Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz

• Published in: arXiv.org 2019-11
• Main Authors: Padilla, Ivan L, Eimer, Joseph R, Li, Yunyang, Addison, Graeme E, Ali, Aamir, Appel, John W, Bennett, Charles L, Bustos, Ricardo, Brewer, Michael K, Chan, Manwei, Chuss, David T, Cleary, Joseph, Couto, Jullianna, Dahal, Sumit, Denis, Kevin, Dünner, Rolando, Essinger-Hileman, Thomas, Fluxá, Pedro, Haridas, Saianeesh K, Harrington, Kathleen, Iuliano, Jeffrey, Karakla, John, Marriage, Tobias A, Miller, Nathan J, Núñez, Carolina, Parker, Lucas, Petroff, Matthew A, Reeves, Rodrigo, Karwan Rostem, Stevens, Robert W, Nunes Valle, Deniz Augusto, Watts, Duncan J, Weiland, Janet L, Wollack, Edward J, Xu, Zhilei
• Format: Article
• Language: English
• Subjects: Big Bang theory; Circular polarization; Cosmic microwave background; Cosmology; Dipoles; Linear polarization; Multipoles; Polarimeters; Sky surveys (astronomy)
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.1911.00391

We report circular polarization measurements from the first two years of observation with the 40 GHz polarimeter of the Cosmology Large Angular Scale Surveyor (CLASS). CLASS is conducting a multi-frequency survey covering 75% of the sky from the Atacama Desert designed to measure the cosmic microwave background (CMB) linear E and B polarization on angular scales \(1^\circ \lesssim \theta \leq 90^\circ\), corresponding to a multipole range of \(2 \leq \ell \lesssim 200\). The modulation technology enabling measurements of linear polarization at the largest angular scales from the ground, the Variable-delay Polarization Modulator, is uniquely designed to provide explicit sensitivity to circular polarization (Stokes \(V\)). We present a first detection of circularly polarized atmospheric emission at 40 GHz that is well described by a dipole with an amplitude of \(124\pm4\,\mathrm{\mu K}\) when observed at an elevation of \(45^\circ\), and discuss its potential impact as a foreground to CMB experiments. Filtering the atmospheric component, CLASS places a 95% C.L. upper limit of \(0.4\,\mathrm{\mu K}^2\) to \(13.5\,\mathrm{\mu K}^2\) on \(\ell(\ell+1)C_\ell^{VV}/(2\pi)\) between \(1 \leq \ell \leq 120\), representing a two-orders-of-magnitude improvement over previous limits.