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This document summarizes the results of a community-based discussion of the potential science impact of the Mayall+BigBOSS highly multiplexed multi-object spectroscopic capability. The KPNO Mayall 4m telescope equipped with the DOE- and internationally-funded BigBOSS spectrograph offers one of the most cost-efficient ways of accomplishing many of the pressing scientific goals identified for this decade by the "New Worlds, New Horizons" report. The BigBOSS Key Project will place unprecedented constraints on cosmological parameters related to the expansion history of the universe. With the addition of an open (publicly funded) community access component, the scientific impact of BigBOSS can be extended to many important astrophysical questions related to the origin and evolution of galaxies, stars, and the IGM. Massive spectroscopy is the critical missing ingredient in numerous ongoing and planned ground- and space-based surveys, and BigBOSS is unique in its ability to provide this to the US community. BigBOSS data from community-led projects will play a vital role in the education and training of students and in maintaining US leadership in these fields of astrophysics. We urge the NSF-AST division to support community science with the BigBOSS multi-object spectrograph through the period of the BigBOSS survey in order to ensure public access to the extraordinary spectroscopic capability., Comment: 5 pages; this white paper was produced as input to the NSF-AST portfolio review

Detailed temperature and abundance radial profile maps have revealed a significant lack of homogeneity within the Perseus Galaxy cluster. Previous surveys of Perseus with the Suzaku telescope, which has a worse angular resolution and less light collecting area than XMM-Newton, revealed over-densities of X-Ray emission. These results provide evidence that the baryon fraction exceeds the universal average, which we had initially hoped to study. We have yet to confirm or deny the existence of clumping in these regions, which could explain such over-abundance of X-Ray emission. This project offers a framework of efficient, automated processing techniques to "clean" images of noise from the mechanics of the telescope, background radiation from local sources such as the solar wind, and more distant sources such as background AGN. The galaxy cluster studied in this project contains high levels of contamination due to its line-of-sight position close to the dust- and star-filled arms of the Milky Way galaxy. Rigorous spectral model fitting of the cluster employ multiple parameters dedicated to accounting for these contaminations. The framework created from this analysis technique will provide the opportunity to expand this analysis to any nearby galaxy cluster, such as the Virgo, Coma, and Ophiuchus Clusters. This research should provide significant insight into how matter, both baryonic and dark matter, is distributed throughout diffuse cluster systems, as well as give clues to the origin of the ICM., Comment: Version 1. arXiv admin note: substantial text overlap with arXiv:1008.2393 by other authors