Redback: A Bayesian inference software package for electromagnetic transients
arXiv:2308.12806 · doi:10.1093/mnras/stae1238
Abstract
Fulfilling the rich promise of rapid advances in time-domain astronomy is only possible through confronting our observations with physical models and extracting the parameters that best describe what we see. Here, we introduce {\sc Redback}; a Bayesian inference software package for electromagnetic transients. {\sc Redback} provides an object-orientated {\sc python} interface to over 12 different samplers and over 100 different models for kilonovae, supernovae, gamma-ray burst afterglows, tidal disruption events, engine-driven transients among other explosive transients. The models range in complexity from simple analytical and semi-analytical models to surrogates built upon numerical simulations accelerated via machine learning. {\sc Redback} also provides a simple interface for downloading and processing data from various catalogs such as \textit{Swift} and Fink. The software can also serve as an engine to simulate transients for telescopes such as the Zwicky Transient Facility and Vera Rubin with realistic cadences, limiting magnitudes, and sky-coverage or a hypothetical user-constructed survey or a generic transient for target-of-opportunity observations with different telescopes. As a demonstration of its capabilities, we show how {\sc Redback} can be used to jointly fit the spectrum and photometry of a kilonova, enabling a more powerful, holistic probe into the properties of a transient. We also showcase general examples of how {\sc Redback} can be used as a tool to simulate transients for realistic surveys, fit models to real, simulated, or private data, multi-messenger inference with gravitational waves, and serve as an end-to-end software toolkit for parameter estimation and interpreting the nature of electromagnetic transients.
Published in MNRAS. 25 pages 11 figures. Redback is available on GitHub at https://github.com/nikhil-sarin/redback
References in corpus (48)
- Array Programming with NumPy
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- Multi-messenger Observations of a Binary Neutron Star Merger
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- 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
- A kilonova as the electromagnetic counterpart to a gravitational-wave source
- Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
- The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications
- GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
- A Radio Counterpart to a Neutron Star Merger
- Kilonovae
- Rapidly-Evolving and Luminous Transients from Pan-STARRS1
- The magnetar model for Type I superluminous supernovae I: Bayesian analysis of the full multicolour light curve sample with MOSFiT
- Data analysis recipes: Fitting a model to data
- The optical afterglow of GW170817 at one year post-merger
- Superluminous Supernovae Powered by Magnetars: Late-time Light Curves and Hard Emission Leakage
- Modelling the spectra of the kilonova AT2017gfo -- I: The photospheric epochs
- Theoretical Models of Optical Transients. I. A Broad Exploration of the Duration-Luminosity Phase Space
- Evidence for an intermediate-mass black hole from a gravitationally lensed gamma-ray burst
- The braking index of millisecond magnetars
- Simulations of early kilonova emission from neutron star mergers
- Cooling Envelope Model for Tidal Disruption Events
- Observable Features of GW170817 Kilonova Afterglow
- Kilohertz quasiperiodic oscillations in short gamma-ray bursts
- Signatures of R-process Enrichment in Supernovae from Collapsars
- The Effect of Jet-Ejecta Interaction on the Viewing Angle Dependence of Kilonova Light Curves
- GRB 170817A as a Refreshed Shock Afterglow viewed off-axis
- A Generalized Semi-Analytic Model for Magnetar-Driven Supernovae
- Searching for quasi-periodic oscillations in astrophysical transients using Gaussian processes
- Extended Self-similar Solution for Circumstellar Material-Supernova Ejecta Interaction
- The Dark Energy Survey Supernova Program: Cosmological Analysis and Systematic Uncertainties
- KilonovaNet: Surrogate Models of Kilonova Spectra with Conditional Variational Autoencoders
- Tidal Disruption Events through the Lens of the Cooling Envelope Model
- Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
- The Landscape of Thermal Transients from Supernova Interacting with a Circumstellar Medium
- Magnetar Flare-Driven Bumpy Declining Light Curves in Hydrogen-poor Superluminous Supernovae
- Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
- From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter
- Prospects of Gravitational Wave Follow-up Through a Wide-field Ultra-violet Satellite: a Dorado Case Study
- 1100 days in the life of the supernova 2018ibb -- The best pair-instability supernova candidate, to date
- Modelling of Long-Term Afterglow Counterparts to Gravitational Wave Events: The Full View of GRB 170817A
- The Multiwavelength Picture of GRB 221009A's Afterglow
- CDF-S XT1: The off-axis afterglow of a neutron star merger at
- Shocks Power Tidal Disruption Events
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- Cautionary tales on heating-rate prescriptions in kilonovae
- Multi-Peaked Non-Thermal Light Curves from Magnetar-Powered Gamma-Ray Bursts
- Probing Interacting Dark Sector with the next generation of gravitational-wave detectors
- Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc
- The origin of the coherent radio flash potentially associated with GRB 201006A
- Surrogate models for lightcurves and photosphere properties of Type II supernovae
- Data-driven approach for modeling the temporal and spectral evolution of kilonova systematic uncertainties
- Unveiling the nature of the Einstein Probe transient EP 241021a
- MUSE IFU observations of galaxies hosting Tidal Disruption Events
- Candidate strongly lensed type Ia supernovae in the Zwicky Transient Facility archive
- The Case for Space: Estimating Precise Time Delays from Ground- and Space-Based Observations of Lensed Supernovae with Glimpse
- EP241217a: a likely Type II GRB with an achromatic bump at z = 4.59
- An Archival Optical Counterpart Search for Extragalactic Fast X-Ray Transients Discovered by Einstein Probe
- The New Status Qvo? SN 2021qvo is Another 2003fg-like Type Ia Supernova with a Rising Light-Curve Bump
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- Kilonova and progenitor properties of merger-driven gamma-ray bursts
- GOTO identification and broadband modelling of the counterpart to the SVOM GRB 250818B