The Astrophysical Journal (Jan 2025)

A Measurement of the Largest-scale CMB E-mode Polarization with CLASS

  • Yunyang Li,
  • Joseph R. Eimer,
  • John W. Appel,
  • Charles L. Bennett,
  • Michael K. Brewer,
  • Sarah Marie Bruno,
  • Ricardo Bustos,
  • Carol Yan Yan Chan,
  • David T. Chuss,
  • Joseph Cleary,
  • Sumit Dahal,
  • Rahul Datta,
  • Jullianna Denes Couto,
  • Kevin L. Denis,
  • Rolando Dünner,
  • Thomas Essinger-Hileman,
  • Kathleen Harrington,
  • Kyle Helson,
  • Johannes Hubmayr,
  • Jeffrey Iuliano,
  • John Karakla,
  • Tobias A. Marriage,
  • Nathan J. Miller,
  • Carolina Morales Perez,
  • Lucas P. Parker,
  • Matthew A. Petroff,
  • Rodrigo A. Reeves,
  • Karwan Rostem,
  • Caleigh Ryan,
  • Rui Shi,
  • Koji Shukawa,
  • Deniz A. N. Valle,
  • Duncan J. Watts,
  • Janet L. Weiland,
  • Edward J. Wollack,
  • Zhilei Xu,
  • Lingzhen Zeng

DOI
https://doi.org/10.3847/1538-4357/adc723
Journal volume & issue
Vol. 986, no. 2
p. 111

Abstract

Read online

We present measurements of large-scale cosmic microwave background E -mode polarization from the Cosmology Large Angular Scale Surveyor 90 GHz data. Using 115 det-yr of observations collected through 2024 with a variable-delay polarization modulator, we achieved a polarization sensitivity of $82\,\mu {\rm{K}}\,{\rm{arcmin}}$ , comparable to Planck at similar frequencies (100 and 143 GHz ). The analysis demonstrates effective mitigation of systematic errors and addresses challenges to large-angular-scale power recovery posed by time-domain filtering in maximum-likelihood map-making. A novel implementation of the pixel-space transfer matrix is introduced, which enables efficient filtering simulations and bias correction in the power spectrum using the quadratic cross-spectrum estimator. Overall, we achieved an unbiased time-domain filtering correction to recover the largest angular scale polarization, with the only power deficit, arising from map-making nonlinearity, being characterized as 30), our results, both independently and in cross-correlation with Planck, remain fully consistent with Planck’s measurements.

Keywords