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Identification of Spinning Dust in Halpha-Correlated Microwave Emission
Gregory Dobler, Douglas P. Finkbeiner
CMB experiments commonly use maps of Halpha intensity as a spatial template for Galactic free-free emission, assuming a power law I_nu \propto nu^-0.15 for the spectrum. Any depart…
Extended Anomalous Foreground Emission in the WMAP 3-Year Data
Gregory Dobler, Douglas P. Finkbeiner
We study the spectral and morphological characteristics of the diffuse Galactic emission in the WMAP temperature data using a template-based multi-linear regression, and obtain the…
Prospects For Detecting Dark Matter With GLAST In Light Of The WMAP Haze
Dan Hooper, Gabrijela Zaharijas, Douglas P. Finkbeiner +1
Observations by the WMAP experiment have identified an excess of microwave emission from the center of the Milky Way. It has previously been shown that this "WMAP Haze" could be sy…
Stellar SEDs from 0.3-2.5 Microns: Tracing the Stellar Locus and Searching for Color Outliers in SDSS and 2MASS
Kevin R. Covey, Zeljko Ivezic, David J. Schlegel +15
The Sloan Digital Sky Survey (SDSS) and Two Micron All Sky Survey (2MASS) are rich resources for studying stellar astrophysics and the structure and formation history of the Galaxy…
Evidence Of Dark Matter Annihilations In The WMAP Haze
Dan Hooper, Douglas P. Finkbeiner, Gregory Dobler
The WMAP experiment has revealed an excess of microwave emission from the region around the center of our Galaxy. It has been suggested that this signal, known as the ``WMAP Haze''…
Exploring the Variable Sky with the Sloan Digital Sky Survey
Branimir Sesar, Zeljko Ivezic, Robert H. Lupton +29
We quantify the variability of faint unresolved optical sources using a catalog based on multiple SDSS imaging observations. The catalog covers SDSS Stripe 82, and contains 58 mill…