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A faint type of supernova from a white dwarf with a helium-rich companion
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The Supernova Legacy Survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints
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PELICAN: deeP architecturE for the LIght Curve ANalysis
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The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics
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The Sloan Digital sky Survey-Ii Supernova Survey: Technical Summary
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The Sloan Digital sky Survey-Ii Supernova Survey: Search Algorithm and Follow-Up Observations
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Optical Spectra of 73 Stripped-Envelope Core-Collapse Supernovae
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PHOTOMETRIC TYPE Ia SUPERNOVA CANDIDATES FROM THE THREE-YEAR SDSS-II SN SURVEY DATA
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TESTING MODELS OF INTRINSIC BRIGHTNESS VARIATIONS IN TYPE Ia SUPERNOVAE AND THEIR IMPACT ON MEASURING COSMOLOGICAL PARAMETERS
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Extending Supernova Spectral Templates for Next-generation Space Telescope Observations
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Models and Simulations for the Photometric LSST Astronomical Time Series Classification Challenge (PLAsTiCC)
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First cosmology results using type Ia supernovae from the Dark Energy Survey: the effect of host galaxy properties on supernova luminosity
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SN2017jgh: a high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope
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A simple and robust method for automated photometric classification of supernovae using neural networks
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Rapidly evolving transients in the Dark Energy Survey
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SuperNNova: an open-source framework for Bayesian, neural network-based supernova classification
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Constraining Dark Energy with Type Ia Supernovae and Large-Scale Structure
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SCONE: Supernova Classification with a Convolutional Neural Network
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Alert Classification for the ALeRCE Broker System: The Real-time Stamp Classifier
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ParSNIP: Generative Models of Transient Light Curves with Physics-enabled Deep Learning
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The Magnetar Model for Type I Superluminous Supernovae. I. Bayesian Analysis of the Full Multicolor Light-curve Sample with MOSFiT
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LSST: From Science Drivers to Reference Design and Anticipated Data Products
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Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
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SuperRAENN: A Semisupervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium-Deep Survey Supernovae
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