activity
20042026
most citedFirst Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

1.9k citations · 16.8k across the 139 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

18 papers · 1 filter

astro-ph.IM2026

First Very Long Baseline Interferometry Fringe Detection at 690GHz

Ming-Tang Chen, Geoffrey B. Crew, Dan Bintley +42

We report the first very long baseline interferometry (VLBI) experiment conducted in the 690 GHz atmospheric window. On 2024 November 21, observations with the Atacama Large Millim…

astro-ph.IM2025

Multiobjective optimization for scattering mitigation and scattering screen reconstruction in VLBI observations of the Galactic Center

Alejandro Mus, Teresa Toscano, Hendrik Müller +3

Imaging reconstruction of interferometric data is a hard ill-posed inverse problem. Its difficulty is increased when observing the Galactic Center, which is obscured by a scatterin…

astro-ph.IM2025

A Novel Calibration and Imaging Method for ALMA Observations of SgrA*

Ezequiel Albentosa-Ruiz, Iván Martí-Vidal, Ciriaco Goddi +1

This document presents a novel method for the intra-field calibration and imaging of the radio source SgrA*, observed with the Atacama Large Millimeter/submillimeter Array (ALMA).…

astro-ph.IM2024★ 30 cited

First Very Long Baseline Interferometry Detections at 870μm

Alexander W. Raymond, Sheperd S. Doeleman, Keiichi Asada +276

The first very long baseline interferometry (VLBI) detections at 870m wavelength (345GHz frequency) are reported, achieving the highest diffraction-limited angular resolutio…

astro-ph.IM2023

Metadata for the Flux Density Calibration of the April 2018 Event Horizon Telescope Data

J. Y. Koay, C. Romero-Cañizales, L. D. Matthews +29

The Event Horizon Telescope (EHT) observations carried out in 2018 April at 1.3 mm wavelengths included 9 stations in the array, comprising 7 single-dish telescopes and 2 phased ar…

astro-ph.IM2023★ 17 cited

A Characterization of the ALMA Phasing System at 345 GHz

G. B. Crew, C. Goddi, L. D. Matthews +3

The development of the Atacama Large Millimeter/submillimeter Array (ALMA) phasing system (APS) has allowed ALMA to function as an extraordinarily sensitive station for very long b…