Broadband Spectral Modeling of the Extreme Gigahertz-Peaked Spectrum Radio Source PKS B0008-421
J. R. Callingham, B. M. Gaensler, R. D. Ekers, S. J. Tingay, R. B., Wayth, J. Morgan, G. Bernardi, M. E. Bell, R. Bhat, J. D. Bowman, F. Briggs,, R. J. Cappallo, A. A. Deshpande, A. Ewall-Wice, L. Feng, L. J. Greenhill, B., J. Hazelton, L. Hindson, N. Hurley-Walker, D. C. Jacobs

TL;DR
This paper presents broadband spectral modeling of the extreme GPS source PKS B0008-421, revealing it as a relic source with a dense surrounding medium, and highlights the potential for future surveys to find similar sources.
Contribution
It introduces a Bayesian spectral fitting routine and demonstrates that a high-frequency spectral break and inhomogeneous free-free absorption best explain the source's spectrum, indicating a relic phase.
Findings
PKS B0008-421 has the steepest spectral slope below the turnover.
Inhomogeneous free-free absorption model is statistically favored.
The source likely ceased injecting fresh particles.
Abstract
We present broadband observations and spectral modeling of PKS B0008-421, and identify it as an extreme gigahertz-peaked spectrum (GPS) source. PKS B0008-421 is characterized by the steepest known spectral slope below the turnover, close to the theoretical limit of synchrotron self-absorption, and the smallest known spectral width of any GPS source. Spectral coverage of the source spans from 0.118 to 22 GHz, which includes data from the Murchison Widefield Array and the wide bandpass receivers on the Australia Telescope Compact Array. We have implemented a Bayesian inference model fitting routine to fit the data with various absorption models. We find that without the inclusion of a high-frequency exponential break the absorption models can not accurately fit the data, with significant deviations above and below the peak in the radio spectrum. The addition of a high-frequency break…
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