The BigBOSS Experiment

Schelgel, D.; Abdalla, F.; Abraham, T.; Ahn, C.; Allende Prieto, C.; Annis, J.; Aubourg, E.; Azzaro, M.; Bailey, S.; Baltay, C.; Baugh, C.

doi:10.2172/1027233

DOE OSTI · 1027233

The BigBOSS Experiment

Schelgel, D.·Abdalla, F.·Abraham, T.·Ahn, C.·Allende Prieto, C.·Annis, J.·Aubourg, E.·Azzaro, M.·Bailey, S.·Baltay, C.·Baugh, C.

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Abstract

BigBOSS will obtain observational constraints that will bear on three of the four 'science frontier' questions identified by the Astro2010 Cosmology and Fundamental Phyics Panel of the Decadal Survey: Why is the universe accelerating; what is dark matter and what are the properties of neutrinos? Indeed, the BigBOSS project was recommended for substantial immediate R and D support the PASAG report. The second highest ground-based priority from the Astro2010 Decadal Survey was the creation of a funding line within the NSF to support a 'Mid-Scale Innovations' program, and it used BigBOSS as a 'compelling' example for support. This choice was the result of the Decadal Survey's Program Priorization panels reviewing 29 mid-scale projects and recommending BigBOSS 'very highly'.

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72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS 79 ASTRONOMY AND ASTROPHYSICS COSMOLOGY Experiment-HEP NEUTRINOS NONLUMINOUS MATTER UNIVERSE

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BibTeX RIS

Schelgel, D., Abdalla, F., Abraham, T., Ahn, C., Allende Prieto, C., Annis, J., Aubourg, E., Azzaro, M., Bailey, S., Baltay, C., Baugh, C.. 2011-01-01. The BigBOSS Experiment. https://doi.org/10.2172/1027233

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