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Far Infrared Variability of Sagittarius A*: 25.5 Hours of Monitoring with
Jordan M. Stone, D. P. Marrone, C. D. Dowell +3
Variable emission from Sgr~A*, the luminous counterpart to the super-massive black hole at the center of our Galaxy, arises from the innermost portions of the accretion flow. Bette…
The redshift distribution of dusty star forming galaxies from the SPT survey
M. L. Strandet, A. Weiß, J. D. Vieira +28
We use the Atacama Large Millimeter/submillimeter Array (ALMA) in Cycle 1 to determine spectroscopic redshifts of high-redshift dusty star-forming galaxies (DSFGs) selected by thei…
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…