EBEX: A Balloon-Borne Telescope for Measuring Cosmic Microwave Background Polarization

EBEX is a long-duration balloon-borne (LDB) telescope designed to probe polarization signals in the cosmic microwave background (CMB). It is designed to measure or place an upper limit on the inflationary B-mode signal, a signal predicted by inflationary theories to be imprinted on the CMB by gravit...

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Main Author: Chapman, Daniel
Format: Thesis
Language:unknown
Published: Columbia University 2015
Subjects:
Online Access:https://dx.doi.org/10.7916/d87d2sz5
https://academiccommons.columbia.edu/doi/10.7916/D87D2SZ5
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spelling ftdatacite:10.7916/d87d2sz5 2023-05-15T13:32:35+02:00 EBEX: A Balloon-Borne Telescope for Measuring Cosmic Microwave Background Polarization Chapman, Daniel 2015 https://dx.doi.org/10.7916/d87d2sz5 https://academiccommons.columbia.edu/doi/10.7916/D87D2SZ5 unknown Columbia University Physics Astrophysics Theses Text article-journal ScholarlyArticle 2015 ftdatacite https://doi.org/10.7916/d87d2sz5 2021-11-05T12:55:41Z EBEX is a long-duration balloon-borne (LDB) telescope designed to probe polarization signals in the cosmic microwave background (CMB). It is designed to measure or place an upper limit on the inflationary B-mode signal, a signal predicted by inflationary theories to be imprinted on the CMB by gravitational waves, to detect the effects of gravitational lensing on the polarization of the CMB, and to characterize polarized Galactic foreground emission. The payload consists of a pointed gondola that houses the optics, polarimetry, detectors and detector readout systems, as well as the pointing sensors, control motors, telemetry sytems, and data acquisition and flight control computers. Polarimetry is achieved with a rotating half-wave plate and wire grid polarizer. The detectors are sensitive to frequency bands centered on 150, 250, and 410 GHz. EBEX was flown in 2009 from New Mexico as a full system test, and then flown again in December 2012 / January 2013 over Antarctica in a long-duration flight to collect scientific data. In the instrumentation part of this thesis we discuss the pointing sensors and attitude determination algorithms. We also describe the real-time map making software, "QuickLook", that was custom-designed for EBEX. We devote special attention to the design and construction of the primary pointing sensors, the star cameras, and their custom-designed flight software package, "STARS" (the Star Tracking Attitude Reconstruction Software). In the analysis part of this thesis we describe the current status of the post-flight analysis procedure. We discuss the data structures used in analysis and the pipeline stages related to attitude determination and map making. We also discuss a custom-designed software framework called "LEAP" (the LDB EBEX Analysis Pipeline) that supports most of the analysis pipeline stages. Thesis Antarc* Antarctica DataCite Metadata Store (German National Library of Science and Technology)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Physics
Astrophysics
spellingShingle Physics
Astrophysics
Chapman, Daniel
EBEX: A Balloon-Borne Telescope for Measuring Cosmic Microwave Background Polarization
topic_facet Physics
Astrophysics
description EBEX is a long-duration balloon-borne (LDB) telescope designed to probe polarization signals in the cosmic microwave background (CMB). It is designed to measure or place an upper limit on the inflationary B-mode signal, a signal predicted by inflationary theories to be imprinted on the CMB by gravitational waves, to detect the effects of gravitational lensing on the polarization of the CMB, and to characterize polarized Galactic foreground emission. The payload consists of a pointed gondola that houses the optics, polarimetry, detectors and detector readout systems, as well as the pointing sensors, control motors, telemetry sytems, and data acquisition and flight control computers. Polarimetry is achieved with a rotating half-wave plate and wire grid polarizer. The detectors are sensitive to frequency bands centered on 150, 250, and 410 GHz. EBEX was flown in 2009 from New Mexico as a full system test, and then flown again in December 2012 / January 2013 over Antarctica in a long-duration flight to collect scientific data. In the instrumentation part of this thesis we discuss the pointing sensors and attitude determination algorithms. We also describe the real-time map making software, "QuickLook", that was custom-designed for EBEX. We devote special attention to the design and construction of the primary pointing sensors, the star cameras, and their custom-designed flight software package, "STARS" (the Star Tracking Attitude Reconstruction Software). In the analysis part of this thesis we describe the current status of the post-flight analysis procedure. We discuss the data structures used in analysis and the pipeline stages related to attitude determination and map making. We also discuss a custom-designed software framework called "LEAP" (the LDB EBEX Analysis Pipeline) that supports most of the analysis pipeline stages.
format Thesis
author Chapman, Daniel
author_facet Chapman, Daniel
author_sort Chapman, Daniel
title EBEX: A Balloon-Borne Telescope for Measuring Cosmic Microwave Background Polarization
title_short EBEX: A Balloon-Borne Telescope for Measuring Cosmic Microwave Background Polarization
title_full EBEX: A Balloon-Borne Telescope for Measuring Cosmic Microwave Background Polarization
title_fullStr EBEX: A Balloon-Borne Telescope for Measuring Cosmic Microwave Background Polarization
title_full_unstemmed EBEX: A Balloon-Borne Telescope for Measuring Cosmic Microwave Background Polarization
title_sort ebex: a balloon-borne telescope for measuring cosmic microwave background polarization
publisher Columbia University
publishDate 2015
url https://dx.doi.org/10.7916/d87d2sz5
https://academiccommons.columbia.edu/doi/10.7916/D87D2SZ5
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_doi https://doi.org/10.7916/d87d2sz5
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