Extreme digitization for ground-based cosmic microwave background experiments

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 viabi...

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Bibliographic Details
Published in:Monthly Notices of the Royal Astronomical Society
Main Authors: Balkenhol, L, Reichardt, CL
Format: Article in Journal/Newspaper
Language:English
Published: OXFORD UNIV PRESS 2019
Subjects:
Online Access:http://hdl.handle.net/11343/227004
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000478053200025&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=d4d813f4571fa7d6246bdc0dfeca3a1c
https://doi.org/10.1093/mnras/stz1497
Description
Summary: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 few bit numbers to address these challenges. Unlike lossless compression, few bit digitisation introduces additional noise into the data. We present a set of one, two, and three bit digitisation schemes and measure the increase in noise in the cosmic microwave background temperature and polarisation power spectra. The digitisation noise is independent of angular scale and is well-described as a constant percentage of the original detector noise. Three bit digitisation increases the map noise level by < 2%, while reducing the data volume by a factor of ten relative to 32-bit oats. Extreme digitisation is a promising strategy for upcoming experiments.