{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360004234434503552.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1088/1538-3873/aaff99"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/1538-3873/131/i=998/a=048001/pdf"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/1538-3873/131/i=998/a=048001?key=crossref.558f032a01120adb57bb66a802edc432"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1901.11385"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"2900 Square Degree Search for the Optical Counterpart of Short Gamma-Ray Burst GRB 180523B with the Zwicky Transient Facility"}],"description":[{"notation":[{"@value":"There is significant interest in the models for production of short gamma-ray bursts. Until now, the number of known short gamma-ray bursts with multi-wavelength afterglows has been small. While the {\\it Fermi} Gamma-Ray Burst Monitor detects many gamma-ray bursts relative to the Neil Gehrels {\\it Swift} Observatory, the large localization regions makes the search for counterparts difficult. With the Zwicky Transient Facility recently achieving first light, it is now fruitful to use its combination of depth ($m_\\textrm{AB} \\sim 20.6$), field of view ($\\approx$ 47 square degrees), and survey cadence (every $\\sim 3$ days) to perform Target of Opportunity observations. We demonstrate this capability on GRB 180523B, which was recently announced by the {\\it Fermi} Gamma-Ray Burst Monitor as a short gamma-ray burst. ZTF imaged $\\approx$ 2900\\,square degrees of the localization region, resulting in the coverage of 61.6\\,\\% of the enclosed probability over 2 nights to a depth of $m_\\textrm{AB} \\sim 20.5$. We characterized 14 previously unidentified transients, and none were found to be consistent with a short gamma-ray burst counterpart. This search with the Zwicky Transient Facility shows it is an efficient camera for searching for coarsely-localized short gamma-ray burst and gravitational-wave counterparts, allowing for a sensitive search with minimal interruption to its nominal cadence."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004234434504328","@type":"Researcher","foaf:name":[{"@value":"Michael W. Coughlin"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503554","@type":"Researcher","foaf:name":[{"@value":"Tomás Ahumada"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503557","@type":"Researcher","foaf:name":[{"@value":"S. Bradley Cenko"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503555","@type":"Researcher","foaf:name":[{"@value":"Virginia Cunningham"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503938","@type":"Researcher","foaf:name":[{"@value":"Shaon Ghosh"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503556","@type":"Researcher","foaf:name":[{"@value":"Leo P. Singer"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503687","@type":"Researcher","foaf:name":[{"@value":"Eric C. Bellm"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504195","@type":"Researcher","foaf:name":[{"@value":"Eric Burns"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504068","@type":"Researcher","foaf:name":[{"@value":"Kishalay De"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504070","@type":"Researcher","foaf:name":[{"@value":"Adam Goldstein"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504333","@type":"Researcher","foaf:name":[{"@value":"V. Zach Golkhou"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503680","@type":"Researcher","foaf:name":[{"@value":"David L. Kaplan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503941","@type":"Researcher","foaf:name":[{"@value":"Mansi M. Kasliwal"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503940","@type":"Researcher","foaf:name":[{"@value":"Daniel A. Perley"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504069","@type":"Researcher","foaf:name":[{"@value":"Jesper Sollerman"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504073","@type":"Researcher","foaf:name":[{"@value":"Ashot Bagdasaryan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503559","@type":"Researcher","foaf:name":[{"@value":"Richard G. Dekany"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504196","@type":"Researcher","foaf:name":[{"@value":"Dmitry A. Duev"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503430","@type":"Researcher","foaf:name":[{"@value":"Michael Feeney"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503688","@type":"Researcher","foaf:name":[{"@value":"Matthew J. Graham"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504074","@type":"Researcher","foaf:name":[{"@value":"David Hale"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503427","@type":"Researcher","foaf:name":[{"@value":"Shri R. Kulkarni"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504321","@type":"Researcher","foaf:name":[{"@value":"Thomas Kupfer"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504326","@type":"Researcher","foaf:name":[{"@value":"Russ R. Laher"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503431","@type":"Researcher","foaf:name":[{"@value":"Ashish Mahabal"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504325","@type":"Researcher","foaf:name":[{"@value":"Frank J. Masci"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503681","@type":"Researcher","foaf:name":[{"@value":"Adam A. Miller"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503686","@type":"Researcher","foaf:name":[{"@value":"James D. Neill"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503684","@type":"Researcher","foaf:name":[{"@value":"Maria T Patterson"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504071","@type":"Researcher","foaf:name":[{"@value":"Reed Riddle"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503562","@type":"Researcher","foaf:name":[{"@value":"Ben Rusholme"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503936","@type":"Researcher","foaf:name":[{"@value":"Roger Smith"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434504065","@type":"Researcher","foaf:name":[{"@value":"Yutaro Tachibana"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234434503565","@type":"Researcher","foaf:name":[{"@value":"Richard Walters"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00046280"},{"@type":"EISSN","@value":"15383873"}],"prism:publicationName":[{"@value":"Publications of the Astronomical Society of the Pacific"}],"dc:publisher":[{"@value":"IOP Publishing"}],"prism:publicationDate":"2019-02-20","prism:volume":"131","prism:number":"998","prism:startingPage":"048001"},"reviewed":"false","dc:rights":["http://iopscience.iop.org/info/page/text-and-data-mining","http://iopscience.iop.org/page/copyright"],"url":[{"@id":"http://stacks.iop.org/1538-3873/131/i=998/a=048001/pdf"},{"@id":"http://stacks.iop.org/1538-3873/131/i=998/a=048001?key=crossref.558f032a01120adb57bb66a802edc432"}],"createdAt":"2019-02-20","modifiedAt":"2020-04-11","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=High%20Energy%20Astrophysical%20Phenomena%20(astro-ph.HE)","dc:title":"High Energy Astrophysical Phenomena (astro-ph.HE)"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=gamma%20rays:%20general","dc:title":"gamma rays: general"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20High%20Energy%20Astrophysical%20Phenomena","dc:title":"Astrophysics - High Energy Astrophysical Phenomena"},{"@id":"https://cir.nii.ac.jp/all?q=QC","dc:title":"QC"},{"@id":"https://cir.nii.ac.jp/all?q=QB","dc:title":"QB"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040282256881748352","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"16J05742"},{"@type":"JGN","@value":"JP16J05742"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-16J05742/"}],"notation":[{"@language":"ja","@value":"可視光・Ｘ線・ガンマ線観測による活動銀河核の長期活動現象の解明"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050001338209209600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA"}]},{"@id":"https://cir.nii.ac.jp/crid/1360001113987250304","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A DECADE OF SHORT-DURATION GAMMA-RAY BURST BROADBAND AFTERGLOWS: ENERGETICS, CIRCUMBURST DENSITIES, AND JET OPENING ANGLES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002218449836160","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Illuminating gravitational waves: A concordant picture of photons from a neutron star merger"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144123813120","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"AN\n                    <i>r</i>\n                    -PROCESS KILONOVA ASSOCIATED WITH THE SHORT-HARD GRB 130603B"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144733804416","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. III. Optical and UV Spectra of a Blue Kilonova from Fast Polar Ejecta"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144969201536","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE NEEDLE IN THE 100 deg<sup>2</sup>HAYSTACK: UNCOVERING AFTERGLOWS OF<i>FERMI</i>GRBs WITH THE PALOMAR TRANSIENT FACTORY"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145036811904","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The afterglow of GRB 050709 and the nature of the short-hard γ-ray bursts"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145944316800","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011146475970176","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Zwicky Transient Facility: System Overview, Performance, and First Results"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692627693696","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285709411201152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Morphological Classification Model to Identify Unresolved PanSTARRS1 Sources: Application in the ZTF Real-time Pipeline"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619700670592","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619783175680","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ATLAS: A High-cadence All-sky Survey System"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620042043776","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VI. Radio Constraints on a Relativistic Jet and Predictions for Late-time Emission from the Kilonova Ejecta"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620055439616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A kilonova as the electromagnetic counterpart to a gravitational-wave source"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620171565952","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Testing the Standard Fireball Model of Gamma‐Ray Bursts Using Late X‐Ray Afterglows Measured by<i>Swift</i>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620475906176","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"GRB 070707: the first short gamma-ray burst  observed by <i>INTEGRAL</i>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620483869824","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620502706816","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The X-ray counterpart to the gravitational-wave event GW170817"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620569017856","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>FERMI</i>OBSERVATIONS OF GRB 090510: A SHORT-HARD GAMMA-RAY BURST WITH AN ADDITIONAL, HARD POWER-LAW COMPONENT FROM 10 keV TO GeV ENERGIES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565167425758464","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"JET COLLIMATION IN THE EJECTA OF DOUBLE NEUTRON STAR MERGERS: A NEW CANONICAL PICTURE OF SHORT GAMMA-RAY BURSTS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565170737362816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"AN ACHROMATIC BREAK IN THE AFTERGLOW OF THE SHORT GRB 140903A: EVIDENCE FOR A NARROW JET"}]},{"@id":"https://cir.nii.ac.jp/crid/1360568619091284992","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"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"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094091701504","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Rapid Reddening and Featureless Optical Spectra of the Optical Counterpart of GW170817, AT 2017gfo, during the First Four Days"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094329510272","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Exploring the Optical Transient Sky with the Palomar Transient Factory"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094622475520","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Electromagnetic evidence that SSS17a is the result of a binary neutron star merger"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094952210432","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"GRB 060313: A New Paradigm for Short‐Hard Bursts?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095179559040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"SHORT VERSUS LONG AND COLLAPSARS VERSUS NON-COLLAPSARS: A QUANTITATIVE CLASSIFICATION OF GAMMA-RAY BURSTS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096390169600","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"GRB 080503: IMPLICATIONS OF A NAKED SHORT GAMMA-RAY BURST DOMINATED BY EXTENDED EMISSION"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659364632064","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Machine Learning for the Zwicky Transient Facility"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569991287808","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The multi-messenger picture of compact binary mergers"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570071716352","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Black-hole-neutron-star collisions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570150071168","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Evolution of a Structured Relativistic Jet and Gamma‐Ray Burst Afterglow Light Curves"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570257901696","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gamma-Ray Bursts"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855571523721088","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Electromagnetic counterparts of compact object mergers powered by the radioactive decay of r-process nuclei"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137043640715904","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A ‘kilonova’ associated with the short-duration γ-ray burst GRB 130603B"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137043980540544","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Observations of the GRB Afterglow ATLAS17aeu and Its Possible Association with GW 170104"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044153099264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Off-axis Prompt X-Ray Transients from the Cocoon of Short Gamma-Ray Bursts"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045674263168","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Afterglow, Energetics, and Host Galaxy of the Short‐Hard Gamma‐Ray Burst 051221a"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046268400000","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The SED Machine: A Robotic Spectrograph for Fast Transient Classification"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518930396288","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The long-lasting optical afterglow plateau of short burst GRB 130912A"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519888304128","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Faint Afterglow and Host Galaxy of the Short-Hard GRB 060121"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418520202831360","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. V. Rising X-Ray Emission from an Off-axis Jet"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418520250184448","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Palomar Transient Factory: System Overview, Performance, and First Results"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418521067418752","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A mildly relativistic wide-angle outflow in the neutron-star merger event GW170817"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418521498125568","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE WIDE-FIELD INFRARED SURVEY EXPLORER (WISE): MISSION DESCRIPTION AND INITIAL ON-ORBIT PERFORMANCE"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699993630368768","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The afterglow and elliptical host galaxy of the short γ-ray burst GRB 050724"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994312182656","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE LOCATIONS OF SHORT GAMMA-RAY BURSTS AS EVIDENCE FOR COMPACT OBJECT BINARY PROGENITORS"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994987717120","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>Swift</i>and<i>NuSTAR</i>observations of GW170817: Detection of a blue kilonova"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470485887872","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An analysis of the durations of Swift gamma-ray bursts"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470516825344","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spectral Features from Ultrarelativistic Ions in Gamma-Ray Bursts?"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470967827200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE AFTERGLOW AND EARLY-TYPE HOST GALAXY OF THE SHORT GRB 150101B AT z = 0.1343"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943467194880","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"PROPER IMAGE SUBTRACTION—OPTIMAL TRANSIENT DETECTION, PHOTOMETRY, AND HYPOTHESIS TESTING"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943572150272","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"FROM ENGINE TO AFTERGLOW: COLLAPSARS NATURALLY PRODUCE TOP-HEAVY JETS AND EARLY-TIME PLATEAUS IN GAMMA-RAY BURST AFTERGLOWS"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418752297216","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A NEW PARADIGM FOR GAMMA-RAY BURSTS: LONG-TERM ACCRETION RATE MODULATION BY AN EXTERNAL ACCRETION DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544419658993152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The GROWTH Marshal: A Dynamic Science Portal for Time-domain Astronomy"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544421134661248","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Zwicky Transient Facility Alert Distribution System"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894285797504","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Observations of Gamma-Ray Bursts of Cosmic Origin"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368937180288","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The protomagnetar model for gamma-ray bursts"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369295798784","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"GRB 090426: the farthest short gamma-ray burst?"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107370339325184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Shocked by GRB 970228: the afterglow of a cosmological fireball"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843307894016","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Short Gamma‐Ray Bursts with Extended Emission"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844780239744","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Making a Short Gamma-Ray Burst from a Long One: Implications for the Nature of GRB 060614"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844812688000","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Deep Chandra X-Ray Study of Neutron Star Coalescence GW170817"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845124466688","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spectral constraints on the redshift of the optical counterpart to the γ-ray burst of 8 May 1997"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670318953515520","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A radio counterpart to a neutron star merger"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319040640256","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DISCOVERY AND REDSHIFT OF AN OPTICAL AFTERGLOW IN 71 deg\n                    <sup>2</sup>\n                    : iPTF13bxl AND GRB 130702A"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670320425237120","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ELECTROMAGNETIC TRANSIENTS POWERED BY NUCLEAR DECAY IN THE TIDAL TAILS OF COALESCING COMPACT BINARIES"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670320914421888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793536403328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE THIRD FERMI GBM GAMMA-RAY BURST CATALOG: THE FIRST SIX YEARS"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793904484992","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Zwicky Transient Facility: Data Processing, Products, and Archive"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951794376861312","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"MID-INFRARED SELECTION OF ACTIVE GALACTIC NUCLEI WITH THE<i>WIDE-FIELD INFRARED SURVEY EXPLORER</i>. I. CHARACTERIZING<i>WISE</i>-SELECTED ACTIVE GALACTIC NUCLEI IN COSMOS"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795304078336","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"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"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795574045184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A COMPARISON OF THE AFTERGLOWS OF SHORT- AND LONG-DURATION GAMMA-RAY BURSTS"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951796137175040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268159678848","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Transient Events from Neutron Star Mergers"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268782470528","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270399202304","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Optimizing searches for electromagnetic counterparts of gravitational wave triggers"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1088/1538-3873/aaff99"},{"@type":"KAKEN","@value":"PRODUCT-22384811"},{"@type":"OPENAIRE","@value":"doi_dedup___::fd0e2b6c9c46b8ec4190679efbe3cb12"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/ab4ad8_references_DOI_RF0g5Q6gaoSVjid3qkYkj6MKt2A"}]}