Faint moving object detection, and the Low Signal-to-Noise recovery of Main Belt comet P/2008 R1 Garradd

J. Kleyna, K. J. Meech and O. R. Hainaut
Publications of the Astronomical Society of the Pacific
Vol. 124, No. 920 (October 2012), pp. 1083-1089
DOI: 10.1086/668253
Stable URL: http://www.jstor.org/stable/10.1086/668253
Page Count: 7
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Faint moving object detection, and the Low Signal-to-Noise recovery of Main Belt comet P/2008 R1 Garradd
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Abstract

ABSTRACT.We describe the recovery of faint main belt comet P/2008 R1 Garradd using several telescopes, culminating in a successful low signal-to-noise ratio (S/N) recovery with the Gemini North telescope with GMOS. This recovery was a time-critical effort for a mission proposal, and had to be performed in a crowded field. We describe techniques and software tools for eliminating systematic noise artifacts and stellar residuals, bringing the final detection image statistics close to the Gaussian ideal for a median image stack, and achieving a detection sensitivity close to this theoretical optimum. The magnitude of Rc = 26.1 ± 0.2Rc=26.1±0.2 with an assumed geometric albedo of 0.05 corresponds to a radius of 0.3 km. For ice to have survived in this object over the age of the solar system implies that the object is a more recent collisional fragment. We discuss the implications of the unexpectedly faint magnitude and nuclear size of P/2008 R1 on the survival of ice inside very small bodies.

Notes and References

This item contains 16 references.

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