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First M87 Event Horizon Telescope Results. III. Data Processing and Calibration

https://hiroshima.repo.nii.ac.jp/records/2008904
https://hiroshima.repo.nii.ac.jp/records/2008904
186947a6-5c9f-4316-9b21-10cc9218435d
名前 / ファイル ライセンス アクション
ApJL_875_L3.pdf ApJL_875_L3.pdf (14.5 MB)
Item type デフォルトアイテムタイプ_(フル)(1)
公開日 2023-03-18
タイトル
タイトル First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
言語 en
作成者 The Event Horizon Telescope Collaboration

× The Event Horizon Telescope Collaboration

en The Event Horizon Telescope Collaboration

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Sasada, Mahito

× Sasada, Mahito

en Sasada, Mahito

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アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利情報
権利情報 © 2019. The American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
主題
主題Scheme Other
主題 black hole physics
主題
主題Scheme Other
主題 galaxies: individual (M87, 3C279)
主題
主題Scheme Other
主題 galaxies: jets
主題
主題Scheme Other
主題 techniques: high angular resolution
主題
主題Scheme Other
主題 techniques: interferometric
内容記述
内容記述 We present the calibration and reduction of Event Horizon Telescope (EHT) 1.3 mm radio wavelength observations of the supermassive black hole candidate at the center of the radio galaxy M87 and the quasar 3C 279, taken during the 2017 April 5–11 observing campaign. These global very long baseline interferometric observations include for the first time the highly sensitive Atacama Large Millimeter/submillimeter Array (ALMA); reaching an angular resolution of 25 μas, with characteristic sensitivity limits of ∼1 mJy on baselines to ALMA and ∼10 mJy on other baselines. The observations present challenges for existing data processing tools, arising from the rapid atmospheric phase fluctuations, wide recording bandwidth, and highly heterogeneous array. In response, we developed three independent pipelines for phase calibration and fringe detection, each tailored to the specific needs of the EHT. The final data products include calibrated total intensity amplitude and phase information. They are validated through a series of quality assurance tests that show consistency across pipelines and set limits on baseline systematic errors of 2% in amplitude and 1° in phase. The M87 data reveal the presence of two nulls in correlated flux density at ∼3.4 and ∼8.3 Gλ and temporal evolution in closure quantities, indicating intrinsic variability of compact structure on a timescale of days, or several light-crossing times for a few billion solar-mass black hole. These measurements provide the first opportunity to image horizon-scale structure in M87.
言語 en
出版者
出版者 The American Astronomical Society
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
関連情報
識別子タイプ DOI
関連識別子 10.3847/2041-8213/ab0c57
関連情報
識別子タイプ DOI
関連識別子 https://doi.org/10.3847/2041-8213/ab0c57
収録物識別子
収録物識別子タイプ ISSN
収録物識別子 2041-8205
収録物識別子
収録物識別子タイプ ISSN
収録物識別子 2041-8213
開始ページ
開始ページ L3
書誌情報 The Astrophysical Journal Letters
The Astrophysical Journal Letters

巻 875, 号 1, p. L3, 発行日 2019-04-10
旧ID 48226
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