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1by Araujo, D. C., Ade, P. A. R., Bond, J. R., Bradford, K. J., Chapman, D., Che, G., Day, P. K., Didier, J., Doyle, S., Eriksen, H. K., Flanigan, D., Groppi, C. E., Hillbrand, S. N., Johnson, B. R., Jones, G., Limon, M., Miller, A. D., Mauskopf, P., McCarrick, H., Mroczkowski, T., Reichborn-Kjennerud, B., Smiley, B., Sobrin, J., Wehus, I. K., Zmuidzinas, J.Subjects: “...half-wave plate...”
Published in SPIE Proceedings, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII (2014)
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2by Araujo, D. C., Ade, P. A. R., Bond, J. R., Bradford, K. J., Chapman, D., Che, G., Day, P. K., Didier, J., Doyle, S., Eriksen, H. K., Flanigan, D., Groppi, C. E., Hillbrand, S. N., Johnson, B. R., Jones, G., Limon, M., Miller, A. D., Mauskopf, P., McCarrick, H., Mroczkowski, T., Reichborn-Kjennerud, B., Smiley, B., Sobrin, J., Wehus, I. K., Zmuidzinas, J.“... millimeter-wave polarimeter, tailored for observing the cosmic microwave background (CMB), to Isi Station...”
Published 2014
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3by 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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4by Reichborn-Kjennerud, B., Aboobaker, Asad, 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., 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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5by Reichborn-Kjennerud, B., Aboobaker, Asad, 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., 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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6by 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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7by 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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8by 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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9by 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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10by 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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11by 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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12by 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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