Extreme digitization for ground-based cosmic microwave background experiments. Issue 3 (4th June 2019)

• Record Type: Journal Article
• Authors: Balkenhol, L; Reichardt, C L
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 487:Issue 3(2019)
• Page Start: 3279
• Page End: 3287
• Publication Date: 2019-06-04
• Subjects: polarization -- techniques: miscellaneous -- cosmic background radiation; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz1497
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: The large size of the time-ordered data of cosmic microwave background experiments presents challenges for mission planning and data analysis. These issues are particularly significant for Antarctica- and space-based experiments, which depend on satellite links to transmit data. We explore the viability of reducing the time-ordered data to a few bit numbers to address these challenges. Unlike lossless compression, few bit digitization introduces additional noise into the data. We present a set of one, two, and three bit digitization schemes and measure the increase in noise in the cosmic microwave background temperature and polarization power spectra. The digitization noise is independent of angular scale and is well described as a constant percentage of the original detector noise. Three bit digitization increases the map noise level by ${\lt } 2{{\ \rm per\ cent}}$, while reducing the data volume by a factor of 10 relative to 32-bit floats. Extreme digitization is a promising strategy for upcoming experiments.