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dc.contributor.authorMasui, Kiyoshi
dc.date.accessioned2022-04-27T17:33:08Z
dc.date.available2022-04-27T17:33:08Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/142147
dc.description.abstract<jats:title>Abstract</jats:title> <jats:p>We present a synthesis of fast radio burst (FRB) morphology (the change in flux as a function of time and frequency) as detected in the 400–800 MHz octave by the FRB project on the Canadian Hydrogen Intensity Mapping Experiment (CHIME/FRB), using events from the first CHIME/FRB catalog. The catalog consists of 62 bursts from 18 repeating sources, plus 474 one-off FRBs, detected between 2018 July 25 and 2019 July 2. We identify four observed archetypes of burst morphology (“simple broadband,” “simple narrowband,” “temporally complex,” and “downward drifting”) and describe relevant instrumental biases that are essential for interpreting the observed morphologies. Using the catalog properties of the FRBs, we confirm that bursts from repeating sources, on average, have larger widths, and we show, for the first time, that bursts from repeating sources, on average, are narrower in bandwidth. This difference could be due to beaming or propagation effects, or it could be intrinsic to the populations. We discuss potential implications of these morphological differences for using FRBs as astrophysical tools.</jats:p>en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/1538-4357/AC33ACen_US
dc.rightsCreative Commons Attribution 4.0 International licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceThe American Astronomical Societyen_US
dc.titleFast Radio Burst Morphology in the First CHIME/FRB Catalogen_US
dc.typeArticleen_US
dc.identifier.citationMasui, Kiyoshi. 2021. "Fast Radio Burst Morphology in the First CHIME/FRB Catalog." Astrophysical Journal, 923 (1).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Research
dc.relation.journalAstrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-04-27T17:29:23Z
dspace.orderedauthorsPleunis, Z; Good, DC; Kaspi, VM; Mckinven, R; Ransom, SM; Scholz, P; Bandura, K; Bhardwaj, M; Boyle, PJ; Brar, C; Cassanelli, T; Chawla, P; (Adam) Dong, F; Fonseca, E; Gaensler, BM; Josephy, A; Kaczmarek, JF; Leung, C; Lin, H-H; Masui, KW; Mena-Parra, J; Michilli, D; Ng, C; Patel, C; Rafiei-Ravandi, M; Rahman, M; Sanghavi, P; Shin, K; Smith, KM; Stairs, IH; Tendulkar, SPen_US
dspace.date.submission2022-04-27T17:29:24Z
mit.journal.volume923en_US
mit.journal.issue1en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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