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Machine Learning for the Zwicky Transient Facility

Authors :
Mahabal, Ashish
Rebbapragada, Umaa
Walters, Richard
Masci, Frank J.
Blagorodnova, Nadejda
Roestel, Jan van
Ye, Quan-Zhi
Biswas, Rahul
Burdge, Kevin
Chang, Chan-Kao
Duev, Dmitry A.
Golkhou, V. Zach
Miller, Adam A.
Nordin, Jakob
Ward, Charlotte
Adams, Scott
Bellm, Eric C.
Branton, Doug
Bue, Brian
Cannella, Chris
Connolly, Andrew
Dekany, Richard
Feindt, Ulrich
Hung, Tiara
Fortson, Lucy
Frederick, Sara
Fremling, C.
Gezari, Suvi
Graham, Matthew
Groom, Steven
Kasliwal, Mansi M.
Kulkarni, Shrinivas
Kupfer, Thomas
Lin, Hsing Wen
Lintott, Chris
Lunnan, Ragnhild
Parejko, John
Prince, Thomas A.
Riddle, Reed
Rusholme, Ben
Saunders, Nicholas
Sedaghat, Nima
Shupe, David L.
Singer, Leo P.
Soumagnac, Maayane T.
Szkody, Paula
Tachibana, Yutaro
Tirumala, Kushal
Velzen, Sjoert van
Wright, Darryl
Mahabal, Ashish
Rebbapragada, Umaa
Walters, Richard
Masci, Frank J.
Blagorodnova, Nadejda
Roestel, Jan van
Ye, Quan-Zhi
Biswas, Rahul
Burdge, Kevin
Chang, Chan-Kao
Duev, Dmitry A.
Golkhou, V. Zach
Miller, Adam A.
Nordin, Jakob
Ward, Charlotte
Adams, Scott
Bellm, Eric C.
Branton, Doug
Bue, Brian
Cannella, Chris
Connolly, Andrew
Dekany, Richard
Feindt, Ulrich
Hung, Tiara
Fortson, Lucy
Frederick, Sara
Fremling, C.
Gezari, Suvi
Graham, Matthew
Groom, Steven
Kasliwal, Mansi M.
Kulkarni, Shrinivas
Kupfer, Thomas
Lin, Hsing Wen
Lintott, Chris
Lunnan, Ragnhild
Parejko, John
Prince, Thomas A.
Riddle, Reed
Rusholme, Ben
Saunders, Nicholas
Sedaghat, Nima
Shupe, David L.
Singer, Leo P.
Soumagnac, Maayane T.
Szkody, Paula
Tachibana, Yutaro
Tirumala, Kushal
Velzen, Sjoert van
Wright, Darryl
Publication Year :
2019

Abstract

The Zwicky Transient Facility is a large optical survey in multiple filters producing hundreds of thousands of transient alerts per night. We describe here various machine learning (ML) implementations and plans to make the maximal use of the large data set by taking advantage of the temporal nature of the data, and further combining it with other data sets. We start with the initial steps of separating bogus candidates from real ones, separating stars and galaxies, and go on to the classification of real objects into various classes. Besides the usual methods (e.g., based on features extracted from light curves) we also describe early plans for alternate methods including the use of domain adaptation, and deep learning. In a similar fashion we describe efforts to detect fast moving asteroids. We also describe the use of the Zooniverse platform for helping with classifications through the creation of training samples, and active learning. Finally we mention the synergistic aspects of ZTF and LSST from the ML perspective.<br />National Science Foundationhttps://doi.org/10.13039/100000001<br />Peer Reviewed

Details

Database :
OAIster
Notes :
application/pdf, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1408325658
Document Type :
Electronic Resource