I am a graduate student at the UH Institute for Astronomy. I study the distribution of galaxies on large scales with the goal of understanding how the Universe has evolved over cosmological time. This gives clues about the dark components of the Universe: dark matter and dark energy.
My work combines all-sky galaxy surveys such as SDSS and Pan-STARRS with cosmic microwave background data from the NASA WMAP satellite. I also use data from Mauna Kea observatories.
Granett, B.R., Szapudi, I., & Neyrinck, M.C. Galaxy Counts on the CMB Cold Spot ApJ Submitted Nov 2009.

Granett, B.R., Neyrinck, M.C. & Szapudi, I., A Map of the Integrated Sachs-Wolfe Signal from Luminous Red Galaxies ApJ v701, p414, 2009.

Granett, B.R., Neyrinck, M.C. & Szapudi, I., An Imprint of Superstructures on the Microwave Background due to the Integrated Sachs-Wolfe Effect ApJ Letters v683, L99, 2008.

Stubbs, et Granett, B.R. et al Toward More Precise Survey Photometry for PanSTARRS and LSST: Measuring Directly the Optical Transmission Spectrum of the Atmosphere PASP v119 p1163, 2007.
Granett, B.R. et al The Pan-STARRS Imaging Sky Probe AMOS conference proceeding Ed.: S. Ryan, 2006.
View my curriculum vitae: PDF document.