Taurus is a balloon-borne cosmic microwave background (CMB) experiment optimized to map the \(E\)-mode polarization and Galactic foregrounds at the largest angular scales (\(\ell <\) 30) and improve measurements of the optical depth to reionization (\(\tau\)). This will pave the way for improved measurements of the sum of neutrino masses in combination with high-resolution CMB data as well as test the \(\Lambda\)CDM model on large angular scales while also providing high-frequency maps of polarized dust foregrounds to the CMB community. These measurements take advantage of the low-loading environment found in the stratosphere and are enabled by a mid-latitude launch location (Wanaka, NZ), which provides access to 70\% of the sky from NASA’s super-pressure balloon platform. Taurus will employ more than 10,000 100~mK transition edge sensor bolometers distributed across two low-frequency (150, 220 GHz) and one high-frequency (280, 350 GHz) dichroic receivers. The instrument and scan strategy are designed for rigorous control of instrumental systematics, enabling high-fidelity linear polarization measurements on the largest angular scales. The liquid helium cryostat housing the detectors and optics is supported by a lightweight gondola. The payload is designed to meet the challenges in mass, power, and thermal control posed by the super-pressure platform. Here we describe a general overview of Taurus, with an emphasis on the instrument design.
A model of the Taurus payload. A rigid truss structure provides support for the cryostat, electronics, and SPB launch provider components, which include the Support Instrumentation Package (SIP), the SIP solar arrays, and antenna boom. The payload sunshielding and thermal treatments are not drawn in order to more clearly show the main sub-systems.
May, J. L., Adler, A. E., Austermann, J. E., Benton, S. J., Bihary, R., Durkin, M., … & Vissers, M. R. (2024, August). Instrument overview of Taurus: a balloon-borne CMB and dust polarization experiment. In Ground-based and Airborne Telescopes X (Vol. 13094, pp. 1296-1310). SPIE.
arXivTartakovsky, S., Adler, A. E., Austermann, J. E., Benton, S. J., Bihary, R., Durkin, M., … & Vissers, M. R. (2024, August). Thermal architecture for a cryogenic super-pressure balloon payload: design and development of the Taurus flight cryostat. In Ground-based and Airborne Telescopes X (Vol. 13094, pp. 1693-1701). SPIE.
arXivAdler, A. E., Austermann, J. E., Benton, S. J., Duff, S. M., Filippini, J. P., Fraisse, A. A., … & Vissers, M. R. (2024). Modeling optical systematics for the Taurus CMB experiment. arXiv preprint arXiv:2406.11992.
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Hi I am Simon and I like tau
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