On the reliability of microvariability tests in quasars
Jos\'e A. de Diego

TL;DR
This paper evaluates the reliability of statistical tests used to detect microvariability in quasars, highlighting the limitations of common methods and proposing improved approaches for more accurate results.
Contribution
It demonstrates the superiority of the Analysis of Variance test over traditional F-tests and suggests combining data from multiple stars to enhance detection reliability.
Findings
ANOVA test outperforms F-test in microvariability detection
Combining data from multiple comparison stars improves test reliability
Inappropriate use of certain tests can lead to unreliable detections
Abstract
Microvariations probe the physics and internal structure of quasars. Unpredictability and small flux variations make this phenomenon elusive and difficult to detect. Variance based probes such as the C and F tests, or a combination of both, are popular methods to compare the light-curves of the quasar and a comparison star. Recently, detection claims in some studies depend on the agreement of the results of the C and F tests, or of two instances of the F-test, in rejecting the non-variation null hypothesis. However, the C-test is a non-reliable statistical procedure, the F-test is not robust, and the combination of tests with concurrent results is anything but a straightforward methodology. A priori Power Analysis calculations and post hoc analysis of Monte-Carlo simulations show excellent agreement for the Analysis of Variance test to detect microvariations, as well as the limitations…
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