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dc.contributor.authorMena-Parra, J
dc.contributor.authorLeung, C
dc.contributor.authorCary, S
dc.contributor.authorMasui, KW
dc.contributor.authorKaczmarek, JF
dc.contributor.authorAmiri, M
dc.contributor.authorBandura, K
dc.contributor.authorBoyle, PJ
dc.contributor.authorCassanelli, T
dc.contributor.authorCliche, J-F
dc.contributor.authorDobbs, M
dc.contributor.authorKaspi, VM
dc.contributor.authorLandecker, TL
dc.contributor.authorLanman, A
dc.contributor.authorSievers, JL
dc.date.accessioned2022-04-27T17:39:37Z
dc.date.available2022-04-27T17:39:37Z
dc.date.issued2022-02-01
dc.identifier.urihttps://hdl.handle.net/1721.1/142150
dc.description.abstract<jats:title>Abstract</jats:title> <jats:p>The Canadian Hydrogen Intensity Mapping Experiment (CHIME) has emerged as the prime telescope for detecting fast radio bursts (FRBs). CHIME/FRB Outriggers will be a dedicated very-long-baseline interferometry (VLBI) instrument consisting of outrigger telescopes at continental baselines working with CHIME and its specialized real-time transient-search backend (CHIME/FRB) to detect and localize FRBs with 50 mas precision. In this paper, we present a minimally invasive clock stabilization system that effectively transfers the CHIME digital backend reference clock from its original GPS-disciplined ovenized crystal oscillator to a passive hydrogen maser. This enables us to combine the long-term stability and absolute time tagging of the GPS clock with the short- and intermediate-term stability of the maser to reduce the clock timing errors between VLBI calibration observations. We validate the system with VLBI-style observations of Cygnus A over a 400 m baseline between CHIME and the CHIME Pathfinder, demonstrating agreement between sky-based and maser-based timing measurements at the 30 ps rms level on timescales ranging from one minute to up to nine days, and meeting the stability requirements for CHIME/FRB Outriggers. In addition, we present an alternate reference clock solution for outrigger stations that lack the infrastructure to support a passive hydrogen maser.</jats:p>en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/1538-3881/ac397aen_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.titleA Clock Stabilization System for CHIME/FRB Outriggersen_US
dc.typeArticleen_US
dc.identifier.citationMena-Parra, J, Leung, C, Cary, S, Masui, KW, Kaczmarek, JF et al. 2022. "A Clock Stabilization System for CHIME/FRB Outriggers." The Astronomical Journal, 163 (2).
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Research
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.relation.journalThe Astronomical 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.updated2022-04-27T17:37:24Z
dspace.orderedauthorsMena-Parra, J; Leung, C; Cary, S; Masui, KW; Kaczmarek, JF; Amiri, M; Bandura, K; Boyle, PJ; Cassanelli, T; Cliche, J-F; Dobbs, M; Kaspi, VM; Landecker, TL; Lanman, A; Sievers, JLen_US
dspace.date.submission2022-04-27T17:37:26Z
mit.journal.volume163en_US
mit.journal.issue2en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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