Interstellar scintillation is an indicator of astrometric stability

TL;DR

This study links interstellar scintillation with astrometric stability in quasars, showing persistent scintillators are more stable and compact, making them ideal for celestial reference frames.

Contribution

It introduces a new metric for source position stability and demonstrates the correlation between scintillation type and astrometric stability in quasars.

Findings

Persistent scintillators have greater positional stability.

Scintillators are more compact on milliarcsecond scales.

Slow scintillators are more stable than rapid ones.

Abstract

We examine the relationship between astrometric stability and astrophysical properties in flat-spectrum radio-loud quasars making up the celestial reference frame. We use position determinations from geodetic VLBI measurements, and develop a new metric for source position stability. We then compare this quantity to two measures of source compactness: structure index, which probes structure on milliarcsecond scales; and the presence of interstellar scintillation associated with the quasar, which probes scales of tens of microarcseconds. We find that persistent scintillators have greater position stability than episodic scintillators, which are in turn more stable than non-scintillators. Scintillators are also more likely to be compact on milliarcsecond scales, as measured by the structure index. Persistent scintillators are therefore excellent candidates for inclusion in any future realisation of the celestial reference frame. A list of these sources is presented in the Appendix. We find that slow (characteristic timescale >3 days) scintillators have more stable positions than rapid scintillators, suggesting they are more compact. High-cadence, long term monitoring is therefore required to identify other members of this population of compact, high brightness temperature quasars.