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20212026
most citedFirst Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric

681 citations · 1.7k across the 68 of their papers we have counts for

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astro-ph.IM2025

Spectral characterization and performance of SPT-SLIM on-chip filterbank spectrometers

C. S. Benson, K. Fichman, M. Adamic +26

The South Pole Telescope Shirokoff Line Intensity Mapper (SPT-SLIM) experiment is a pathfinder for demonstrating the use of on-chip spectrometers for millimeter (mm) Line Intensity…

astro-ph.IM2025

First frequency phase transfer from the 3 mm to the 1 mm band on an Earth-sized baseline

Sara Issaoun, Dominic W. Pesce, María J. Rioja +33

Frequency Phase Transfer (FPT) is a technique designed to increase coherence and sensitivity in radio interferometry by making use of the non-dispersive nature of the troposphere t…

astro-ph.IM2025

Concept integral field unit spectrometer instrument for the next-generation mm-wave cosmological surveys

Attila Kovács, Garrett K. Keating, Thomas R. Greve +1

Past millimeter-wave galaxy surveys have primarily probed the brightest starburst galaxies only and suffered heavily from confusion. The interpretation of existing surveys has also…

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.IM2024

Upgrading the Submillimeter Array: wSMA and beyond

Paul K. Grimes, Garrett K. Keating, Raymond Blundell +12

The Submillimeter Array (SMA) is an array of 8 antennas operating at millimeter and submillimeter wavelengths on Maunakea, Hawaii, operated by the Smithsonian Astrophysical Observa…

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…