Transits against Fainter Stars: The Power of Image Deconvolution

TL;DR

This paper demonstrates that image deconvolution and high-resolution imaging significantly improve the detection of transiting planets around faint stars, addressing blending issues in deep stellar surveys.

Contribution

It introduces a powerful mitigation strategy using image deconvolution and high-resolution imaging to reduce blending confusion in deep transit surveys.

Findings

Effective blending mitigation with image deconvolution.

Successful application to Lupus-TR-3 and IR imaging.

Implications for CoRoT and KEPLER missions.

Abstract

Compared to bright star searches, surveys for transiting planets against fainter (V=12-18) stars have the advantage of much higher sky densities of dwarf star primaries, which afford easier detection of small transiting bodies. Furthermore, deep searches are capable of probing a wider range of stellar environments. On the other hand, for a given spatial resolution and transit depth, deep searches are more prone to confusion from blended eclipsing binaries. We present a powerful mitigation strategy for the blending problem that includes the use of image deconvolution and high resolution imaging. The techniques are illustrated with Lupus-TR-3 and very recent IR imaging with PANIC on Magellan. The results are likely to have implications for the CoRoT and KEPLER missions designed to detect transiting planets of terrestrial size.