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Detecting a small Kuiper Belt object using archival data of HST's Fine Guidance Sensor

Zucker, Shay and Schlichting, Hilke E. and Ofek, Eran O. and Wenz, Mike and Sari, Re'em and Gal-Yam, Avishay and Livio, Mario and Nelan, Ed (2010) Detecting a small Kuiper Belt object using archival data of HST's Fine Guidance Sensor. In: High Time Resolution Astrophysics (HTRA) IV - The Era of Extremely Large Telescopes. Proceedings of Science. No.108. SISSA , Trieste, Italy, Art. No. 024. http://resolver.caltech.edu/CaltechAUTHORS:20180824-100033196

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Abstract

The Kuiper Belt is a remnant of the primordial Solar System. Measurements of its size distribution constrain its accretion and collisional history, and the importance of material strength of Kuiper Belt objects. Small, sub-kilometer-sized, Kuiper Belt objects elude direct detection, but the signature of their occultations of background stars should be detectable. Such an occultation event lasts typically a fraction of a second, thus making it a classical high time-resolution observation. Here we report an analysis of archival data of HST’s Fine Guidance Sensors (FGS), that reveals an occultation by such a small object. The detection introduces the FGS as a valuable HTRA instrument. We discuss the statistical aspects regarding the validation of the detection claim, and its physical implications.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.22323/1.108.0024DOIArticle
ORCID:
AuthorORCID
Ofek, Eran O.0000-0002-6786-8774
Gal-Yam, Avishay0000-0002-3653-5598
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Record Number:CaltechAUTHORS:20180824-100033196
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180824-100033196
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:89135
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:28 Aug 2018 14:58
Last Modified:28 Aug 2018 14:58

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