DeepZipper II: Searching for Lensed Supernovae in Dark Energy Survey Data with Deep Learning
Robert Morgan, B. Nord, K. Bechtol, A. M\"oller, W. G. Hartley, S., Birrer, S. J. Gonz\'alez, M. Martinez, R. A. Gruendl, E. J. Buckley-Geer, A., J. Shajib, A. Carnero Rosell, C. Lidman, T. Collett, T. M. C. Abbott, M., Aguena, F. Andrade-Oliveira, J. Annis, D. Bacon, S. Bocquet

TL;DR
This paper introduces DeepZipper II, a deep learning method for detecting gravitationally lensed supernovae in Dark Energy Survey data, achieving high recall and identifying three candidates for further study.
Contribution
The paper presents a novel multi-branch deep learning architecture trained on simulations to efficiently identify lensed supernovae in large astronomical datasets.
Findings
Achieved 61.13% recall with 0.02% false positive rate on DES data.
Selected 2,245 candidates from over 3 million systems.
Identified three promising lensed supernova candidates for follow-up.
Abstract
Gravitationally lensed supernovae (LSNe) are important probes of cosmic expansion, but they remain rare and difficult to find. Current cosmic surveys likely contain and 5-10 LSNe in total while next-generation experiments are expected to contain several hundreds to a few thousands of these systems. We search for these systems in observed Dark Energy Survey (DES) 5-year SN fields -- 10 3-sq. deg. regions of sky imaged in the bands approximately every six nights over five years. To perform the search, we utilize the DeepZipper approach: a multi-branch deep learning architecture trained on image-level simulations of LSNe that simultaneously learns spatial and temporal relationships from time series of images. We find that our method obtains a LSN recall of 61.13% and a false positive rate of 0.02% on the DES SN field data. DeepZipper selected 2,245 candidates from a…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astronomy and Astrophysical Research · CCD and CMOS Imaging Sensors
