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Matthew J Holman

Publications and source records attributed to Matthew J Holman.

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heliostack: A Novel Approach to Minor Planet Discovery

The study of faint solar system objects is a promising avenue for understanding the origin and evolution of planetary systems. However, such objects are difficult to detect in conventional surveys. Here we introduce heliostack, an algorithm for nonlinear shift-and-stack searches for solar system objects, which enables us to combine images taken over longer time spans than was previously possible. Applying this algorithm to a number of existing archival and forthcoming surveys will allow us to maximize their potential for discovering faint solar system objects. In this work, we apply heliostack to archival Hubble Space Telescope (HST) data, completing an exhaustive search for Cold Classical Kuiper Belt Objects in a set of HST images taken over a 15-day time span in 2003. We successfully recover both of the known sub-threshold objects in the data, and add two new discoveries. These two new objects are the first to ever be discovered in stacks of images taken over a time span longer than about one day.

astro-ph.EP

A Novel Orbit Parameterization in Spherical Coordinates

We present a novel orbit parameterization in spherical coordinates. This parameterization enables the mixing of varying and invariant orbital parameters, and clarifies the physics of the orbit. It also simplifies the process of placing synthetic populations at exactly specified locations on the sky, which is particularly useful for survey design and simulation studies.

astro-ph.EP

A TESS Search for Distant Solar System Objects: Yield Estimates

As the NASA Transiting Exoplanet Survey Satellite (TESS) fulfills its primary mission, it is executing an unprecedented survey of almost the entire sky: TESS's approved extended mission will likely extend sky coverage to ~94%, including ~60% of the ecliptic. In an accompanying note we demonstrated that `digital tracking' techniques can be used to efficiently `shift-and-stack' TESS full frame images (FFIs) and showed that combining ~1,300 exposures from a TESS sector gives a 50% detection threshold of $I_C\sim 22.0\pm0.5$, raising the possibility that TESS could discover the hypothesized Planet Nine. In this note, we estimate the yield for such a survey and demonstrate that this technique has the potential to discover hundreds of Kuiper Belt Objects, Scattered Disk Objects and Centaurs in TESS FFI data.

astro-ph.EP