activity
20042026
most citedFirst Results from High Angular Resolution ALMA Observations Toward the HL Tau Region

1.2k citations · 1.8k across the 30 of their papers we have counts for

collaborators

29 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.IM2026

The ngVLA Band-4 Water Vapor Radiometry Concept

Tirupati Kumara Sridharan, Robert Lehmensiek, Yoshiharu Asaki

The ngVLA has adopted a standalone system with a ~1.5 m diameter antenna and associated ambient temperature receiver and electronics at each antenna as its baseline design fo…

astro-ph.EP2024★ 24 cited

Into the thick of it: ALMA 0.45 mm observations of HL Tau at 2 au resolution

Osmar M. Guerra-Alvarado, Carlos Carrasco-González, Enrique Macías +7

Aims. To comprehend the efficiency of dust evolution within protoplanetary disks, it is crucial to conduct studies of these disks using high-resolution observations at multiple wav…

astro-ph.IM2023

ALMA High-frequency Long Baseline Campaign in 2021: Highest Angular Resolution Submillimeter Wave Images for the Carbon-rich Star R Lep

Yoshiharu Asaki, Luke T. Maud, Harold Francke +11

The Atacama Large Millimeter/submillimeter Array (ALMA) was used in 2021 to image the carbon-rich evolved star R Lep in Bands 8-10 (397-908 GHz) with baselines up to 16 km. The goa…

astro-ph.IM2023★ 4 cited

Updates to ALMA Site Properties: using the ESO-Allegro Phase RMS database -- ALMA Memo 624

Luke T. Maud, Andrés F. Pérez-Sánchez, Yoshiharu Asaki +3

We present a long-term overview of the atmospheric phase stability at the Atacama Large Millimeter/submillimeter Array (ALMA) site, using >5 years of data, that acts as the success…

astro-ph.IM2023★ 28 cited

The Transformational Power of Frequency Phase Transfer Methods for ngEHT

María J. Rioja, Richard Dodson, Yoshiharu Asaki

(Sub) mm VLBI observations are strongly hindered by limited sensitivity, with the fast tropospheric fluctuations being the dominant culprit. We predict great benefits from applying…