Personal webpage of Dr. Gunther Witzel
I am a staff scientist in the department for Very Long Baseline Interferometry (VLBI) at the Max Planck Institute for Radio Astronomy (MPIfR) in Bonn, working with Prof. A. Zensus. Before joining the MPIfR, I worked for more than six years at UCLA in the Galactic Center Group of Prof. A. Ghez, Nobel laureat of 2020. For my PhD projects I worked with Prof. A. Eckart at the 1. Pysikalisches Insitut of the University of Cologne.
My main interest is focused on the central regions of galaxies, in particular of our own galaxy, the Milky Way. I am an infrared astronomer by trade, working on observational methods to observe stars on their orbits around the supermassive black hole (SMBH) a the Galactic Center, Sagittarius A*, and to study the accretion process onto the SMBH itsself. I am working on a wide range of topics, from post-processing methods of NIR polarization data, precise astrometry and photometry with adaptive optics in crowded fields, modeling of radiative processes linked to the accretion onto Sagittarius A* and statistical methods of time series analysis in general. Recently, I have extended my scope to multi-wavelegth observations including the radio and mm/submm regime and VLBI studies. I am member of the Event Horizon Telescope Collaboration, the Galactic Center Orbit Initiative, the M2FINDERS collaboration, and the Spitzer/IRAC and Chandra Sgr A* monitoring campaigne.
Phone:
+49 228 525 358
Email: gwitzel (at) mpifr-bonn.mpg.de
Address: Max-Planck-Insitut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
My Publications on ADS
Variability studies of Sagittarius A* provide direct information on the physics at spatial scales of the event horizon of the supermassive black hole at the center of the Milky Way. Learn about a long term study of the properties of this variability and some extraordinary events in 2019 here.
I presented a research talk (part 1 and part 2) on Sagittarius A* at the IAA in Granda, Spain, in November 2018.
The mysterious object G1 and G2 have been discovered in 2012 and are the only resolved instances of objects that tidally interact with a supermassive black hole. Despite predictions that G2 would be desinigrated during its periapsis passage in 2014, G2 survived. This implies a massive stellar core hidden at the center of the extended gas and dust envelope. Learn more.
I gave a research talk on G1 and G2 at the TDE Workshop in Jerusalem, Israel, in November 2015.
The instrumental polarization calibration for adaptive opitcs supported Nasmyth focus intruments is a challenge. We successfully calibrated the instrumental polarization of NAOS/CONICA at the VLT. A summary of our findings can be found in the ESO Messenger Vol. 142.
Griffith Observatory, Los Angeles Photo: GW
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