TRANSLIENT: Detecting Transients Resulting from Point Source Motion or Astrometric Errors
O. Springer, E. O. Ofek, B. Zackay, R. Konno, A. Sharon, G. Nir, A., Rubin, A. Haddad, J. Friedman, L. Schein Lubomirsky, I. Aizenberg, A., Krassilchtchikov, A. Gal-Yam

TL;DR
The paper introduces TRANSLIENT, a novel method extending image subtraction techniques to detect and distinguish moving sources from stationary ones, improving false alarm reduction in transient astrophysical observations.
Contribution
It presents a new hypothesis testing-based algorithm, TRANSLIENT, for detecting point source motion, which is numerically stable, fast, and optimal in small translation limits.
Findings
TRANSLIENT outperforms proper image subtraction in ROC curves.
It effectively distinguishes between motion and variability.
The method is validated on simulated and real telescope data.
Abstract
Detection of moving sources over complicated background is important for several reasons. First is measuring the astrophysical motion of the source. Second is that such motion resulting from atmospheric scintillation, color refraction, or astrophysical reasons is a major source of false alarms for image subtraction methods. We extend the Zackay, Ofek, and Gal-Yam image subtraction formalism to deal with moving sources. The new method, named translient (translational transient) detector, applies hypothesis testing between the hypothesis that the source is stationary and that the source is moving. It can be used to detect source motion or to distinguish between stellar variability and motion. For moving source detection, we show the superiority of translient over the proper image subtraction, using the improvement in the receiver-operating characteristic curve. We show that in the small…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
