Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/179927
Share/Export:
logo share SHARE logo core CORE BASE
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE

Invite to open peer review
Title

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

AuthorsThe Event Horizon Telescope Collaboration; Alberdi, Antxón CSIC ORCID ; Gómez, José L. CSIC ORCID
KeywordsBlack hole physics
Galaxies: individual (M87, 3C279)
Galaxies: jets
Techniques: high angular resolution
Techniques: interferometric
Issue Date10-Apr-2019
PublisherInstitute of Physics Publishing
American Astronomical Society
CitationAstrophysical Journal Letters 875(1): L3 (2019)
AbstractWe 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.© 2019. The American Astronomical Society
Publisher version (URL)http://dx.doi.org/10.3847/2041-8213/ab0c57
URIhttp://hdl.handle.net/10261/179927
DOI10.3847/2041-8213/ab0c57
ISSN2041-8205
E-ISSN2041-8213
Appears in Collections:(IAA) Artículos




Files in This Item:
Show full item record

CORE Recommender

SCOPUSTM   
Citations

355
checked on May 16, 2024

WEB OF SCIENCETM
Citations

422
checked on Feb 22, 2024

Page view(s)

630
checked on May 22, 2024

Download(s)

198
checked on May 22, 2024

Google ScholarTM

Check

Altmetric

Altmetric


WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.