Supernova Photometric Classification Pipelines Trained on Spectroscopically Classified Supernovae from the Pan-STARRS1 Medium-Deep Survey. (arXiv:1905.07422v1 [astro-ph.HE])

Supernova Photometric Classification Pipelines Trained on Spectroscopically Classified Supernovae from the Pan-STARRS1 Medium-Deep Survey. (arXiv:1905.07422v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Villar_V/0/1/0/all/0/1">V. A. Villar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Berger_E/0/1/0/all/0/1">E. Berger</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Miller_G/0/1/0/all/0/1">G. Miller</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chornock_R/0/1/0/all/0/1">R. Chornock</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rest_A/0/1/0/all/0/1">A. Rest</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jones_D/0/1/0/all/0/1">D. O. Jones</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Drout_M/0/1/0/all/0/1">M. R. Drout</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Foley_R/0/1/0/all/0/1">R. J. Foley</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kirshner_R/0/1/0/all/0/1">R. Kirshner</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lunnan_R/0/1/0/all/0/1">R. Lunnan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Magnier_E/0/1/0/all/0/1">E. Magnier</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Milisavljevic_D/0/1/0/all/0/1">D. Milisavljevic</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sanders_N/0/1/0/all/0/1">N. Sanders</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Scolnic_D/0/1/0/all/0/1">D. Scolnic</a>

Photometric classification of supernovae (SNe) is imperative as recent and
upcoming optical time-domain surveys, such as the Large Synoptic Survey
Telescope (LSST), overwhelm the available resources for spectrosopic follow-up.
Here we develop a range of light curve classification pipelines, trained on 518
spectroscopically-classified SNe from the Pan-STARRS1 Medium-Deep Survey
(PS1-MDS): 357 Type Ia, 93 Type II, 25 Type IIn, 21 Type Ibc, and 17 Type I
SLSNe. We present a new parametric analytical model that can accommodate a
broad range of SN light curve morphologies, including those with a plateau, and
fit this model to data in four PS1 filters (griz). We test a number of feature
extraction methods, data augmentation strategies, and machine learning
algorithms to predict the class of each SN. Our best pipelines result in 90%
average accuracy, 70% average purity, and 80% average completeness for all SN
classes, with the highest success rates for Type Ia SNe and SLSNe and the
lowest for Type Ibc SNe. Despite the greater complexity of our classification
scheme, the purity of our Type Ia SN classification, 95%, is on par with
methods developed specifically for Type Ia versus non-Type Ia binary
classification. As the first of its kind, this study serves as a guide to
developing and training classification algorithms for a wide range of SN types
with a purely empirical training set, particularly one that is similar in its
characteristics to the expected LSST main survey strategy. Future work will
implement this classification pipeline on ~3000 PS1/MDS light curves that lack
spectroscopic classification.

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