activity
20082024
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 · 3.6k across the 25 of their papers we have counts for

collaborators

25 papers

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.HE2023★ 1.9k cited

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

The Event Horizon Telescope Collaboration

We present the first Event Horizon Telescope (EHT) observations of Sagittarius A* (Sgr A), the Galactic center source associated with a supermassive black hole. These observati…

astro-ph.HE2023★ 154 cited

A ring-like accretion structure in M87 connecting its black hole and jet

Ru-Sen Lu, Keiichi Asada, Thomas P. Krichbaum +118

The nearby radio galaxy M87 is a prime target for studying black hole accretion and jet formation^{1,2}. Event Horizon Telescope observations of M87 in 2017, at a wavelength of 1.3…

astro-ph.IM2022★ 60 cited

BURSTT: Bustling Universe Radio Survey Telescope in Taiwan

Hsiu-Hsien Lin, Kai-yang Lin, Chao-Te Li +44

Fast Radio Bursts (FRBs) are bright millisecond-duration radio transients that appear about 1,000 times per day, all-sky, for a fluence threshold 5 Jy ms at 600 MHz. The FRB radio-…

astro-ph.IM2020★ 1 cited

Commissioning of Namakanui on the JCMT

Izumi Mizuno, Per Friberg, Ryan Berthold +39

Namakanui is an instrument containing three inserts in an ALMA type Dewar. The three inserts are Alaihi, Uu and Aweoweo operating around 86, 230 and 345GHz. The receiver is being c…

astro-ph.IM2019★ 1.1k cited

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

The Event Horizon Telescope Collaboration

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comp…

astro-ph.IM2018★ 1 cited

Electronics Instrumentation for the Greenland Telescope

Derek Kubo, Chih-Chiang Han, Hiroaki Nishioka +37

The Greenland Telescope project has recently participated in an experiment to image the supermassive black hole shadow at the center of M87 using Very Long Baseline Interferometry…

astro-ph.IM2016★ 8 cited

The Greenland Telescope: Antenna Retrofit Status and Future Plans

Philippe Raffin, Paul T. P. Ho, Keiichi Asada +32

Since the ALMA North America Prototype Antenna was awarded to the Smithsonian Astrophysical Observatory (SAO), SAO and the Academia Sinica Institute of Astronomy & Astrophysics (AS…

astro-ph.IM2016★ 8 cited

The Atacama Large Millimeter/submillimeter Array (ALMA) Band-1 Receiver

Yau De Huang, Oscar Morata, Patrick Michel Koch +29

The Atacama Large Millimeter/submillimeter Array(ALMA) Band 1 receiver covers the 35-50 GHz frequency band. Development of prototype receivers, including the key components and sub…

astro-ph.CO2016★ 1 cited

AMiBA: Cluster Sunyaev-Zel'dovich Effect Observations with the Expanded 13-Element Array

Kai-Yang Lin, Hiroaki Nishioka, Fu-Cheng Wang +35

The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is a co-planar interferometer array operating at a wavelength of 3mm to measure the Sunyaev-Zeldovich effect (SZ…

astro-ph.GA2015★ 16 cited

First-generation Science Cases for Ground-based Terahertz Telescopes

Hiroyuki Hirashita, Patrick M. Koch, Satoki Matsushita +33

Ground-based observations at terahertz (THz) frequencies are a newly explorable area of astronomy for the next ten years. We discuss science cases for a first-generation 10-m class…

astro-ph.IM2014★ 4 cited

The Greenland Telescope (GLT): Antenna status and future plans

Philippe Raffin, Juan Carlos Algaba-Marcos, Keichi Asada +29

The ALMA North America Prototype Antenna was awarded to the Smithsonian Astrophysical Observatory (SAO) in 2011. SAO and the Academia Sinica Institute of Astronomy & Astrophysics (…

astro-ph.IM2013★ 1 cited

Platform Deformation Phase Correction for the AMiBA-13 Co-planar Interferometer

Yu-Wei Liao, Kai-Yang Lin, Yau-De Huang +17

We present a new way to solve the platform deformation problem of co-planar interferometers. The platform of a co-planar interferometer can be deformed due to driving forces and gr…

astro-ph.IM2010★ 4 cited

1.2 Meter Shielded Cassegrain Antenna for Close-Packed Radio Interferometer

Patrick M. Koch, Philippe Raffin, Yau-De Huang +17

Interferometric millimeter observations of the cosmic microwave background and clusters of galaxies with arcmin resolutions require antenna arrays with short spacings. Having all a…

astro-ph.CO2010★ 5 cited

Contamination of the Central Sunyaev--Zel'dovich Decrements in AMiBA Galaxy Cluster Observations

Guo-Chin Liu, Mark Birkinshaw, Jiun-Huei Proty Wu +26

We investigate the contamination of the Sunyaev--Zel'dovich (SZ) effect for six galaxy clusters, A1689, A1995, A2142, A2163, A2261, and A2390, observed by the Y. T. Lee Array for M…

astro-ph.CO2010★ 19 cited

AMiBA Wideband Analog Correlator

Chao-Te Li, Derek Y. Kubo, Warwick Wilson +27

A wideband analog correlator has been constructed for the Yuan-Tseh Lee Array for Microwave Background Anisotropy. Lag correlators using analog multipliers provide large bandwidth…

astro-ph.CO2010★ 8 cited

AMiBA: Sunyaev-Zel'dovich effect derived properties and scaling relations of massive galaxy clusters

Yu-Wei Liao, Jiun-Huei Proty Wu, Paul T. P. Ho +27

The Sunyaev-Zel'dovich Effect (SZE) has been observed toward six massive galaxy clusters, at redshifts 0.091 \leq z \leq 0.322 in the 86-102 GHz band with the Y. T. Lee Array for M…

astro-ph.CO2009★ 16 cited

AMiBA: scaling relations between the integrated Compton-y and X-ray derived temperature, mass, and luminosity

Chih-Wei Locutus Huang, Jiun-Huei Proty Wu, Paul T. P. Ho +27

We investigate the scaling relations between the X-ray and the thermal Sunyaev-Zel'dovich Effect (SZE) properties of clusters of galaxies, using data taken during 2007 by the Y.T.…

astro-ph.IM2009

Platform Deformation Refined Pointing and Phase Correction for the AMiBA Hexapod Telescope

Patrick M. Koch, Michael Kesteven, Yu-Yen Chang +26

The Array for Microwave Background Anisotropy (AMiBA) is a radio interferometer for research in cosmology, currently operating 7 0.6m diameter antennas co-mounted on a 6m diameter…

astro-ph.CO2009★ 31 cited

AMiBA: Broadband Heterodyne CMB Interferometry

Ming-Tang Chen, Chao-Te Li, Yuh-Jing Hwang +28

The Y. T. Lee Array for Microwave Background (AMiBA) has reported the first science results on the detection of galaxy clusters via the Sunyaev Zel'dovich effect. The science objec…

astro-ph.IM2009★ 16 cited

AMiBA: System Performance

Kai-Yang Lin, Chao-Te Li, Paul T. P. Ho +29

The Y.T. Lee Array for Microwave Background Anisotropy (AMiBA) started scientific operation in early 2007. This work describes the optimization of the system performance for the me…

astro-ph.CO2009★ 45 cited

The AMiBA Hexapod Telescope Mount

Patrick M. Koch, Michael Kesteven, Hiroaki Nishioka +35

AMiBA is the largest hexapod astronomical telescope in current operation. We present a description of this novel hexapod mount with its main mechanical components -- the support co…

astro-ph2008★ 14 cited

Tests of AMiBA Data Integrity

Hiroaki Nishioka, Fu-Cheng Wang, Jiun-Huei Proty Wu +26

We describe methods used to validate data from the Y.T. Lee Array for Microwave Background Anisotropy (AMiBA), an interferometric array designed to measure the Sunyaev-Zel'dovich e…

astro-ph2008★ 38 cited

The Yuan-Tseh Lee Array for Microwave Background Anisotropy

Paul T. P. Ho, Pablo Altamirano, Chia-Hao Chang +52

The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is the first interferometer dedicated to studying the cosmic microwave background (CMB) radiation at 3mm wavelen…