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1by Reichborn-Kjennerud, B., Aboobaker, Asad, M., Ade, P., Aubin, F., Baccigalupi, C., Bao, C., Borrill, J., Cantalupo, C., Chapman, D., Didier, J., Dobbs, M., Grain, J., Grainger, W., Hanany, S., Hillbrand, S., Hubmayr, J., Jaffe, A., Johnson, B., Jones, T., Kisner, T., Klein, J., Korotkov, A., Leach, S., Lee, A., Levinson, L., Limon, M., Macdermid, K., Matsumura, T., Meng, X., Miller, A., J., Milligan, M., Pascale, E., Polsgrove, D., Ponthieu, N., Raach, K., Sagiv, I., Smecher, G., Stivoli, F., Stompor, Radek, Tran, H., Tristram, M., Tucker, G. S., Vinokurov, Y., Yadav, A., Zaldarriaga, M., Zilic, K.“... foreground signals from dust. The polarized sky signals will be modulated with an achromatic half wave plate...”
Published in SPIE Proceedings, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V (2010)
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