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The IPAC Image Subtraction and Discovery Pipeline for the Intermediate Palomar Transient FactoryWe describe the near real-time transient-source discovery engine for the intermediate Palomar Transient Factory (iPTF), currently in operations at the Infrared Processing and Analysis Center (IPAC), Caltech. We coin this system the IPAC/iPTF Discovery Engine (or IDE). We review the algorithms used for PSF-matching, image subtraction, detection, photometry, and machine-learned (ML) vetting of extracted transient candidates. We also review the performance of our ML classifier. For a limiting signal-to-noise ratio of 4 in relatively unconfused regions, bogus candidates from processing artifacts and imperfect image subtractions outnumber real transients by approximately equal to 10:1. This can be considerably higher for image data with inaccurate astrometric and/or PSF-matching solutions. Despite this occasionally high contamination rate, the ML classifier is able to identify real transients with an efficiency (or completeness) of approximately equal to 97% for a maximum tolerable false-positive rate of 1% when classifying raw candidates. All subtraction-image metrics, source features, ML probability-based real-bogus scores, contextual metadata from other surveys, and possible associations with known Solar System objects are stored in a relational database for retrieval by the various science working groups. We review our efforts in mitigating false-positives and our experience in optimizing the overall system in response to the multitude of science projects underway with iPTF.
Document ID
20170006207
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Masci, Frank J.
(California Inst. of Tech. Pasadena, CA, United States)
Laher, Russ R.
(California Inst. of Tech. Pasadena, CA, United States)
Rebbapragada, Umaa D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Doran, Gary B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Miller, Adam A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Bellm, Eric
(California Inst. of Tech. Pasadena, CA, United States)
Kasliwal, Mansi
(California Inst. of Tech. Pasadena, CA, United States)
Ofek, Eran O.
(Weizmann Inst. of Science Rehovot, Israel)
Surace, Jason
(California Inst. of Tech. Pasadena, CA, United States)
Shupe, David L.
(California Inst. of Tech. Pasadena, CA, United States)
Grillmair, Carl J.
(California Inst. of Tech. Pasadena, CA, United States)
Jackson, Ed
(California Inst. of Tech. Pasadena, CA, United States)
Barlow, Tom
(California Inst. of Tech. Pasadena, CA, United States)
Yan, Lin
(California Inst. of Tech. Pasadena, CA, United States)
Cao, Yi
(California Inst. of Tech. Pasadena, CA, United States)
Cenko, S. Bradley
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Storrie-Lombardi, Lisa J.
(California Inst. of Tech. Pasadena, CA, United States)
Helou, George
(California Inst. of Tech. Pasadena, CA, United States)
Prince, Thomas A.
(California Inst. of Tech. Pasadena, CA, United States)
Kulkarni, Shrinivas R.
(California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
July 7, 2017
Publication Date
December 8, 2016
Publication Information
Publication: The Astronomical Society of the Pacific
Publisher: The Astronomical Society of the Pacific
Volume: 129
Issue: 971
ISSN: 0004-6280
e-ISSN: 1538-3873
Subject Category
Numerical Analysis
Astrophysics
Report/Patent Number
GSFC-E-DAA-TN44010
Funding Number(s)
CONTRACT_GRANT: NAS5-26555
Distribution Limits
Public
Copyright
Other
Keywords
methods: analytical – methods: data analysis – methods: statistical – tech

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