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Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER

P. A. R. Ade,M. Amiri,S. J. Benton,A. S. Bergman,R. Bihary,J. J. Bock,J. R. Bond,J. A. Bonetti,S. A. Bryan,H. C. Chiang,C. R. Contaldi,O. Dore,A. J. Duivenvoorden,H. K. Eriksen,J. P. Filippini,A. A. Fraisse,K. Freese,M. Galloway,A. E. Gambrel,N. N. Gandilo,K. Ganga, S. Gourapura,R. Gualtieri,J. E. Gudmundsson,M. Halpern,J. Hartley,M. Hasselfield,G. Hilton,W. Holmes,V. V. Hristov,Z. Huang,K. D. Irwin,W. C. Jones,A. Karakci,C. L. Kuo,Z. D. Kermish,J. s. -y. Leung, S. Li,D. S. Y. Mak,P. V. Mason,K. Megerian,L. Moncelsi,T. A. Morford,J. M. Nagy,C. B. Netterfield,M. Nolta,R. O'Brient,B. Osherson,I. L. Padilla,B. Racine,A. S. Rahlin,C. Reintsema,J. E. Ruhl,M. C. Runyan,T. M. Ruud,J. A. Shariff,E. C. Shaw,C. Shiu,J. D. Soler,X. Song,A. Trangsrud,C. Tucker,R. S. Tucker,A. D. Turner,J. F. van der List,A. C. Weber,I. K. Wehus,D. V. Wiebe,E. Y. Young, SPIDER Collaboration

ASTROPHYSICAL JOURNAL（2025）

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Key words
Cosmic microwave background radiation,Observational cosmology,Interstellar emissions
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