activity
20092026
most citedAn independent hybrid imaging of Sgr A* from the data in EHT 2017 observations

8 citations · 13 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Short timescale variation in the submillimeter flux of Sagittarius A*

Makoto Miyoshi, Yoshiaki Kato, Yoshiharu Asaki +8

We study short-timescale 340 GHz flux-density variability of Sgr A* using ALMA Cycle 3 observations. Careful self-calibration enabled 10 s snapshot imaging with very high effective…

astro-ph.HE2024★ 8 cited

An independent hybrid imaging of Sgr A* from the data in EHT 2017 observations

Makoto Miyoshi, Yoshiaki Kato, Junichiro Makino

We propose that the ring structure found by the Event Horizon Telescope Collaboration (EHTC) as the black hole shadow of Sgr A*is an artifact by the bumpy PSF (Point Spread Functio…

astro-ph.IM2024

Black hole ring images from PSF structures

Makoto Miyoshi, Yoshiaki Kato, Junichiro Makino

Two critical aspects of radio interferometric imaging analysis are data calibration and deconvolution of the point spread function (PSF) structure. Both of these are particularly i…

astro-ph.HE2024

The jet and resolved features of the central supermassive black hole of M 87 observed with EHT in 2017 -- Comparison with the GMVA 86 GHz results

Makoto Miyoshi, Yoshiaki Kato, Junichiro Makino +1

M 87 is the best target for studying black hole accretion and jet formation. Reanalysis of the EHT public data at 230 GHz shows a core-knots structure at the center and jet feature…

astro-ph.HE2022★ 2 cited

Comments on "Imaging Reanalyses of EHT Data"

Makoto Miyoshi, Yoshiaki Kato, Jun Makino

On June 14, 2022, the EHT collaboration (hereafter EHTC) made the web page (https://eventhorizontelescope.org/blog/imaging-reanalyses-eht-data) with the title "Imaging Reanalyses o…

astro-ph.HE2009★ 3 cited

Oscillation Phenomena in the disk around the massive black hole Sagittarius A*

M. Miyoshi, Zhi-Qiang Shen, T. Oyama +2

We report the detection of radio QPOs with structure changes using the Very Long Baseline Array (VLBA) at 43 GHz. We found conspicuous patterned changes of the structure with P = 1…