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EBEX is a balloon-borne telescope designed to measure the polarization of thecosmic microwave background radiation. During its eleven day science flight inthe Austral Summer of 2012, it operated 955 spider-web transition edge sensor(TES) bolometers separated into bands at 150, 250 and 410 GHz. This is thefirst time that an array of TES bolometers has been used on a balloon platformto conduct science observations. Polarization sensitivity was provided by awire grid and continuously rotating half-wave plate. The balloon implementationof the bolometer array and readout electronics presented unique developmentrequirements. Here we present an outline of the readout system, the remotetuning of the bolometers and Superconducting QUantum Interference Device(SQUID) amplifiers, and preliminary current noise of the bolometer array andreadout system.

The performance of the bolometer array and readout system during the 2012/2013 flight of the E and B experiment (EBEX)