The LCO Outbursting Objects Key Project: Overview and Year 1 Status
Tim Lister, Michael S. P. Kelley, Carrie E. Holt, Henry H. Hsieh,, Michele T. Bannister, Aayushi A. Verma, Matthew M. Dobson, Matthew M. Knight,, Youssef Moulane, Megan E. Schwamb, Dennis Bodewits, James Bauer, Joseph, Chatelain, Estela Fern\'andez-Valenzuela, Daniel Gardener

TL;DR
The LOOK Project systematically monitors small bodies for outbursts using LCO telescopes, providing valuable data on outburst characteristics, frequency, and underlying processes, and serves as a testbed for future large-scale surveys like LSST.
Contribution
It introduces a coordinated observational program for outburst detection in small Solar System bodies and reports initial findings, demonstrating its effectiveness and potential for future survey integration.
Findings
Detected activity and outbursts on comet C/2014 UN271
Discovered and followed up outbursts on multiple comets
Identified outburst activity in P/2020 X1 (ATLAS) at discovery
Abstract
The LCO Outbursting Objects Key (LOOK) Project uses the telescopes of the Las Cumbres Observatory (LCO) Network to: (1) to systematically monitor a sample of Dynamically New Comets over the whole sky, and (2) use alerts from existing sky surveys to rapidly respond to and characterize detected outburst activity in all small bodies. The data gathered on outbursts helps to characterize each outburst's evolution with time, assess the frequency and magnitude distribution of outbursts in general, and contributes to the understanding of outburst processes and volatile distribution in the Solar System. The LOOK Project exploits the synergy between current and future wide-field surveys such as ZTF, PanSTARRS, and LSST as well as rapid-response telescope networks such as LCO, and serves as an excellent testbed for what will be needed the much larger number of objects coming from Rubin…
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Taxonomy
TopicsAstro and Planetary Science · Atmospheric Ozone and Climate · Isotope Analysis in Ecology
