Measuring Reionization, Neutrino Mass, and Cosmic Inflation with BFORE
Sean Bryan, Peter Ade, J. Richard Bond, Francois Boulanger, Mark, Devlin, Simon Doyle, Jeffrey Filippini, Laura Fissel, Christopher Groppi,, Gilbert Holder, Johannes Hubmayr, Philip Mauskopf, Jeffrey McMahon, Johanna, Nagy, C. Barth Netterfield, Michael Niemack, Giles Novak

TL;DR
BFORE is a balloon mission designed to measure the cosmic microwave background across large sky areas, aiming to improve understanding of reionization, neutrino mass, and cosmic inflation through advanced multi-frequency observations.
Contribution
It introduces a novel balloon platform for CMB measurements that enhances large-scale data collection and foreground separation, utilizing advanced TES multichroic detectors and microwave readout technologies.
Findings
Improved measurement of optical depth to reionization tau.
Potential detection of primordial gravitational wave B-mode signals at r~0.01.
Enhanced foreground separation and galaxy cluster velocity measurements.
Abstract
BFORE is a NASA high-altitude ultra-long-duration balloon mission proposed to measure the cosmic microwave background (CMB) across half the sky during a 28-day mid-latitude flight launched from Wanaka, New Zealand. With the unique access to large angular scales and high frequencies provided by the balloon platform, BFORE will significantly improve measurements of the optical depth to reionization tau, breaking parameter degeneracies needed for a measurement of neutrino mass with the CMB. The large angular scale data will enable BFORE to hunt for the large-scale gravitational wave B-mode signal, as well as the degree-scale signal, each at the r~0.01 level. The balloon platform allows BFORE to map Galactic dust foregrounds at frequencies where they dominate, in order to robustly separate them from CMB signals measured by BFORE, in addition to complementing data from ground-based…
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