Observing low elevation sky and the CMB Cold Spot with BICEP3 at the South Pole
Abstract
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.
- Publication:
-
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X
- Pub Date:
- December 2020
- DOI:
- 10.1117/12.2562066
- arXiv:
- arXiv:2012.09363
- Bibcode:
- 2020SPIE11453E..2DK
- Keywords:
-
- Astrophysics - Cosmology and Nongalactic Astrophysics;
- Astrophysics - Instrumentation and Methods for Astrophysics
- E-Print:
- 12 pages, 10 figures