KilonovaNet: Surrogate Models of Kilonova Spectra with Conditional Variational Autoencoders
arXiv:2204.00285 · doi:10.1093/mnras/stac2342
Abstract
Detailed radiative transfer simulations of kilonova spectra play an essential role in multimessenger astrophysics. Using the simulation results in parameter inference studies requires building a surrogate model from the simulation outputs to use in algorithms requiring sampling. In this work, we present KilonovaNet, an implementation of conditional variational autoencoders (cVAEs) for the construction of surrogate models of kilonova spectra. This method can be trained on spectra directly, removing overhead time of pre-processing spectra, and greatly speeds up parameter inference time. We build surrogate models of three state-of-the-art kilonova simulation data sets and present in-depth surrogate error evaluation methods, which can in general be applied to any surrogate construction method. By creating synthetic photometric observations from the spectral surrogate, we perform parameter inference for the observed light curve data of GW170817 and compare the results with previous analyses. Given the speed with which KilonovaNet performs during parameter inference, it will serve as a useful tool in future gravitational wave observing runs to quickly analyze potential kilonova candidates
References in corpus (63)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- LSST: from Science Drivers to Reference Design and Anticipated Data Products
- Advanced LIGO
- An Introduction to Variational Autoencoders
- dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
- Transient Events from Neutron Star Mergers
- A gravitational-wave standard siren measurement of the Hubble constant
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei
- Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
- Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger
- INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817
- The X-ray counterpart to the gravitational wave event GW 170817
- A kilonova as the electromagnetic counterpart to a gravitational-wave source
- Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
- Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger
- Using gravitational-wave standard sirens
- The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
- Observation of gravitational waves from two neutron star-black hole coalescences
- Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
- Swift and NuSTAR observations of GW170817: detection of a blue kilonova
- Opacities and Spectra of the r-process Ejecta from Neutron Star Mergers
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South
- GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
- KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector
- What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?
- Kilonovae
- The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
- Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts and Nucleosynthesis
- Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
- Early Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger
- AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817
- Systematic Opacity Calculations for Kilonovae
- Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations
- Impact of ejecta morphology and composition on the electromagnetic signatures of neutron star mergers
- Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs
- J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817
- POSSIS: predicting spectra, light curves and polarization for multi-dimensional models of supernovae and kilonovae
- Models of Kilonova/macronova emission from black hole-neutron star mergers
- Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts
- GROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR
- The First Hours of the GW170817 Kilonova and the Importance of Early Optical and Ultraviolet Observations for Constraining Emission Models
- Searching for Electromagnetic Counterparts to Gravitational-wave Merger Events with the Prototype Gravitational-wave Optical Transient Observer (GOTO-4)
- Axisymmetric Radiative Transfer Models of Kilonovae
- Optical follow-up of the neutron star-black hole mergers S200105ae and S200115j
- GRANDMA Observations of Advanced LIGO's and Advanced Virgo's Third Observational Campaign
- Simulations of early kilonova emission from neutron star mergers
- Polarisation spectral synthesis for Type Ia supernova explosion models
- Statistical Gravitational Waveform Models: What to Simulate Next?
- A low-mass binary neutron star: long-term ejecta evolution and kilonovae with weak blue emission
- Kilonova Detectability with Wide-Field Instruments
- GROWTH on S190426c. II. Real-Time Search for a Counterpart to the Probable Neutron Star-Black Hole Merger using an Automated Difference Imaging Pipeline for DECam
- Measuring the Hubble Constant with a sample of kilonovae
- Towards rapid transient identification and characterization of kilonovae
- Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run
- Addressing Variance Shrinkage in Variational Autoencoders using Quantile Regression
- Using Neural Networks to Perform Rapid High-Dimensional Kilonova Parameter Inference
- A Broad Grid of 2D Kilonova Emission Models
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- Redback: A Bayesian inference software package for electromagnetic transients
- Spectroscopic r-Process Abundance Retrieval for Kilonovae I: The Inferred Abundance Pattern of Early Emission from GW170817
- KilonovAE: Exploring Kilonova Spectral Features with Autoencoders
- Kilonova Light-Curve Interpolation with Neural Networks
- Interpolated kilonova spectra models: necessity for a phenomenological, blue component in the fitting of AT2017gfo spectra
- Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm