Observing low elevation sky and the CMB Cold Spot with BICEP3 at the South Pole
BICEP3 is a 520 mm aperture on-axis refracting telescope at the South Pole, which observes the polarization of the cosmic microwave background (CMB) at 95 GHz to search for the B-mode signal from inflationary gravitational waves. In addition to this main target, we have developed a low-elevation obs...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Other Authors: | , |
Format: | Book Part |
Language: | English |
Published: |
Society of Photo-Optical Instrumentation Engineers (SPIE)
2020
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Subjects: | |
Online Access: | https://authors.library.caltech.edu/107250/ https://authors.library.caltech.edu/107250/1/114532D.pdf https://authors.library.caltech.edu/107250/5/SPIE-AS20-c7f7b295-ef05-ea11-813b-005056be78dc.pdf https://authors.library.caltech.edu/107250/2/2012.09363.pdf https://resolver.caltech.edu/CaltechAUTHORS:20201222-083041699 |
Summary: | BICEP3 is a 520 mm aperture on-axis refracting telescope at the South Pole, which observes the polarization of the cosmic microwave background (CMB) at 95 GHz to search for the B-mode signal from inflationary gravitational waves. In addition to this main target, we have developed a low-elevation observation strategy to extend coverage of the Southern sky at the South Pole, where BICEP3 can quickly achieve degree-scale E-mode measurements over a large area. An interesting E-mode measurement is probing a potential polarization anomaly around the CMB Cold Spot. During the austral summer seasons of 2018-19 and 2019-20, BICEP3 observed the sky with a flat mirror to redirect the beams to various low elevation ranges. The preliminary data analysis shows degree-scale E-modes measured with high signal-to-noise ratio. |
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