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<link>https://repositorio.uchile.cl/handle/2250/117736</link>
<description>Artículos de revistas</description>
<pubDate>Sat, 09 May 2026 17:54:24 GMT</pubDate>
<dc:date>2026-05-09T17:54:24Z</dc:date>
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<title>Improved upper limit on degree-scale CMB B-mode polarization power from the 670 square-degree POLARBEAR survey</title>
<link>https://repositorio.uchile.cl/handle/2250/195699</link>
<description>Improved upper limit on degree-scale CMB B-mode polarization power from the 670 square-degree POLARBEAR survey
Adachi, S.; Adkins, T.; Aguilar Faúndez, Mario Andrés Osvaldo; Arnold, K. S.; Baccigalupi, C.; Barron, D.; Chapman, S.; Cheung, K.; Chinone, Y.; Crowley, K. T.; Elleflot, T.; Errard, J.; Fabbian, G.; Feng, C.; Fujino, T.; Galitzki, N.; Halverson, N. W.; Hasegawa, M.; Hazumi, M.; Hirose, H.; Howe, L.; Ito, J.; Jeong, O.; Kaneko, D.; Katayama, N.; Keating, B.; Kisner, T.; Krachmalnicoff, N.; Kusaka, A.; Lee, T.; Linder, E.; Lonappan, A. I.; Lowry, L. N.; Matsuda, F.; Matsumura, T.; Minami, Y.; Murata, M.; Nishino, H.; Nishinomiya, Y.; Poletti, D.; Reichardt, C. L.; Ross, C.; Segawa, Y.; Siritanasak, P.; Stompor, R.; Suzuki, A.; Tajima, O.; Takakura, S.; Takatori, S.; Tanabe, D.; Teply, G.; Yamada, K.; Zhou, Y.
We report an improved measurement of the degree-scale cosmic microwave background B-mode angular-power spectrum over 670 deg(2) sky area at 150 GHz with Polarbear. In the original analysis of the data, errors in the angle measurement of the continuously rotating half-wave plate, a polarization modulator, caused significant data loss. By introducing an angle-correction algorithm, the data volume is increased by a factor of 1.8. We report a new analysis using the larger data set. We find the measured B-mode spectrum is consistent with the ?CDM model with Galactic dust foregrounds. We estimate the contamination of the foreground by cross-correlating our data and Planck 143, 217, and 353 GHz measurements, where its spectrum is modeled as a power law in angular scale and a modified blackbody in frequency. We place an upper limit on the tensor-to-scalar ratio r &lt; 0.33 at 95% confidence level after marginalizing over the foreground parameters.
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<pubDate>Sat, 01 Jan 2022 00:00:00 GMT</pubDate>
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<dc:date>2022-01-01T00:00:00Z</dc:date>
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<title>Intellectual Property Regimes and Their Impact on Agricultural Research and Development</title>
<link>https://repositorio.uchile.cl/handle/2250/190908</link>
<description>Intellectual Property Regimes and Their Impact on Agricultural Research and Development
Timmermann C.
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<pubDate>Wed, 01 Jan 2020 00:00:00 GMT</pubDate>
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<dc:date>2020-01-01T00:00:00Z</dc:date>
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<title>Mainetti, j.A. filosofía médica</title>
<link>https://repositorio.uchile.cl/handle/2250/190909</link>
<description>Mainetti, j.A. filosofía médica
Stepke, FL
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<pubDate>Wed, 01 Jan 2020 00:00:00 GMT</pubDate>
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<dc:date>2020-01-01T00:00:00Z</dc:date>
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<title>Agriculture and Non-proprietary Science</title>
<link>https://repositorio.uchile.cl/handle/2250/190907</link>
<description>Agriculture and Non-proprietary Science
Timmermann C.
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<pubDate>Wed, 01 Jan 2020 00:00:00 GMT</pubDate>
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<dc:date>2020-01-01T00:00:00Z</dc:date>
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