Kilonova Luminosity Function Constraints based on Zwicky Transient Facility Searches for 13 Neutron Star Mergers
arXiv:2006.11306 · doi:10.3847/1538-4357/abc335
Abstract
We present a systematic search for optical counterparts to 13 gravitational wave (GW) triggers involving at least one neutron star during LIGO/Virgo's third observing run. We searched binary neutron star (BNS) and neutron star black hole (NSBH) merger localizations with the Zwicky Transient Facility (ZTF) and undertook follow-up with the Global Relay of Observatories Watching Transients Happen (GROWTH) collaboration. The GW triggers had a median localization of 4480 deg^2, median distance of 267 Mpc and false alarm rates ranging from 1.5 to 1e-25 per yr. The ZTF coverage had a median enclosed probability of 39%, median depth of 20.8mag, and median response time of 1.5 hr. The O3 follow-up by the GROWTH team comprised 340 UVOIR photometric points, 64 OIR spectra, and 3 radio. We find no promising kilonova (radioactivity-powered counterpart) and we convert the upper limits to constrain the underlying kilonova luminosity function. Assuming that all kilonovae are at least as luminous as GW170817 at discovery (-16.1mag), we calculate our joint probability of detecting zero kilonovae is only 4.2%. If we assume that all kilonovae are brighter than -16.6mag (extrapolated peak magnitude of GW170817) and fade at 1 mag/day (similar to GW170817), the joint probability of zero detections is 7%. If we separate the NSBH and BNS populations, the joint probability of zero detections, assuming all kilonovae are brighter than -16.6mag, is 9.7% for NSBH and 7.9% for BNS mergers. Moreover, <57% (<89%) of putative kilonovae could be brighter than -16.6mag assuming flat (fading) evolution, at 90% confidence. If we further account for the online terrestrial probability for each GW trigger, we find that <68% of putative kilonovae could be brighter than -16.6mag. Comparing to model grids, we find that some kilonovae must have Mej < 0.03 Msun or Xlan>1e-4 or phi>30deg to be consistent with our limits. (Abridged)
Submitted to ApJ
References in corpus (101)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
- Multi-messenger Observations of a Binary Neutron Star Merger
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- The Swift Ultra-Violet/Optical Telescope
- The Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
- The Zwicky Transient Facility: Data Processing, Products, and Archive
- ATLAS: A High-Cadence All-Sky Survey System
- Las Cumbres Observatory Global Telescope Network
- 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 Palomar Transient Factory: System Overview, Performance and First Results
- A Method of Correcting Near-Infrared Spectra for Telluric Absorption
- 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
- Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
- A kilonova as the electromagnetic counterpart to a gravitational-wave source
- The X-ray counterpart to the gravitational wave event GW 170817
- The Zwicky Transient Facility: Science Objectives
- The Eccentric Kozai-Lidov Effect and Its Applications
- 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
- 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
- A Radio Counterpart to a Neutron Star Merger
- Determining the Type, Redshift, and Age of a Supernova Spectrum
- The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
- Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. V. Rising X-ray Emission from an Off-Axis Jet
- Rapid Bayesian position reconstruction for gravitational-wave transients
- Progenitors of gravitational wave mergers: Binary evolution with the stellar grid-based code ComBinE
- Mergers of neutron star black hole binaries with small mass ratios: nucleosynthesis, gamma-ray bursts and electromagnetic transients
- The Sloan Digital Sky Survey Data Release 7 Spectroscopic M Dwarf Catalog I: Data
- MASTER optical detection of the first LIGO/Virgo neutron stars merging GW170817
- The Automated Palomar 60-Inch Telescope
- Proper image subtraction - optimal transient detection, photometry and hypothesis testing
- Black Hole-Neutron Star Mergers: Disk Mass Predictions
- The SED Machine: a robotic spectrograph for fast transient classification
- Fully-Automated Reduction of Longslit Spectroscopy with the Low Resolution Imaging Spectrometer at Keck Observatory
- The WISE AGN Catalog
- Remnant baryon mass outside of the black hole after a neutron star-black hole merger
- A Deep Chandra X-ray Study of Neutron Star Coalescence GW170817
- Identifying Elusive Electromagnetic Counterparts to Gravitational Wave Mergers: an end-to-end simulation
- 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
- PTF12os and iPTF13bvn. Two stripped-envelope supernovae from low-mass progenitors in NGC 5806
- POSSIS: predicting spectra, light curves and polarization for multi-dimensional models of supernovae and kilonovae
- High-resolution magnetohydrodynamics simulation of black hole-neutron star merger: Mass ejection and short gamma-ray burst
- Constraints on the ejecta of the GW170817 neutron-star merger from its electromagnetic emission
- Models of Kilonova/macronova emission from black hole-neutron star mergers
- Real-bogus classification for the Zwicky Transient Facility using deep learning
- The GROWTH Marshal: A Dynamic Science Portal for Time-Domain Astronomy
- A Strong Jet Signature in the Late-Time Lightcurve of GW170817
- The electromagnetic counterparts of compact binary mergers
- A Fully Automated Integral Field Spectrograph Pipeline for the SEDMachine: pysedm
- The Zwicky Transient Facility Alert Distribution System
- Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration
- Machine Learning for the Zwicky Transient Facility
- 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
- GRB170817A associated with GW170817: multifrequency observations and modeling of prompt gamma-ray emission
- The First Hours of the GW170817 Kilonova and the Importance of Early Optical and Ultraviolet Observations for Constraining Emission Models
- Progenitor models of the electromagnetic transient associated with the short GRB 130603B
- Evidence for Cocoon Emission from the Early Light Curve of SSS17a
- A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
- Spitzer Mid-Infrared Detections of Neutron Star Merger GW170817 Suggests Synthesis of the Heaviest Elements
- GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-Infrared Counterpart to a Neutron Star-Black Hole Merger
- Searching for Electromagnetic Counterparts to Gravitational-wave Merger Events with the Prototype Gravitational-wave Optical Transient Observer (GOTO-4)
- ZTF Early Observations of Type Ia Supernovae I: Properties of the 2018 Sample
- A Morphological Classification Model to Identify Unresolved PanSTARRS1 Sources: Application in the ZTF Real-Time Pipeline
- Optical follow-up of the neutron star-black hole mergers S200105ae and S200115j
- Transient processing and analysis using : Alert Management, Photometry and Evaluation of Lightcurves
- The IPAC Image Subtraction and Discovery Pipeline for the intermediate Palomar Transient Factory
- The Fate of Binaries in the Galactic Center: The Mundane and the Exotic
- Palomar Gattini-IR: Survey overview, data processing system, on-sky performance and first results
- Optimizing searches for electromagnetic counterparts of gravitational wave triggers
- The landscape of disk outflows from black hole - neutron star mergers
- Census of the Local Universe (CLU) Narrow-Band Survey I: Galaxy Catalogs from Preliminary Fields
- On Discovering Electromagnetic Emission from Neutron Star Mergers: The Early Years of Two Gravitational Wave Detectors
- Searches After Gravitational-waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo's Third Observing Run
- Quasar and galaxy classification in Gaia Data Release 2
- An ASKAP search for a radio counterpart to the first high-significance neutron star-black hole merger LIGO/Virgo S190814bv
- The Needle in the 100 deg2 Haystack: Uncovering Afterglows of Fermi GRBs with the Palomar Transient Factory
- DASH: Deep Learning for the Automated Spectral Classification of Supernovae and their Hosts
- iPTF Search for an Optical Counterpart to Gravitational Wave Trigger GW150914
- Intermediate Palomar Transient Factory: Realtime Image Subtraction Pipeline
- catsHTM - A tool for fast accessing and cross-matching large astronomical catalogs
- 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
- A Machine Learning Based Source Property Inference for Compact Binary Mergers
- STROOPWAFEL: Simulating rare outcomes from astrophysical populations, with application to gravitational-wave sources
- : Estimating Transient Discovery Rates for the Zwicky Transient Facility
- GROWTH on S190510g: DECam Observation Planning and Follow-Up of a Distant Binary Neutron Star Merger Candidate
- 2900 square degree search for the optical counterpart of short gamma-ray burst GRB 180523B with the Zwicky Transient Facility
- The Kitt Peak Electron Multiplying CCD demonstrator
- Dynamic Scheduling: Target of Opportunity Observations of Gravitational Wave Events
Cited by in corpus (68)
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- Rates of Compact Object Coalescences
- Accurate precision Cosmology with redshift unknown gravitational wave sources
- First Multimessenger Observations of a Neutron Star Merger
- Data-driven expectations for electromagnetic counterpart searches based on LIGO/Virgo public alerts
- A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
- A data science platform to enable time-domain astronomy
- Fast-transient Searches in Real Time with ZTFReST: Identification of Three Optically-discovered Gamma-ray Burst Afterglows and New Constraints on the Kilonova Rate
- The Fast Flavor Instability in Hypermassive Neutron Star Disk Outflows
- Kilonova Detectability with Wide-Field Instruments
- Updated observing scenarios and multi-messenger implications for the International Gravitational-wave Network's O4 and O5
- Kilonova Emission From Black Hole-Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches
- Target of Opportunity Observations of Gravitational Wave Events with Vera C. Rubin Observatory
- Continued radio observations of GW170817 3.5 years post-merger
- No Detectable Kilonova Counterpart is Expected for O3 Neutron Star-Black Hole Candidates
- Long-duration Gamma-ray Burst and Associated Kilonova Emission from Fast-spinning Black Hole--Neutron Star Mergers
- Cosmological Fast Optical Transients with the Zwicky Transient Facility: A Search for Dirty Fireballs
- Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
- Detectability of kilonovae in optical surveys: - examination of the LVC O3 run follow-up
- The BlackGEM telescope array I: Overview
- Population Properties of Gravitational-Wave Neutron Star--Black Hole Mergers
- A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources
- An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
- Swift/UVOT follow-up of Gravitational Wave Alerts in the O3 era
- Optimizing Cadences with Realistic Light Curve Filtering for Serendipitous Kilonova Discovery with Vera Rubin Observatory
- Optimizing Serendipitous Detections of Kilonovae: Cadence and Filter Selection
- Electromagnetic Signatures from the Tidal Tail of a Black Hole - Neutron Star Merger
- Neutrino follow-up with the Zwicky Transient Facility: Results from the first 24 campaigns
- Eighteen Years of Kilonova Discoveries with Swift
- A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run
- Prospects for kilonova signals in the gravitational-wave era
- Revealing nature of GRB 210205A, ZTF21aaeyldq (AT2021any), and follow-up observations with the 4K4K CCD Imager+3.6m DOT
- Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
- The potential role of binary neutron star merger afterglows in multimessenger cosmology
- Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
- GRANDMA Observations of ZTF/Fink Transients during Summer 2021
- Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
- Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
- Radio Afterglows from Compact Binary Coalescences: Prospects for Next-Generation Telescopes
- On the detection of the electromagnetic counterparts from lensed gravitational wave events by binary neutron star mergers
- Target of Opportunity Observations Detectability of Kilonovae with WFST
- The detection efficiency of type Ia supernovae from the Zwicky Transient Facility: Limits on the intrinsic rate of early flux excesses
- Enabling the discovery of fast transients: A kilonova science module for the Fink broker
- HEALPix Alchemy: Fast All-Sky Geometry and Image Arithmetic in a Relational Database for Multimessenger Astronomy Brokers
- Panning for gold, but finding helium: discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observations
- The luminosity functions of kilonovae from binary neutron star mergers under different equation of states
- Formation of GW230529 from Isolated Binary Evolution
- Black-Hole Neutron Star Simulations with the BAM code: First Tests and Simulations
- Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
- In search of short gamma-ray burst optical counterpart with the Zwicky Transient Facility
- SAGUARO: Time-domain Infrastructure for the Fourth Gravitational-wave Observing Run and Beyond
- Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses
- Foraging with MUSHROOMS: A Mixed-Integer Linear Programming Scheduler for Multimessenger Target of Opportunity Searches with the Zwicky Transient Facility
- IIb or not IIb: A Catalog of ZTF Kilonova Imposters
- Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
- AT2019wxt: An ultra-stripped supernova candidate discovered in electromagnetic follow-up of a gravitational wave trigger
- Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
- WINTER on S250206dm: A near-infrared search for an electromagnetic counterpart to a gravitational-wave event
- Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)
- Kilonova-Targeting Lightcurve Classification for Wide Field Survey Telescope
- An Online Framework for Fitting Fast Transient Lightcurves
- Gravitational Waves and Electromagnetic Transients
- Machine-directed gravitational-wave counterpart discovery
- India's first robotic eye for time domain astrophysics: the GROWTH-India telescope
- Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm
- Mergers of binary neutron star systems: a multi-messenger revolution
- ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
- Light curves and polarizations of gravitationally lensed kilonovae