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Douglas Finkbeiner, Assistant Professor of Astronomy

Douglas Finkbeiner was born in Ann Arbor, MI, graduated from Pioneer High School in 1989, and enrolled in the College of Engineering at the University of Michigan. His Freshman year he helped build Sunrunner and was active planning race strategy for the U of M Solar Car Team. After study programs in literature (Freiburg, Germany) and art history (Florence, Italy), and a summer at the Cambridge Institute of Astronomy with Simon White, he graduated in 1994 with a dual major in physics and German literature.

As a graduate student in the UC Berkeley Physics Department, Finkbeiner worked with Marc Davis & David Schlegel to produce a dust map, useful for estimating Galactic extinction and Galactic microwave emission, which is a significant foreground for CMB anisotropy experiments.

As a postdoc in the Department of Astrophysical Sciences at Princeton, Finkbeiner became involved with the Sloan Digital Sky Survey (SDSS), in particular the problem of finding a self-consistent global photometric solution for several hundred million objects. This "ubercalibration" was done with Nikhil Padmanabhan and David Schlegel. Finkbeiner also studied the Galactic microwave emission in the WMAP data, finding signs of both the long-suspected spinning dust emission and the unexpected haze, which may be synchrotron emission from cosmic-ray electrons and positrons produced by dark matter annihilation. This possibility is now being investigated at CfA by Finkbeiner, along with postdoc Greg Dobler. CfA has also joined Pan-STARRs.

Other links:
DEEP2
astrometry.net
Murchinson Widefield Array
Initiative in Innovative Computing