ログイン
言語:

WEKO3

  • トップ
  • ランキング
To
lat lon distance
To

Field does not validate



インデックスリンク

インデックスツリー

メールアドレスを入力してください。

WEKO

One fine body…

WEKO

One fine body…

アイテム

  1. 学術雑誌論文等

First M87 Event Horizon Telescope Results. II. Array and Instrumentation

https://hiroshima.repo.nii.ac.jp/records/2008903
https://hiroshima.repo.nii.ac.jp/records/2008903
59c16b14-a086-4a36-b8e4-465ae4459587
名前 / ファイル ライセンス アクション
ApJL_875_L2.pdf ApJL_875_L2.pdf (3.1 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. II. Array and Instrumentation
言語 en
作成者 The Event Horizon Telescope Collaboration

× The Event Horizon Telescope Collaboration

en The Event Horizon Telescope Collaboration

Search repository
Sasada, Mahito

× Sasada, Mahito

en Sasada, Mahito

Search repository
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)
主題
主題Scheme Other
主題 Galaxy: center
主題
主題Scheme Other
主題 gravitational lensing: strong
主題
主題Scheme Other
主題 instrumentation: interferometers
主題
主題Scheme Other
主題 echniques: high angular resolution
内容記述
内容記述 The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of ∼1.3 mm, EHT angular resolution (λ/D) is ∼25 μas, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of the EHT, detail the technology and instrumentation that enable observations, and provide measures of its performance. Meeting the EHT science objectives has required several key developments that have facilitated the robust extension of the VLBI technique to EHT observing wavelengths and the production of instrumentation that can be deployed on a heterogeneous array of existing telescopes and facilities. To meet sensitivity requirements, high-bandwidth digital systems were developed that process data at rates of 64 gigabit s^−1, exceeding those of currently operating cm-wavelength VLBI arrays by more than an order of magnitude. Associated improvements include the development of phasing systems at array facilities, new receiver installation at several sites, and the deployment of hydrogen maser frequency standards to ensure coherent data capture across the array. These efforts led to the coordination and execution of the first Global EHT observations in 2017 April, and to event-horizon-scale imaging of the supermassive black hole candidate 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/ab0c96
関連情報
識別子タイプ DOI
関連識別子 https://doi.org/10.3847/2041-8213/ab0c96
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 L2
書誌情報 The Astrophysical Journal Letters
The Astrophysical Journal Letters

巻 875, 号 1, p. L2, 発行日 2019-04-10
旧ID 48225
戻る
0
views
See details
Views

Versions

Ver.1 2025-02-21 04:38:32.985259
Show All versions

Share

Mendeley Twitter Facebook Print Addthis

Cite as

エクスポート

OAI-PMH
  • OAI-PMH JPCOAR 2.0
  • OAI-PMH JPCOAR 1.0
  • OAI-PMH DublinCore
  • OAI-PMH DDI
Other Formats
  • JSON
  • BIBTEX

Confirm


Powered by WEKO3


Powered by WEKO3