papers

Publications (7)

astro-ph.HE2012

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-ph2008

Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre

Sheperd Doeleman, Jonathan Weintroub, Alan E. E. Rogers +25

The cores of most galaxies are thought to harbour supermassive black holes, which power galactic nuclei by converting the gravitational energy of accreting matter into radiation (r…

astro-ph.CO2009

Imaging an Event Horizon: submm-VLBI of a Super Massive Black Hole

Sheperd Doeleman, Eric Agol, Don Backer +20

A long standing goal in astrophysics is to directly observe the immediate environment of a black hole with angular resolution comparable to the event horizon. Realizing this goal w…

astro-ph.GA2016

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.IM2009

The Synoptic All-Sky Infrared (SASIR) Survey

Joshua S. Bloom, J. Xavier Prochaska, William Lee +42

We are proposing to conduct a multicolor, synoptic infrared (IR) imaging survey of the Northern sky with a new, dedicated 6.5-meter telescope at San Pedro Mártir (SPM) Observatory…

astro-ph.GA2010

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.GA2018

Detection of intrinsic source structure at ~3 Schwarzschild radii with Millimeter-VLBI observations of SAGITTARIUS A*

Ru-Sen Lu, Thomas P. Krichbaum, Alan L. Roy +53

We report results from very long baseline interferometric (VLBI) observations of the supermassive black hole in the Galactic center, Sgr A*, at 1.3 mm (230 GHz). The observations w…