Search Results - "Ruhl, J.E."

Neutrino physics from the cosmic microwave background and large scale structure by Abazajian, K.N., Arnold, K., Austermann, J., Benson, B.A., Bischoff, C., Bock, J., Bond, J.R., Borrill, J., Calabrese, E., Carlstrom, J.E., Carvalho, C.S., Chang, C.L., Chiang, H.C., Church, S., Cooray, A., Crawford, T.M., Dawson, K.S., Das, S., Devlin, M.J., Dobbs, M., Dodelson, S., Doré, O., Dunkley, J., Errard, J., Fraisse, A., Gallicchio, J., Halverson, N.W., Hanany, S., Hildebrandt, S.R., Hincks, A., Hlozek, R., Holder, G., Holzapfel, W.L., Honscheid, K., Hu, W., Hubmayr, J., Irwin, K., Jones, W.C., Kamionkowski, M., Keating, B., Keisler, R., Knox, L., Komatsu, E., Kovac, J., Kuo, C.-L., Lawrence, C., Lee, A.T., Leitch, E., Linder, E., Lubin, P., McMahon, J., Miller, A., Newburgh, L., Niemack, M.D., Nguyen, H., Nguyen, H.T., Page, L., Pryke, C., Reichardt, C.L., Ruhl, J.E., Sehgal, N., Seljak, U., Sievers, J., Silverstein, E., Slosar, A., Smith, K.M., Spergel, D., Staggs, S.T., Stark, A., Stompor, R., Vieregg, A.G., Wang, G., Watson, S., Wollack, E.J., Wu, W.L.K., Yoon, K.W., Zahn, O.

“…This is a report on the status and prospects of the quantification of neutrino properties through the cosmological neutrino background for the Cosmic Frontier…”
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Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck by Sánchez, J, Omori, Y, Chang, C, Bleem, L.E, Drlica-Wagner, A, Raghunathan, S, Zacharegkas, G, Abbott, T.M.C, Aguena, M, Alarcon, A, Alves, O, Baxter, E, Bechtol, K, Benson, B.A, Bernstein, G.M, Bocquet, S, Brooks, D, Burke, D.L, Campos, A, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Cawthon, R, Chang, C.L, Chen, A, Choi, A, Chown, R, Crites, A.T, Pereira, M.E.S, de Haan, T, De Vicente, J, DeRose, J, Desai, S, Diehl, H.T, Dobbs, M.A, Dodelson, S, Elvin-Poole, J, Everett, W, Ferrero, Ismael, Flaugher, B, Fosalba, P, Frieman, J, García-Bellido, J, Gatti, M, George, E.M, Gerdes, D.W, Giannini, G, Gruen, D, Gruendl, R.A, Gschwend, J, Gutierrez, G, Hinton, S.R, Holzapfel, W.L, Honscheid, K, James, D.J, Knox, L, Kuropatkin, N, Lahav, O, Luong-Van, D, Marshall, J.L, McCullough, J, Melchior, P, Mena-Fernández, J, Miquel, R, Mohr, J.J, Muir, J, Myles, J, Natoli, T, Padin, S, Palmese, A, Pandey, S, Paz-Chinchón, F, Pieres, A, Plazas Malagón, A.A, Porredon, A, Pryke, C, Raveri, M, Rodriguez-Monroy, M, Ross, A.J, Ruhl, J.E, Rykoff, E, Sánchez, C, Sanchez, E, Scarpine, V, Schaffer, K.K, Sevilla-Noarbe, I, Sheldon, E, Smith, M, Soares-Santos, M, Staniszewski, Z, Suchyta, E, Swanson, Molly E. C, Tarle, G, Thomas, D, Troxel, M.A, Tucker, D.L, Vieira, J.D, Vincenzi, M, Weaverdyck, N, Yanny, B

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The thermal design, characterization, and performance of the S pider long-duration balloon cryostat by Gudmundsson, J.E., Ade, P.A.R., Amiri, M., Benton, S.J., Bock, J.J., Bond, J.R., Bryan, S.A., Chiang, H.C., Contaldi, C.R., Crill, B.P., Dore, O., Filippini, J.P., Fraisse, A.A., Gambrel, A., Gandilo, N.N., Hasselfield, M., Halpern, M., Hilton, G., Holmes, W., Hristov, V.V., Irwin, K.D., Jones, W.C., Kermish, Z., MacTavish, C.J., Mason, P.V., Megerian, K., Moncelsi, L., Montroy, T.E., Morford, T.A., Nagy, J.M., Netterfield, C.B., Rahlin, A.S., Reintsema, C.D., Ruhl, J.E., Runyan, M.C., Shariff, J.A., Soler, J.D., Trangsrud, A., Tucker, C., Tucker, R.S., Turner, A.D., Wiebe, D.V., Young, E.

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A Measurement of Ω from the North American Test Flight of Boomerang by Melchiorri, A, Ade, P. A. R, de Bernardis, P, Bock, J. J, Borrill, J, Boscaleri, A, Crill, B. P, De Troia, G, Farese, P, Ferreira, P. G, Ganga, K, de Gasperis, G, Giacometti, M, Hristov, V. V, Jaffe, A. H, Lange, A. E, Masi, S, Mauskopf, P. D, Miglio, L, Netterfield, C. B, Pascale, E, Piacentini, F, Romeo, G, Ruhl, J. E, Vittorio, N

“…We use the angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, to constrain…”
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Measurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American Test Flight of Boomerang by Mauskopf, P. D, Ade, P. A. R, de Bernardis, P, Bock, J. J, Borrill, J, Boscaleri, A, Crill, B. P, DeGasperis, G, De Troia, G, Farese, P, Ferreira, P. G, Ganga, K, Giacometti, M, Hanany, S, Hristov, V. V, Iacoangeli, A, Jaffe, A. H, Lange, A. E, Lee, A. T, Masi, S, Melchiorri, A, Melchiorri, F, Miglio, L, Montroy, T, Netterfield, C. B, Pascale, E, Piacentini, F, Richards, P. L, Romeo, G, Ruhl, J. E, Scannapieco, E, Scaramuzzi, F, Stompor, R, Vittorio, N

“…We describe a measurement of the angular power spectrum of anisotropies in the cosmic microwave background (CMB) at scales of 0 3 to 5 degrees from the North…”
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The BOOMERanG experiment and the curvature of the universe by Masi, S., De Bernardis, P., De Troia, G., Giacometti, M., Iacoangeli, A., Piacentini, F., Polenta, G., Ade, P.A.R., Mauskopf, P.D., Bock, J.J., Bond, J.R., Contaldi, C.R., Pogosyan, D., Prunet, S., Borrill, J., Boscaleri, A., Pascale, E., Coble, K., Farese, P., Montroy, T., Ruhl, J.E., Crill, B.P., Hristov, V.V., Jones, W.C., Lange, A.E., Mason, P., De Gasperis, G., Natoli, P., Ganga, K., Hivon, E., Vittorio, N., Jaffe, A.H., Martinis, L., Scaramuzzi, F., Melchiorri, A., Netterfield, C.B., Pongetti, F., Romeo, G.

“…We describe the BOOMERanG experiment and its main result, i.e. the measurement of the large scale curvature of the Universe. BOOMERanG is a balloon-borne…”
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A MEASUREMENT OF THE ANGULAR POWER SPECTRUM OF THE CMB TEMPERATUREANISOTROPY FROM THE 2003 FLIGHT OF Boomerang by Jones, W.C., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis,P., De Gasperis, G., de Oliveira-Costa, A., De Troia, G., Di Stefano, G., Hivon, E., Jaffe, A.H., Kisner, T.S., Lange, A.E., MacTavish, C.J., Masi,S., Mauskopf, P.D., Melchiorri, A., Montroy, T.E., Natoli, P., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta,G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Veneziani, M., Vittorio, N.

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Observations of the temperature and polarization anisotropies with Boomerang 2003 by Jones, W.C., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., De Gasperis, G., de Oliveira-Costa, A., De Troia, G., Di Stefano, G., Hivon, E., Jaffe, A.H., Kisner, T.S., Lange, A.E., MacTavish, C.J., Masi, S., Mauskopf, P.D., Melchiorri, A., Montroy, T.E., Natoli, P., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Veneziani, M., Vittorio, N.

“…The Boomerang experiment completed its final long duration balloon (LDB) flight over Antarctica in January 2003. The focal plane was upgraded to accommodate…”
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Searching for non-Gaussian signals in the BOOMERanG 2003 CMB map: Preliminary results by De Troia, G., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., de Gasperis, G., de Oliveira-Costa, A., Di Stefano, G., Ferreira, P.G., Hivon, E., Jaffe, A., Kisner, T., Kunz, M., Jones, W.C., Lange, A.E., Masi, S., Mauskopf, P.D., MacTavish, C., Melchiorri, A., Montroy, T., Natoli, P., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Veneziani, M., Vittorio, N.

“…We analyse the 145 GHz temperature map produced from the 2003 flight of BOOMERanG in search for deviations from Gaussianity. We perform a pixel space analysis…”
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The millimeter sky as seen with BOOMERanG by Masi, S., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., De Gasperis, G., De Oliveira-Costa, A., De Troia, G., Di Stefano, G., Ehlers, P., Hivon, E., Hristov, V., Iacoangeli, A., Jaffe, A.H., Jones, W.C., Kisner, T.S., Lange, A.E., MacTavish, C.J., Marini Bettolo, C., Mason, P., Mauskopf, P.D., Montroy, T.E., Nati, F., Nati, L., Natoli, P., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Torbet, E., Veneziani, M., Vittorio, N.

“…BOOMERanG is a balloon-borne, mm-wave scanning telescope, which measured the first images of the CMB with sub-horizon resolution in 1998. In 2003 the…”
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CMB polarization with Boomerang 2003 by Piacentini, F., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., De Gasperis, G., de Oliveira-Costa, A., De Troia, G., Di Stefano, G., Hivon, E., Jaffe, A.H., Kisner, T.S., Jones, W.C., Lange, A.E., Marini-Bettolo, C., Masi, S., Mauskopf, P.D., MacTavish, C.J., Melchiorri, A., Montroy, T.E., Nati, F., Nati, L., Natoli, P., Netterfield, C.B., Pascale, E., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Veneziani, M., Vittorio, N.

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Improved measurement of the angular power spectrum of temperatureanisotropy in the CMB from two new analyses of BOOMERANGobservations by Ruhl, J.E., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Contaldi, C.R., Crill, B.P., de Bernardis, P., de Troia,G., Ganga, K., Giacometti, M., Hivon, E., Hristov, V.V., Iacoangeli, A., Jaffe, A.H., Jones, W.C., Lange, A.E., Masi, S., Mason, P., Mauskopf,P.D., Melchiorri, A., Montroy, T., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S., Romeo, G.

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CMB polarization with B oomerang 2003 by Piacentini, F., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., De Gasperis, G., de Oliveira-Costa, A., De Troia, G., Di Stefano, G., Hivon, E., Jaffe, A.H., Kisner, T.S., Jones, W.C., Lange, A.E., Marini-Bettolo, C., Masi, S., Mauskopf, P.D., MacTavish, C.J., Melchiorri, A., Montroy, T.E., Nati, F., Nati, L., Natoli, P., Netterfield, C.B., Pascale, E., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Veneziani, M., Vittorio, N.

“…This paper reports results from the B oomerang 2003 flights, devoted to the measurement of intensity and polarization of the cosmic microwave background…”
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Measuring CMB polarization with Boomerang by Montroy, T, Ade, P.A.R, Balbi, A, Bock, J.J, Bond, J.R, Borrill, J, Boscaleri, A, Cabella, P, Contaldi, C.R, Crill, B.P, de Bernardis, P, De Gasperis, G, de Oliveira-Costa, A, De Troia, G, di Stefano, G, Ganga, K, Hivon, E, Hristov, V.V, Iacoangeli, A, Jaffe, A.H, Kisner, T.S, Jones, W.C, Lange, A.E, Masi, S, Mauskopf, P.D, MacTavish, C, Melchiorri, A, Nati, F, Natoli, P, Netterfield, C.B, Pascale, E, Piacentini, F, Pogosyan, D, Polenta, G, Prunet, S, Ricciardi, S, Romeo, G, Ruhl, J.E, Torbet, E, Tegmark, M, Vittorio, N

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A measurement of Omega from the North American test flight of Boomerang by Melchiorri, A., Ade, P.A.R., De Bernardis, P., Bock, J.J., Borrill, J., Boscaleri, A., Crill, B.P., De Troia, G., Farese, P., Ferreira, P.G., Ganga, K., de Gasperis, G., Giacometti, M., Hristov, V.V., Jaffe, A.H., Lange, A.E., Masi, S., Mauskopf, P.D., Miglio, L., Netterfield, C.B., Pascale, E., Piacentini, F., Romeo, G., Ruhl, J.E., Vittorio, N.

“…We use the power spectrum of the Cosmic Microwave Background, measured during the North American test flight of the BOOMERANG experiment, to constrain the…”
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Measurement of a peak in the cosmic microwave background power spectrum from the North American test flight of Boomerang by Mauskopf, P.D., Ade, P.A.R., Bock, J.J., Borrill, J., Boscaleri, A., Crill, B.P., de Bernardis, P., DeGasperis, G., De Troia, G., Farese, P., Ferreira, P.G., Ganga, K., Giacometti, M., Hanany, S., Hristov, V.V., Iacoangeli, A., Jaffe, A.H., Lange, A.E., Lee, A.T., Masi, S., Melchiorri, A., Melchiorri, F., Miglio, L., Montroy, T., Netterfield, C.B., Pascale, E., Piacentini, F., Richards, P.L., Romeo, G., Ruhl, J.E., Scannapieco, E., Scaramuzzi, F., Stompor, R., Vittorio, N.

“…We describe a measurement of the angular power spectrum of anisotrophies in the Cosmic Microwave Background (CMB) from 0.2 deg to approx. 10 deg. from the test…”
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Measuring CMB polarization with B oomerang by Montroy, T, Ade, P.A.R, Balbi, A, Bock, J.J, Bond, J.R, Borrill, J, Boscaleri, A, Cabella, P, Contaldi, C.R, Crill, B.P, de Bernardis, P, De Gasperis, G, de Oliveira-Costa, A, De Troia, G, di Stefano, G, Ganga, K, Hivon, E, Hristov, V.V, Iacoangeli, A, Jaffe, A.H, Kisner, T.S, Jones, W.C, Lange, A.E, Masi, S, Mauskopf, P.D, MacTavish, C, Melchiorri, A, Nati, F, Natoli, P, Netterfield, C.B, Pascale, E, Piacentini, F, Pogosyan, D, Polenta, G, Prunet, S, Ricciardi, S, Romeo, G, Ruhl, J.E, Torbet, E, Tegmark, M, Vittorio, N

“…B oomerang is a balloon-borne telescope designed for long duration (LDB) flights around Antarctica. The second LDB flight of B oomerang took place in January…”
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BOOMERANG returns by Mauskopf, P.D., Ade, P.A.R., Balbi, A., Cabella, P., De Gasperis, G., Natoli, P., Vittorio, N., Bock, J.J., Hristov, V.V., Jones, W.C., Lange, A.E., Bond, J.R., Contaldi, C.R., J. Borrill, J., Boscaleri, A., Crill, B.P., de Bernardis, P., De Troia, G., Iacoangeli, A., Masi, S., Melchiorri, A., Nati, F., Piacentini, F., Polenta, G., Ricciardi, S., de Oliveira-Costa, A., Tegmark, M., di Stefano, G., Romeo, G., Ganga, K., Hivon, E., Jaffe, A.H., Ruhl, J.E., Kisner, T.S., Montroy, T., Torbet, E., Mactavish, C., Netterfield, C.B., Pascale, E., Pogosyan, D., Prunet, S.

“…BOOMERANG was one of the first experiments to map large areas of the cosmic microwave background (CMB) with high signal-to-noise during a long duration balloon…”
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Mapping the CMB sky: THE BOOMERanG experiment by de Bernardis, P., Ade, P.A.R., Artusa, R., Bock, J.J., Boscaleri, A., Crill, B.P., De Troia, G., Farese, P.C., Giacometti, M., Hristov, V.V., Iacoangeli, A., Lange, A.E., Lee, A.T., Masi, S., Martinis, L., Mason, P.V., Mauskopf, P.D., Melchiorri, F., Miglio, L., Montroy, T., Netterfield, C.B., Pascale, E., Piacentini, F., Richards, P.L., Ruhl, J.E., Scaramuzzi, F.

“…We describe the BOOMERanG experiment, a stratospheric balloon telescope intended to measure the Cosmic Microwave Background anisotropy at angular scales…”
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Probing primordial non Gaussianity in the BOOMERanG CMB maps: an analysis based on analytical Minkowski functionals by Migliaccio, M., Natoli, P., De Troia, G., Hikage, C., Komatsu, E., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Contaldi, C.R., Crill, B.P., de Bernardis, P., de Gasperis, G., de Oliveira-Costa, A., Di Stefano, G., Hivon, E., Kisner, T.S., Jones, W.C., Lange, A.E., Masi, S., Mauskopf, P.D., MacTavish, C.J., Melchiorri, A., Montroy, T.E., Netterfield, C.B., Pascale, E., Piacentini, F., Polenta, G., Ricciardi, S., Romeo, G., Ruhl, J.E., Tegmark, M., Veneziani, M., Vittorio, N.

“…Minkowski functionals are a powerful tool to constrain the Gaussianity of the Cosmic Microwave Background (CMB). In the limit of a weakly non Gaussian field, a…”
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