

Timing Analysis of Light Curves in the Tartarus Active Galactic Nuclei Database

Paul M. O'Neill·Kirpal Nandra·Iossif E. Papadakis·T. Jane Turner

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Abstract

The Tartarus database contains products for 529 ASCA observations of active galactic nuclei. We have been updating Tartarus to include observing sequences conducted after 1999 January. The revised database will contain products for 375 objects, with a total of 614 observing sequences. We have begun a systematic timing analysis of the Tartarus light curves. We present here some preliminary results of an investigation into the relation between excess variance and black-hole mass. Having optimised our analysis to minimize the scatter in the variance measurements, we find that the narrow-line active galactic nuclei follow roughly the same relation as the broad-line objects.

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Paul M. O'Neill, Kirpal Nandra, Iossif E. Papadakis, T. Jane Turner. 2004-03-24. Timing Analysis of Light Curves in the Tartarus Active Galactic Nuclei Database. https://doi.org/10.1063/1.1781024

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