Zobrazeno 1 - 10
of 132
pro vyhledávání: '"McMahon JJ"'
The aim of the present study was to determine the reliability and differences between three fascicle length (FL) estimation methods when utilizing a 10-cm ultrasound (US) probe. Thirteen males (24.1 ± 3.8 years, 79.3 ± 14 kg, 179 ± 6.6 cm) partici
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a1a350ae864c1954b297eef3590acb6d
The countermovement jump (CMJ) has been suggested to be an important test of neuromuscular performance for rugby league (RL) players. Identifying force platform-derived CMJ variables that may be more applicable to RL positions (e.g., forwards and bac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eae3d5244cd0a9b93cc962e5529fdb34
https://usir.salford.ac.uk/id/eprint/63685/1/PMC8956158.pdf
https://usir.salford.ac.uk/id/eprint/63685/1/PMC8956158.pdf
Autor:
Gupta, N, Reichardt, CL, Ade, PAR, Anderson, AJ, Archipley, M, Austermann, JE, Avva, JS, Beall, JA, Bender, AN, Benson, BA, Bianchini, F, Bleem, LE, Carlstrom, JE, Chang, CL, Chiang, HC, Citron, R, Moran, C Corbett, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Everett, W, Feng, C, Gallicchio, J, George, EM, Gilbert, A, Halverson, NW, Harrington, N, Henning, JW, Hilton, GC, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Huang, N, Hubmayr, J, Irwin, KD, Knox, L, Lee, AT, Li, D, Lowitz, A, Luong-Van, D, Marrone, DP, McMahon, JJ, Meyer, SS, Mocanu, LM, Mohr, JJ, Montgomery, J, Nadolski, A, Natoli, T, Nibarger, JP, Noble, GI, Novosad, V, Padin, S, Patil, S, Pryke, C, Ruhl, JE, Saliwanchik, BR, Sayre, JT, Schaffer, KK, Shirokoff, E, Sievers, C, Smecher, G, Staniszewski, Z, Stark, AA, Story, KT, Switzer, ER, Tucker, C, Vanderlinde, K, Veach, T, Vieira, JD, Wang, G, Whitehorn, N, Williamson, R, Wu, WLK, Yefremenko, V, Zhang, L
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 490, iss 4
We study the polarization properties of extragalactic sources at 95 and 150 GHz in the SPTpol 500 deg2 survey. We estimate the polarized power by stacking maps at known source positions, and correct for noise bias by subtracting the mean polarized po
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::7b38ac5634d657ac4a4158a5a0b77bfc
https://escholarship.org/uc/item/8vt124dx
https://escholarship.org/uc/item/8vt124dx
Autor:
Gupta, N, Reichardt, CL, Ade, PAR, Anderson, AJ, Archipley, M, Austermann, JE, Avva, JS, Beall, JA, Bender, AN, Benson, BA, Bianchini, F, Bleem, LE, Carlstrom, JE, Chang, CL, Chiang, HC, Citron, R, Corbett Moran, C, Crawford, TM, Crites, AT, de Haan, T, Dobbs, MA, Everett, W, Feng, C, Gallicchio, J, George, EM, Gilbert, A, Halverson, NW, Harrington, N, Henning, JW, Hilton, GC, Holder, GP, Holzapfel, WL, Hou, Z, Hrubes, JD, Huang, N, Hubmayr, J, Irwin, KD, Knox, L, Lee, AT, Li, D, Lowitz, A, Luong-Van, D, Marrone, DP, McMahon, JJ, Meyer, SS, Mocanu, LM, Mohr, JJ, Montgomery, J, Nadolski, A, Natoli, T, Nibarger, JP, Noble, GI, Novosad, V, Padin, S, Patil, S, Pryke, C, Ruhl, JE, Saliwanchik, BR, Sayre, JT, Schaffer, KK, Shirokoff, E, Sievers, C, Smecher, G, Staniszewski, Z, Stark, AA, Story, KT, Switzer, ER, Tucker, C, Vanderlinde, K, Veach, T, Vieira, JD, Wang, G, Whitehorn, N, Williamson, R, Wu, WLK, Yefremenko, V, Zhang, L
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 490, iss 4
We study the polarization properties of extragalactic sources at 95 and 150 GHz in the SPTpol 500 deg2 survey. We estimate the polarized power by stacking maps at known source positions, and correct for noise bias by subtracting the mean polarized po
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::bb7a958023a3d67eb41e129ec6c5b75c
https://escholarship.org/uc/item/8vt124dx
https://escholarship.org/uc/item/8vt124dx
Autor:
Raghunathan, S, Patil, S, Baxter, E, Benson, BA, Bleem, LE, Crawford, TM, Holder, GP, McClintock, T, Reichardt, CL, Varga, TN, Whitehorn, N, Ade, PAR, Allam, S, Anderson, AJ, Austermann, JE, Avila, S, Avva, JS, Bacon, D, Beall, JA, Bender, AN, Bianchini, F, Bocquet, S, Brooks, D, Burke, DL, Carlstrom, JE, Carretero, J, Castander, FJ, Chang, CL, Chiang, HC, Citron, R, Costanzi, M, Crites, AT, da Costa, LN, Desai, S, Diehl, HT, Dietrich, JP, Dobbs, MA, Doel, P, Everett, S, Evrard, AE, Feng, C, Flaugher, B, Fosalba, P, Frieman, J, Gallicchio, J, García-Bellido, J, Gaztanaga, E, George, EM, Giannantonio, T, Gilbert, A, Gruendl, RA, Gschwend, J, Gupta, N, Gutierrez, G, de Haan, T, Halverson, NW, Harrington, N, Henning, JW, Hilton, GC, Hollowood, DL, Holzapfel, WL, Honscheid, K, Hrubes, JD, Huang, N, Hubmayr, J, Irwin, KD, Jeltema, T, Kind, M Carrasco, Knox, L, Kuropatkin, N, Lahav, O, Lee, AT, Li, D, Lima, M, Lowitz, A, Maia, MAG, Marshall, JL, McMahon, JJ, Melchior, P, Menanteau, F, Meyer, SS, Miquel, R, Mocanu, LM, Mohr, JJ, Montgomery, J, Moran, C Corbett, Nadolski, A, Natoli, T, Nibarger, JP, Noble, G, Novosad, V, Ogando, RLC, Padin, S, Plazas, AA, Pryke, C, Rapetti, D, Romer, AK, Roodman, A, Rosell, A Carnero, Rozo, E
Publikováno v:
Physical review letters, vol 123, iss 18
We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new estimator that extracts the lensing dipole signature from s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::dba9976bd82f619e0b9ce896a66bfb82
https://escholarship.org/uc/item/3f81n7n1
https://escholarship.org/uc/item/3f81n7n1
Autor:
Prat, J, Baxter, E, Shin, T, Sánchez, C, Chang, C, Jain, B, Miquel, R, Alarcon, A, Bacon, D, Bernstein, GM, Cawthon, R, Crawford, TM, Davis, C, De Vicente, J, Dodelson, S, Eifler, TF, Friedrich, O, Gatti, M, Gruen, D, Hartley, WG, Holder, GP, Hoyle, B, Jarvis, M, Krause, E, MacCrann, N, Mawdsley, B, Nicola, A, Omori, Y, Pujol, A, Rau, MM, Reichardt, CL, Samuroff, S, Sheldon, E, Troxel, MA, Vielzeuf, P, Zuntz, J, Abbott, TMC, Abdalla, FB, Annis, J, Avila, S, Aylor, K, Benson, BA, Bertin, E, Bleem, LE, Brooks, D, Burke, DL, Carlstrom, JE, Carrasco Kind, M, Carretero, J, Chang, CL, Cho, HM, Chown, R, Crites, AT, Cunha, CE, Da Costa, LN, Desai, S, Diehl, HT, Dietrich, JP, Dobbs, MA, Doel, P, Everett, WB, Evrard, AE, Flaugher, B, Fosalba, P, García-Bellido, J, Gaztanaga, E, George, EM, Gerdes, DW, Giannantonio, T, Gruendl, RA, Gschwend, J, Gutierrez, G, De Haan, T, Halverson, NW, Harrington, NL, Holzapfel, WL, Honscheid, K, Hou, Z, Hrubes, JD, James, DJ, Jeltema, T, Knox, L, Kron, R, Kuehn, K, Kuropatkin, N, Lahav, O, Lee, AT, Leitch, EM, Lima, M, Luong-Van, D, Maia, MAG, Manzotti, A, Marrone, DP, Marshall, JL, McMahon, JJ, Melchior, P, Menanteau, F, Meyer, SS, Miller, CJ, Mocanu, LM
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 487, iss 1
Correlations between tracers of the matter density field and gravitational lensing are sensitive to the evolution of the matter power spectrum and the expansion rate across cosmic time. Appropriately defined ratios of such correlation functions, on t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::628d1ba30a31bd596f58245196a92c7f
https://escholarship.org/uc/item/34h3304v
https://escholarship.org/uc/item/34h3304v
Autor:
Raghunathan, S, Patil, S, Baxter, E, Benson, BA, Bleem, LE, Chou, TL, Crawford, TM, Holder, GP, McClintock, T, Reichardt, CL, Rozo, E, Varga, TN, Abbott, TMC, Ade, PAR, Allam, S, Anderson, AJ, Annis, J, Austermann, JE, Avila, S, Beall, JA, Bechtol, K, Bender, AN, Bernstein, G, Bertin, E, Bianchini, F, Brooks, D, Burke, DL, Carlstrom, JE, Carretero, J, Chang, CL, Chiang, HC, Cho, H-M, Citron, R, Crites, AT, Cunha, CE, da Costa, LN, Davis, C, Desai, S, Diehl, HT, Dietrich, JP, Dobbs, MA, Doel, P, Eifler, TF, Everett, W, Evrard, AE, Flaugher, B, Fosalba, P, Frieman, J, Gallicchio, J, García-Bellido, J, Gaztanaga, E, George, EM, Gilbert, A, Gruen, D, Gruendl, RA, Gschwend, J, Gupta, N, Gutierrez, G, de Haan, T, Halverson, NW, Harrington, N, Hartley, WG, Henning, JW, Hilton, GC, Hollowood, DL, Holzapfel, WL, Honscheid, K, Hou, Z, Hoyle, B, Hrubes, JD, Huang, N, Hubmayr, J, Irwin, KD, James, DJ, Jeltema, T, Kim, AG, Kind, M Carrasco, Knox, L, Kovacs, A, Kuehn, K, Kuropatkin, N, Lee, AT, Li, TS, Lima, M, Maia, MAG, Marshall, JL, McMahon, JJ, Melchior, P, Menanteau, F, Meyer, SS, Miller, CJ, Miquel, R, Mocanu, L, Montgomery, J, Nadolski, A, Natoli, T, Nibarger, JP, Novosad, V, Padin, S, Plazas, AA
Publikováno v:
Astrophysical Journal, vol 872, iss 2
The Astrophysical Journal, vol 872, iss 2
The Astrophysical Journal, vol 872, iss 2
We use cosmic microwave background (CMB) temperature maps from the 500 deg 2 SPTpol survey to measure the stacked lensing convergence of galaxy clusters from the Dark Energy Survey (DES) Year-3 redMaPPer (RM) cluster catalog. The lensing signal is ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::ac6aa84428cd8f2a87539dc80e697c71
https://escholarship.org/uc/item/7664b9j2
https://escholarship.org/uc/item/7664b9j2
The aims of this study were to compare the effects of the exclusion or inclusion of the catch phase during power clean (PC) derivatives on force-time characteristics during isometric and dynamic tasks, after two 4-week mesocycles of resistance traini
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::aecc39593d53784ef8699ecab0821d77
Autor:
Simard, G, Omori, Y, Aylor, K, Baxter, EJ, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Cho, HM, Chown, R, Crawford, TM, Crites, AT, Haan, TD, Dobbs, MA, Everett, WB, George, EM, Halverson, NW, Harrington, NL, Henning, JW, Holder, GP, Hou, Z, Holzapfel, WL, Hrubes, JD, Knox, L, Lee, AT, Leitch, EM, Luong-Van, D, Manzotti, A, McMahon, JJ, Meyer, SS, Mocanu, LM, Mohr, JJ, Natoli, T, Padin, S, Pryke, C, Reichardt, CL, Ruhl, JE, Sayre, JT, Schaffer, KK, Shirokoff, E, Staniszewski, Z, Stark, AA, Story, KT, Vanderlinde, K, Vieira, JD, Williamson, R, Wu, WLK
Publikováno v:
Simard, G; Omori, Y; Aylor, K; Baxter, EJ; Benson, BA; Bleem, LE; et al.(2018). Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg2 SPT-SZ and Planck Gravitational Lensing Map. Astrophysical Journal, 860(2), 137-137. doi: 10.3847/1538-4357/aac264. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/3fz895wq
© 2018. The American Astronomical Society. All rights reserved. We report constraints on cosmological parameters from the angular power spectrum of a cosmic microwave background (CMB) gravitational lensing potential map created using temperature dat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::a0d46835c83a6331f3e7fea8e7ecd6c7
http://www.escholarship.org/uc/item/3fz895wq
http://www.escholarship.org/uc/item/3fz895wq
Autor:
Baxter, EJ, Raghunathan, S, Crawford, TM, Fosalba, P, Hou, Z, Holder, GP, Omori, Y, Patil, S, Rozo, E, Abbott, TMC, Annis, J, Aylor, K, Benoit-Lévy, A, Benson, BA, Bertin, E, Bleem, L, Buckley-Geer, E, Burke, DL, Carlstrom, J, Rosell, A Carnero, Kind, M Carrasco, Carretero, J, Chang, CL, Cho, H-M, Crites, AT, Crocce, M, Cunha, CE, da Costa, LN, D'Andrea, CB, Davis, C, de Haan, T, Desai, S, Dietrich, JP, Dobbs, MA, Dodelson, S, Doel, P, Drlica-Wagner, A, Estrada, J, Everett, WB, Neto, A Fausti, Flaugher, B, Frieman, J, García-Bellido, J, George, EM, Gaztanaga, E, Giannantonio, T, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Halverson, NW, Harrington, NL, Hartley, WG, Holzapfel, WL, Honscheid, K, Hrubes, JD, Jain, B, James, DJ, Jarvis, M, Jeltema, T, Knox, L, Krause, E, Kuehn, K, Kuhlmann, S, Kuropatkin, N, Lahav, O, Lee, AT, Leitch, EM, Li, TS, Lima, M, Luong-Van, D, Manzotti, A, March, M, Marrone, DP, Marshall, JL, Martini, P, McMahon, JJ, Melchior, P, Menanteau, F, Meyer, SS, Miller, CJ, Miquel, R, Mocanu, LM, Mohr, JJ, Natoli, T, Nord, B, Ogando, RLC, Padin, S, Plazas, AA, Pryke, C, Rapetti, D, Reichardt, CL, Romer, AK, Roodman, A, Ruhl, JE, Rykoff, E, Sako, M, Sanchez, E, Sayre, JT, Scarpine, V
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 476, iss 2
Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy clusters, p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::15ce572bc630382351482d272ef33fb7
https://escholarship.org/uc/item/2fn9n72j
https://escholarship.org/uc/item/2fn9n72j