activity
20002016
most citedEvent-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre

851 citations · 1.8k across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2016★ 88 cited

Persistent Asymmetric Structure of Sagittarius A* on Event Horizon Scales

Vincent L. Fish, Michael D. Johnson, Sheperd S. Doeleman +69

The Galactic Center black hole Sagittarius A* (Sgr A*) is a prime observing target for the Event Horizon Telescope (EHT), which can resolve the 1.3 mm emission from this source on…

astro-ph.IM2014★ 26 cited

Performance of the Caltech Submillimeter Observatory Dual-Color 180-720 GHz Balanced SIS Receivers

J. W. Kooi, R. A. Chamberlin, R. Monje +12

We report on balanced SIS receivers covering the astronomical important 180-720 GHz submillimeter atmospheric window. To facilitate remote observations and automated spectral line…

astro-ph.HE2013★ 39 cited

Fine-scale structure of the quasar 3C 279 Measured with 1.3 mm very long baseline interferometry

Ru-Sen Lu, Vincent L. Fish, Kazunori Akiyama +30

We report results from 5-day VLBI observations of the well-known quasar 3C 279 at 1.3 mm (230 GHz) in 2011. The measured nonzero closure phases on triangles including stations in A…

astro-ph.HE2012★ 426 cited

Jet Launching Structure Resolved Near the Supermassive Black Hole in M87

Sheperd S. Doeleman, Vincent L. Fish, David E. Schenck +30

Approximately 10% of active galactic nuclei exhibit relativistic jets, which are powered by accretion of matter onto super massive black holes. While the measured width profiles of…

astro-ph.GA2010★ 214 cited

1.3 mm Wavelength VLBI of Sagittarius A*: Detection of Time-Variable Emission on Event Horizon Scales

Vincent L. Fish, Sheperd S. Doeleman, Christopher Beaudoin +27

Sagittarius A*, the ~4 x 10^6 solar mass black hole candidate at the Galactic Center, can be studied on Schwarzschild radius scales with (sub)millimeter wavelength Very Long Baseli…

astro-ph.GA2010★ 44 cited

A Comprehensive Survey of Hydrogen Chloride in the Galaxy

Ruisheng Peng, Hiroshige Yoshida, Richard A. Chamberlin +3

We report new observations of the fundamental transition of HCl (at 625.918GHz) toward a sample of 25 galactic star-forming regions, molecular clouds, and evolved stars, ca…