BICEP/Keck XX: Component-separated maps of polarized CMB and thermal dust emission using Planck and BICEP/Keck Observations through the 2018 Observing Season

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Main Authors: Keck Collaboration, Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, Bischoff, C. A., Beck, D., Bock, J. J., Boenish, H., Buza, V., Cantrall, B., Cheshire IV, J. R., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A. J., Denison, E., Duband, L., Echter, M., Eiben, M., Elwood, B. D., Fatigoni, S., Filippini, J. P., Fortes, A., Gao, M., Giannakopoulos, C., Goeckner-Wald, N., Goldfinger, D. C., Gratton, S., Grayson, J. A., Greathouse, A., Grimes, P. K., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S. A., Henderson, S., Hoang, T. D., Hubmayr, J., Hui, H., Irwin, K. D., Kang, J. H., Karkare, K. S., Kefeli, S., Kovac, J. M., Kuo, C., Lasko, K., Lau, K. K., Lautzenhiser, M., Lennox, A., Liu, T., Mackey, S., Maher, N., Megerian, K. G., Minutolo, L., Moncelsi, L., Nakato, Y., Nguyen, H. T., OBrient, R., Paine, S. N., Patel, A., Petroff, M. A., Polish, A. R., Prouve, T., Pryke, C., Reintsema, C. D., Richter, S., Romand, T., Salatino, M., Schillaci, A., Schmitt, B., Schwartz, R., Sheehy, C. D., Singari, B., Soliman, A., Germaine, T. St., Steiger, A., Steinbach, B., Sudiwala, R., Teply, G., Thompson, K. L., Tucker, C., Turner, A. D., Vergès, C., Vieregg, A. G., Wandui, A., Weber, A. C., Willmert, J., Wong, C. L., Wu, W. L. K., Yang, H., Yu, C., Zheng, L., Zhang, C., Zhang, S.
Format: Preprint
Published: 2025
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author Keck Collaboration
Ade, P. A. R.
Ahmed, Z.
Amiri, M.
Barkats, D.
Thakur, R. Basu
Bischoff, C. A.
Beck, D.
Bock, J. J.
Boenish, H.
Buza, V.
Cantrall, B.
Cheshire IV, J. R.
Connors, J.
Cornelison, J.
Crumrine, M.
Cukierman, A. J.
Denison, E.
Duband, L.
Echter, M.
Eiben, M.
Elwood, B. D.
Fatigoni, S.
Filippini, J. P.
Fortes, A.
Gao, M.
Giannakopoulos, C.
Goeckner-Wald, N.
Goldfinger, D. C.
Gratton, S.
Grayson, J. A.
Greathouse, A.
Grimes, P. K.
Hall, G.
Halal, G.
Halpern, M.
Hand, E.
Harrison, S. A.
Henderson, S.
Hoang, T. D.
Hubmayr, J.
Hui, H.
Irwin, K. D.
Kang, J. H.
Karkare, K. S.
Kefeli, S.
Kovac, J. M.
Kuo, C.
Lasko, K.
Lau, K. K.
Lautzenhiser, M.
Lennox, A.
Liu, T.
Mackey, S.
Maher, N.
Megerian, K. G.
Minutolo, L.
Moncelsi, L.
Nakato, Y.
Nguyen, H. T.
OBrient, R.
Paine, S. N.
Patel, A.
Petroff, M. A.
Polish, A. R.
Prouve, T.
Pryke, C.
Reintsema, C. D.
Richter, S.
Romand, T.
Salatino, M.
Schillaci, A.
Schmitt, B.
Schwartz, R.
Sheehy, C. D.
Singari, B.
Soliman, A.
Germaine, T. St.
Steiger, A.
Steinbach, B.
Sudiwala, R.
Teply, G.
Thompson, K. L.
Tucker, C.
Turner, A. D.
Vergès, C.
Vieregg, A. G.
Wandui, A.
Weber, A. C.
Willmert, J.
Wong, C. L.
Wu, W. L. K.
Yang, H.
Yu, C.
Zheng, L.
Zhang, C.
Zhang, S.
author_facet Keck Collaboration
Ade, P. A. R.
Ahmed, Z.
Amiri, M.
Barkats, D.
Thakur, R. Basu
Bischoff, C. A.
Beck, D.
Bock, J. J.
Boenish, H.
Buza, V.
Cantrall, B.
Cheshire IV, J. R.
Connors, J.
Cornelison, J.
Crumrine, M.
Cukierman, A. J.
Denison, E.
Duband, L.
Echter, M.
Eiben, M.
Elwood, B. D.
Fatigoni, S.
Filippini, J. P.
Fortes, A.
Gao, M.
Giannakopoulos, C.
Goeckner-Wald, N.
Goldfinger, D. C.
Gratton, S.
Grayson, J. A.
Greathouse, A.
Grimes, P. K.
Hall, G.
Halal, G.
Halpern, M.
Hand, E.
Harrison, S. A.
Henderson, S.
Hoang, T. D.
Hubmayr, J.
Hui, H.
Irwin, K. D.
Kang, J. H.
Karkare, K. S.
Kefeli, S.
Kovac, J. M.
Kuo, C.
Lasko, K.
Lau, K. K.
Lautzenhiser, M.
Lennox, A.
Liu, T.
Mackey, S.
Maher, N.
Megerian, K. G.
Minutolo, L.
Moncelsi, L.
Nakato, Y.
Nguyen, H. T.
OBrient, R.
Paine, S. N.
Patel, A.
Petroff, M. A.
Polish, A. R.
Prouve, T.
Pryke, C.
Reintsema, C. D.
Richter, S.
Romand, T.
Salatino, M.
Schillaci, A.
Schmitt, B.
Schwartz, R.
Sheehy, C. D.
Singari, B.
Soliman, A.
Germaine, T. St.
Steiger, A.
Steinbach, B.
Sudiwala, R.
Teply, G.
Thompson, K. L.
Tucker, C.
Turner, A. D.
Vergès, C.
Vieregg, A. G.
Wandui, A.
Weber, A. C.
Willmert, J.
Wong, C. L.
Wu, W. L. K.
Yang, H.
Yu, C.
Zheng, L.
Zhang, C.
Zhang, S.
contents We present component-separated polarization maps of the cosmic microwave background (CMB) and Galactic thermal dust emission, derived using data from the BICEP/Keck experiments through the 2018 observing season and Planck. By employing a maximum-likelihood method that utilizes observing matrices, we produce unbiased maps of the CMB and dust signals. We outline the computational challenges and demonstrate an efficient implementation of the component map estimator. We show methods to compute and characterize power spectra of these maps, opening up an alternative way to infer the tensor-to-scalar ratio from our data. We compare the results of this map-based separation method with the baseline BICEP/Keck analysis. Our analysis demonstrates consistency between the two methods, finding an 84% correlation between the pipelines.
format Preprint
id arxiv_https___arxiv_org_abs_2509_21648
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle BICEP/Keck XX: Component-separated maps of polarized CMB and thermal dust emission using Planck and BICEP/Keck Observations through the 2018 Observing Season
Keck Collaboration
Ade, P. A. R.
Ahmed, Z.
Amiri, M.
Barkats, D.
Thakur, R. Basu
Bischoff, C. A.
Beck, D.
Bock, J. J.
Boenish, H.
Buza, V.
Cantrall, B.
Cheshire IV, J. R.
Connors, J.
Cornelison, J.
Crumrine, M.
Cukierman, A. J.
Denison, E.
Duband, L.
Echter, M.
Eiben, M.
Elwood, B. D.
Fatigoni, S.
Filippini, J. P.
Fortes, A.
Gao, M.
Giannakopoulos, C.
Goeckner-Wald, N.
Goldfinger, D. C.
Gratton, S.
Grayson, J. A.
Greathouse, A.
Grimes, P. K.
Hall, G.
Halal, G.
Halpern, M.
Hand, E.
Harrison, S. A.
Henderson, S.
Hoang, T. D.
Hubmayr, J.
Hui, H.
Irwin, K. D.
Kang, J. H.
Karkare, K. S.
Kefeli, S.
Kovac, J. M.
Kuo, C.
Lasko, K.
Lau, K. K.
Lautzenhiser, M.
Lennox, A.
Liu, T.
Mackey, S.
Maher, N.
Megerian, K. G.
Minutolo, L.
Moncelsi, L.
Nakato, Y.
Nguyen, H. T.
OBrient, R.
Paine, S. N.
Patel, A.
Petroff, M. A.
Polish, A. R.
Prouve, T.
Pryke, C.
Reintsema, C. D.
Richter, S.
Romand, T.
Salatino, M.
Schillaci, A.
Schmitt, B.
Schwartz, R.
Sheehy, C. D.
Singari, B.
Soliman, A.
Germaine, T. St.
Steiger, A.
Steinbach, B.
Sudiwala, R.
Teply, G.
Thompson, K. L.
Tucker, C.
Turner, A. D.
Vergès, C.
Vieregg, A. G.
Wandui, A.
Weber, A. C.
Willmert, J.
Wong, C. L.
Wu, W. L. K.
Yang, H.
Yu, C.
Zheng, L.
Zhang, C.
Zhang, S.
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
We present component-separated polarization maps of the cosmic microwave background (CMB) and Galactic thermal dust emission, derived using data from the BICEP/Keck experiments through the 2018 observing season and Planck. By employing a maximum-likelihood method that utilizes observing matrices, we produce unbiased maps of the CMB and dust signals. We outline the computational challenges and demonstrate an efficient implementation of the component map estimator. We show methods to compute and characterize power spectra of these maps, opening up an alternative way to infer the tensor-to-scalar ratio from our data. We compare the results of this map-based separation method with the baseline BICEP/Keck analysis. Our analysis demonstrates consistency between the two methods, finding an 84% correlation between the pipelines.
title BICEP/Keck XX: Component-separated maps of polarized CMB and thermal dust emission using Planck and BICEP/Keck Observations through the 2018 Observing Season
topic Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2509.21648