Results 101 to 110 of about 6,477 (211)
New Measurements of Fine-Scale CMB Polarization Power Spectra from
CAPMAP at Both 40 and 90 GHz
, 2008 We present new measurements of the cosmic microwave background (CMB)
polarization from the final season of the Cosmic Anisotropy Polarization MAPper
(CAPMAP). The data set was obtained in winter 2004-2005 with the 7 m antenna in
Crawford Hill, New Jersey,B. Winstein, C. Bischoff, Chu T. S., D. Barkats, D. Samtleben, G. W. Nixon, Haslam C. G. T., J. J. McMahon, J. O. Gundersen, K. M. Smith, K. Vanderlinde, L. Hyatt, M. M. Hedman, P. Farese, S. T. Staggs, T. Gaier +15 morecore +1 more sourceChip-scale, full-Stokes polarimeter
Optics Express, 2019 The polarization of light conveys unique information that can be exploited by crucial applications. The bulky and costly discrete optical components used in conventional polarimeters limit their broad adoption. A compact, low-cost polarimeter would bring this functionality into a myriad of new scenarios and revolutionize its exploitation.Zhongjin Lin, Leslie Rusch, Yuxuan Chen, Wei Shi +3 moreopenaire +3 more sourcesPolarimetry from the Ground Up
, 2007 Ground-based solar polarimetry has made great progress over the last decade.
Nevertheless, polarimetry is still an afterthought in most telescope and
instrument designs, and most polarimeters are designed based on experience and
rules of thumb rather ...Keller, C. U., Snik, F.core +1 more sourceStellar Polarimetry: Where Are We and Where Are We Going?
, 2012 On the final day of the Stellar Polarimetry conference, participants split up
into three "breakout sessions" to discuss the future of the field in the areas
of instrumentation, upcoming opportunities, and community priorities.Brown, John C., Hoffman, Jennifer L., Nordsieck, Kenneth, St-Louis, Nicole, Wade, Gregg +4 morecore +1 more sourceDesign and Performance of a 30/40 GHz Diplexed Focal Plane for the BICEP Array
The Astrophysical Journal Supplement SeriesWe demonstrate a wideband diplexed focal plane suitable for observing low-frequency foregrounds that are important for cosmic microwave background polarimetry.Corwin Shiu, Ahmed Soliman, Roger O’Brient, Bryan Steinbach, James J. Bock, Clifford F. Frez, William C. Jones, Krikor. G. Megerian, Lorenzo Moncelsi, Alessandro Schillaci, Anthony D. Turner, Alexis C. Weber, Cheng Zhang, Silvia Zhang +13 moredoaj +1 more sourceStatus of the RHIC Spin Program
, 2004 The Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory
has been developing the capability of accelerating, storing and colliding
high-energy polarized proton beams over the past several years.Bland, L. C.core +2 more sourcesInclusive cross section and double helicity asymmetry for \pi^0
production in p+p collisions at sqrt(s)=200 GeV: Implications for the
polarized gluon distribution in the proton
, 2007 The PHENIX experiment presents results from the RHIC 2005 run with polarized
proton collisions at sqrt(s)=200 GeV, for inclusive \pi^0 production at
mid-rapidity.Adare, A., Afanasiev, S., Aidala, C., Ajitanand, N.N., Akiba, Y., Al-Bataineh, H., Alexander, J., Aoki, K., Aphecetche, Laurent, Armendariz, R., Aronson, S.H., Asai, J., Atomssa, E. T., Averbeck, R., Awes, T.C., Azmoun, B., Babintsev, V., Baksay, G., Baksay, L., Baldisseri, A., Barish, K.N., Barnes, P.D., Bassalleck, B., Bathe, S., Batsouli, S., Baublis, V., Bazilevsky, A., Belikov, S., Bennett, R., Berdnikov, Y., Bickley, A.A., Boissevain, J.G., Borel, H., Boyle, K., Brooks, M.L., Buesching, H., Bumazhnov, V., Bunce, G., Butsyk, S., Campbell, S., Chang, B.S., Charvet, J.-L., Chernichenko, S., Chi, C.Y., Chiba, J., Chiu, M., Choi, I.J., Chujo, T., Chung, P., Churyn, A., Cianciolo, V., Cleven, C.R., Cole, B.A., Comets, M.P., Constantin, P., Csanad, M., Csörgö, T., D'Enterria, D., Dahms, T., Das, K., David, G., Deaton, M.B., Dehmelt, K., Delagrange, H., Denisov, A., Deshpande, A., Desmond, E.J., Dietzsch, O., Dion, A., Donadelli, M., Drapier, O., Drees, A., Dubey, A.K., Durum, A., Dzhordzhadze, V., Efremenko, Y.V., Egdemir, J., Ellinghaus, F., Emam, W.S., En'Yo, H., Enokizono, A., Esumi, S., Eyser, K.O., Fields, D.E., Finger Jr., M., Finger, M., Fleuret, F., Fokin, S.L., Fraenkel, Z., Frantz, J.E., Franz, A., Frawley, A.D., Fujiwara, K., Fukao, Y., Fusayasu, T., Gadrat, S., Garishvili, I., Glenn, A., Gong, H., Gonin, M., Gosset, J., Goto, Y., Granier De Cassagnac, R., Grau, N., Greene, S.V., Grosse Perdekamp, M., Gunji, T., Gustafsson, H.-A., Hachiya, T., Hadj Henni, A., Haegemann, C., Haggerty, J.S., Hamagaki, H., Han, R., Harada, H., Hartouni, E.P., Haruna, K., Haslum, E., Hayano, R., He, X., Heffner, M., Hemmick, T.K., Hester, T., Hiejima, H., Hill, J.C., Hobbs, R., Hohlmann, M., Holzmann, W., Homma, K., Hong, B., Horaguchi, T., Hornback, D., Ichihara, T., Imai, K., Inaba, M., Inoue, Y., Isenhower, D., Isenhower, L., Ishihara, M., Isobe, T., Issah, M., Isupov, A., Jacak, B.V., Jia, J., Jin, J., Jinnouchi, O., Johnson, B.M., Joo, K.S., Jouan, D., Kajihara, F., Kametani, S., Kamihara, N., Kamin, J., Kaneta, M., Kang, J.H., Kanou, H., Kawall, D., Kazantsev, A.V., Khanzadeev, A., Kikuchi, J., Kim, D.H., Kim, D.J., Kim, E., Kinney, E., Kiss, A., Kistenev, E., Kiyomichi, A., Klay, J., Klein-Boesing, C., Kochenda, L., Kochetkov, V., Komkov, B., Konno, M., Kotchetkov, D., Kozlov, A., Kral, A., Kravitz, A., Kubart, J., Kunde, G.J., Kurihara, N., Kurita, K., Kweon, M.J., Kwon, Y., Kyle, G.S., Lacey, R., Lai, Y.-S., Lajoie, J.G., Lebedev, A.,, Lee, D.M., Lee, M.K., Lee, T., Leitch, M.J., Leite, M.A.L., Lenzi, B., Li, Xiaojian, Liska, T., Litvinenko, A., Liu, M.X., Love, B., Lynch, D., Maguire, C.F., Makdisi, Y.I., Malakhov, A., Malik, M.D., Manko, V.I., Mao, Y., Masek, L., Masui, H., Matathias, F., Mccumber, M., McGaughey, P.L., Miake, Y., Mikes, P., Miki, K., Miller, T.E., Milov, A., Mioduszewski, S., Mishra, M., Mitchell, J.T., Mitrovski, M., Morreale, A., Morrison, D.P., Moukhanova, T.V., Mukhopadhyay, D., Murata, J., Nagamiya, S., Nagata, Y., Nagle, J.L., Naglis, M., Nakagawa, I., Nakamiya, Y., Nakamura, T., Nakano, K., Newby, J., Nguyen, M., Norman, B.E., Nyanin, A.S., O'Brien, E., Oda, S.X., Ogilvie, C.A., Ohnishi, H., Oka, M., Okada, H., Okada, K., Omiwade, O.O., Oskarsson, A., Ouchida, M., Ozawa, K., Pak, R., Pal, D., Palounek, A.P.T., Pantuev, V., Papavassiliou, V., Park, J., Park, W.J., Pate, S.F., Pei, H., Peng, J.-C., Pereira, H., Peresedov, V., Peressounko, D.Yu., Pinkenburg, C., Purschke, M.L., Purwar, A.K., Qu, H., Rak, J., Rakotozafindrabe, A., Ravinovich, I., Read, K.F., Rembeczki, S., Reuter, M., Reygers, K., Riabov, V., Riabov, Y., Roche, G., Romana, A., Rosati, M., Rosendahl, S.S.E., Rosnet, P., Rukoyatkin, P., Rykov, V.L., Sahlmueller, B., Saito, N., Sakaguchi, T., Sakai, S., Sakata, H., Samsonov, V., Sato, S., Sawada, S., Seele, J., Seidl, R., Semenov, V., Seto, R., Sharma, D., Shein, I., Shevel, A., Shibata, T.-A., Shigaki, K., Shimomura, M., Shoji, K., Sickles, A., Silva, C.L., Silvermyr, D., Silvestre, C., Sim, K.S., Singh, C.P., Singh, V., Skutnik, S., Slunecka, M., Soldatov, A., Soltz, R.A., Sondheim, W.E., Sorensen, S.P., Sourikova, I.V., Staley, F., Stankus, P.W., Stenlund, E., Stepanov, M., Ster, A., Stoll, S.P., Sugitate, T., Suire, C., Sziklai, J., Tabaru, T., Takagi, S., Takagui, E.M., Taketani, A., Tanaka, Y., Tanida, K., Tannenbaum, M.J., Taranenko, A., Tarjan, P., Thomas, T.L., Togawa, M., Toia, A., Tojo, J., Tomasek, L., Torii, H., Towell, R.S., Tram, V.-N., Tserruya, I., Tsuchimoto, Y., Vale, C., Valle, H., Van Hecke, H.W., Velkovska, J., Vertesi, R., Vinogradov, A.A., Virius, M., Vrba, V., Vznuzdaev, E., Wagner, M., Walker, D., Wang, X.R., Watanabe, Y., Wessels, J., White, S.N., Winter, D., Woody, C.L., Wysocki, M., Xie, W., Yamaguchi, Y., Yanovich, A., Yasin, Z., Ying, J., Yokkaichi, S., Young, G.R., Younus, I., Yushmanov, I.E., Zajc, W.A., Zaudtke, O., Zhang, C., Zhou, S., Zimanyi, J., Zolin, L. +374 morecore +3 more sourcesPolarization of stars with debris disks: comparing observations with
models
, 2019 The $Herschel$ Space telescope carried out an unprecedented survey of nearby
stars for debris disks. The dust present in these debris disks scatters and
polarizes stellar light in the visible part of the spectrum.Augereau, Jean-Charles, Bastien, Pierre, Simon, Amélie, Storer, Émilie, Vandeportal, Julien +4 morecore +3 more sources