paper

Sun-related variability in the light curves of compact radio sources. A new view on Extreme Scattering Events

arXiv:2412.05373 · doi:10.1051/0004-6361/202346966

Abstract

An in-depth analysis of variability has been carried out on the 2 GHz and 8 GHz light curves from the impressive database of the US Navy's extragalactic source monitoring program at the Green Bank Interferometer (GBI), complemented by UMRAO light curves for selected sources. The data have been inspected in a search for one-year periodic patterns. Variations on timescales below one year have been isolated through a de-trending algorithm and analysed, looking for correlations with the Sun's position relative to the sources. Objects at ecliptic latitude below ~20deg show one-year periodic drops in flux densities, centred close to the time of minimum solar elongation; both interplanetary scintillation and instrumental effects may contribute to these events. However, in some cases the drops extend to much larger angular distances, affecting sources at high ecliptic latitudes, and causing variability on timescales of months. Three different kinds of such events have been identified in the data; their exact nature is not yet known. These events significantly alter the sources' variability characteristics estimated at GHz frequencies. In particular, we found that many extreme scattering events previously identified in the GBI monitoring program are the consequence of Sun-related effects; others occur simultaneously in several objects, which excludes interstellar scattering as their possible cause. These discoveries have a severe impact on our understanding of extreme scattering events. Furthermore, Sun-related variability can significantly alter results of variability studies, which are very powerful tools for the investigation of active galactic nuclei. Without a thorough comprehension of the mechanisms that cause these variations, the estimation of some essential information about the emitting regions, such as their size and all the derived quantities, might be seriously compromised.

20 pages, 14 figures, 3 tables. Accepted for publication in Astronomy & Astrophysics

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