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ANTARES: A gateway to ZTF and LSST alerts

Published online by Cambridge University Press:  09 October 2020

Chien-Hsiu Lee
Affiliation:
NSF’s National Optical-Infrared Astronomy Research Laboratory, AZ 85719, USA emails: [email protected], [email protected], [email protected], [email protected], [email protected]
Monika Soraisam
Affiliation:
National Center for Supercomputing Applications, IL 61801, USA email: [email protected] University of Illinois at Urbana-Champaign, IL 61801, USA email: [email protected]
Gautham Narayan
Affiliation:
University of Illinois at Urbana-Champaign, IL 61801, USA email: [email protected]
Thomas Matheson
Affiliation:
NSF’s National Optical-Infrared Astronomy Research Laboratory, AZ 85719, USA emails: [email protected], [email protected], [email protected], [email protected], [email protected]
Abhijit Saha
Affiliation:
NSF’s National Optical-Infrared Astronomy Research Laboratory, AZ 85719, USA emails: [email protected], [email protected], [email protected], [email protected], [email protected]
Carl Stubens
Affiliation:
NSF’s National Optical-Infrared Astronomy Research Laboratory, AZ 85719, USA emails: [email protected], [email protected], [email protected], [email protected], [email protected]
Nicholas Wolf
Affiliation:
NSF’s National Optical-Infrared Astronomy Research Laboratory, AZ 85719, USA emails: [email protected], [email protected], [email protected], [email protected], [email protected]
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Abstract

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Studies of white dwarfs have greatly benefited from time-domain surveys and subsequent follow-up observations. However, with the avalanche of alerts delivered by ZTF and LSST and the limited resources for follow-up, we will need brokers to select intriguing alerts that warrant follow-up in a timely manner. At the University of Arizona and NSF’s OIR Lab, we are developing the Arizona-NOAO Temporal Analysis and Response to Events System, to hunt for the rarest of the rare events in the time-domain. In this work, we provide an overview of the ANTARES system, how we use ZTF as a training set, and the way forwards to LSST.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

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