Zobrazeno 1 - 10
of 621
pro vyhledávání: '"Hill Ca"'
All nitrogen-fixing bacteria and archaea (diazotrophs) use molybdenum (Mo) nitrogenase to reduce dinitrogen (N2) to ammonia. Some diazotrophs also contain alternative nitrogenases that lack Mo: vanadium (V) and iron-only (Fe) nitrogenases. Among diaz
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cd0049b1f6c6ce90d8166d1f6f1076fc
https://doi.org/10.1101/2021.06.03.447018
https://doi.org/10.1101/2021.06.03.447018
Internal Delensing of Cosmic Microwave Background Polarization B-Modes with the POLARBEAR Experiment
Autor:
Adachi, S, Aguilar Faúndez, MAO, Akiba, Y, Ali, A, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Bianchini, F, Borrill, J, Carron, J, Cheung, K, Chinone, Y, Crowley, K, El Bouhargani, H, Elleflot, T, Errard, J, Fabbian, G, Feng, C, Fujino, T, Goeckner-Wald, N, Hasegawa, M, Hazumi, M, Hill, CA, Howe, L, Katayama, N, Keating, B, Kikuchi, S, Kusaka, A, Lee, AT, Leon, D, Linder, E, Lowry, LN, Matsuda, F, Matsumura, T, Minami, Y, Namikawa, T, Navaroli, M, Nishino, H, Peloton, J, Pham, ATP, Poletti, D, Puglisi, G, Reichardt, CL, Segawa, Y, Sherwin, BD, Silva-Feaver, M, Siritanasak, P, Stompor, R, Tajima, O, Takatori, S, Tanabe, D, Teply, GP, Vergès, C, POLARBEAR Collaboration
Publikováno v:
Physical review letters, vol 124, iss 13
Using only cosmic microwave background polarization data from the polarbear experiment, we measure B-mode polarization delensing on subdegree scales at more than 5σ significance. We achieve a 14% B-mode power variance reduction, the highest to date
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::634311c573887b055efd4556ce3061da
https://escholarship.org/uc/item/55j0c2wf
https://escholarship.org/uc/item/55j0c2wf
Autor:
Ade, P, Aguirre, J, Ahmed, Z, Aiola, S, Ali, A, Alonso, D, Alvarez, MA, Arnold, K, Ashton, P, Austermann, J, Awan, H, Baccigalupi, C, Baildon, T, Barron, D, Battaglia, N, Battye, R, Baxter, E, Bazarko, A, Beall, JA, Bean, R, Beck, D, Beckman, S, Beringue, B, Bianchini, F, Boada, S, Boettger, D, Bond, JR, Borrill, J, Brown, ML, Bruno, SM, Bryan, S, Calabrese, E, Calafut, V, Calisse, P, Carron, J, Challinor, A, Chesmore, G, Chinone, Y, Chluba, J, Cho, HMS, Choi, S, Coppi, G, Cothard, NF, Coughlin, K, Crichton, D, Crowley, KD, Crowley, KT, Cukierman, A, D'Ewart, JM, Dünner, R, De Haan, T, Devlin, M, Dicker, S, Didier, J, Dobbs, M, Dober, B, Duell, CJ, Duff, S, Duivenvoorden, A, Dunkley, J, Dusatko, J, Errard, J, Fabbian, G, Feeney, S, Ferraro, S, Fluxà, P, Freese, K, Frisch, JC, Frolov, A, Fuller, G, Fuzia, B, Galitzki, N, Gallardo, PA, Ghersi, JTG, Gao, J, Gawiser, E, Gerbino, M, Gluscevic, V, Goeckner-Wald, N, Golec, J, Gordon, S, Gralla, M, Green, D, Grigorian, A, Groh, J, Groppi, C, Guan, Y, Gudmundsson, JE, Han, D, Hargrave, P, Hasegawa, M, Hasselfield, M, Hattori, M, Haynes, V, Hazumi, M, He, Y, Healy, E, Henderson, SW, Hervias-Caimapo, C, Hill, CA
Publikováno v:
Journal of Cosmology and Astroparticle Physics, vol 2019, iss 2
Journal of Cosmology and Astroparticle Physics, vol 2019, iss 02
Journal of Cosmology and Astroparticle Physics, vol 2019, iss 02
The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scientific goals of the experiment, motivate the design, and forecast its pe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::15f34af456cdfae92998dceaf730338c
Autor:
Hasebe, T, Kashima, S, Ade, PAR, Akiba, Y, Alonso, D, Arnold, K, Aumont, J, Baccigalupi, C, Barron, D, Basak, S, Beckman, S, Borrill, J, Boulanger, F, Bucher, M, Calabrese, E, Chinone, Y, Cho, HM, Cukierman, A, Curtis, DW, de Haan, T, Dobbs, M, Dominjon, A, Dotani, T, Duband, L, Ducout, A, Dunkley, J, Duval, JM, Elleflot, T, Eriksen, HK, Errard, J, Fischer, J, Fujino, T, Funaki, T, Fuskeland, U, Ganga, K, Goeckner-Wald, N, Grain, J, Halverson, NW, Hamada, T, Hasegawa, M, Hattori, K, Hattori, M, Hayes, L, Hazumi, M, Hidehira, N, Hill, CA, Hilton, G, Hubmayr, J, Ichiki, K, Iida, T, Imada, H, Inoue, M, Inoue, Y, Irwin, KD, Ishino, H, Jeong, O, Kanai, H, Kaneko, D, Katayama, N, Kawasaki, T, Kernasovskiy, SA, Keskitalo, R, Kibayashi, A, Kida, Y, Kimura, K, Kisner, T, Kohri, K, Komatsu, E, Komatsu, K, Kuo, CL, Kurinsky, NA, Kusaka, A, Lazarian, A, Lee, AT, Li, D, Linder, E, Maffei, B, Mangilli, A, Maki, M, Matsumura, T, Matsuura, S, Meilhan, D, Mima, S, Minami, Y, Mitsuda, K, Montier, L, Nagai, M, Nagasaki, T, Nagata, R, Nakajima, M, Nakamura, S, Namikawa, T, Naruse, M, Nishino, H, Nitta, T, Noguchi, T, Ogawa, H, Oguri, S, Okada, N, Okamoto, A
Publikováno v:
Journal of Low Temperature Physics, vol 193, iss 5-6
The high-frequency telescope for LiteBIRD is designed with refractive and reflective optics. In order to improve sensitivity, this paper suggests the new optical configurations of the HFT which have approximately 7 times larger focal planes than that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::7f36521c79d6957ed3d608e0887109fc
https://escholarship.org/uc/item/8s4897pp
https://escholarship.org/uc/item/8s4897pp
Autor:
Gallardo, Pa, Gudmundsson, J, Koopman, Bj, Matsuda, Ft, Simon, Sm, Ali, A, Bryan, S, Chinone, Y, Coppi, G, Cothard, N, Devlin, Mj, Dicker, S, Fabbian, G, Galitzki, N, Hill, Ca, Keating, B, Kusaka, A, Lashner, J, Lee, At, Limon, M, Mauskopf, Pd, Mcmahon, J, Nati, F, Niemack, Md, Orlowski-Scherer, Jl, Parshley, Sc, Puglisi, G, Reichardt, Cl, Salatino, M, Staggs, S, Suzuki, A, Vavagiakis, Em, Wollack, Ej, Xu, Z, Zhu, N
The Simons Observatory (SO) is a new experiment that aims to measure the cosmic microwave background (CMB) in temperature and polarization. SO will measure the polarized sky over a large range of microwave frequencies and angular scales using a combi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::cbe5df08020114b2001554402b94e1ad
http://hdl.handle.net/10281/290837
http://hdl.handle.net/10281/290837
Autor:
Ade, PAR, Aguilar, M, Akiba, Y, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Bianchini, F, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Crowley, K, Cukierman, A, Dünner, R, Dobbs, M, Ducout, A, Elleflot, T, Errard, J, Fabbian, G, Feeney, SM, Feng, C, Fujino, T, Galitzki, N, Gilbert, A, Goeckner-Wald, N, Groh, JC, Hall, G, Halverson, N, Hamada, T, Hasegawa, M, Hazumi, M, Hill, CA, Howe, L, Inoue, Y, Jaehnig, G, Jaffe, AH, Jeong, O, Kaneko, D, Katayama, N, Keating, B, Keskitalo, R, Kisner, T, Krachmalnicoff, N, Kusaka, A, Jeune, ML, Lee, AT, Leitch, EM, Leon, D, Linder, E, Lowry, L, Matsuda, F, Matsumura, T, Minami, Y, Montgomery, J, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Pham, ATP, Poletti, D, Puglisi, G, Reichardt, CL, Richards, PL, Ross, C, Segawa, Y, Sherwin, BD, Silva-Feaver, M, Siritanasak, P, Stebor, N, Stompor, R, Suzuki, A, Tajima, O, Takakura, S
Publikováno v:
Ade, PAR; Aguilar, M; Akiba, Y; Arnold, K; Baccigalupi, C; Barron, D; et al.(2017). A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data. Astrophysical Journal, 848(2). doi: 10.3847/1538-4357/aa8e9f. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/100162cr
© 2017. The American Astronomical Society. All rights reserved. We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::aca8650fe0a973dc8edde6dfc50a2088
http://www.escholarship.org/uc/item/100162cr
http://www.escholarship.org/uc/item/100162cr
Publikováno v:
Psychology & Health. Jan2008, Vol. 23 Issue 1, p41-56. 16p.
Publikováno v:
In Value in Health October-November 2017 20(9):A569-A569
Publikováno v:
In Value in Health November 2016 19(7):A491-A491
Autor:
Garcia Sanchez, JJ, Hill, CA
Publikováno v:
In Value in Health November 2016 19(7):A489-A489