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1. Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

Author

Hikage, Chiaki, Oguri, Masamune, Hamana, Takashi, More, Surhud, Mandelbaum, Rachel, Takada, Masahiro, Köhlinger, Fabian, Miyatake, Hironao, Nishizawa, Atsushi J., Aihara, Hiroaki, Armstrong, Robert, Bosch, James, Coupon, Jean, Ducout, Anne, Ho, Paul, Hsieh, Bau-Ching, Komiyama, Yutaka, Lanusse, François, Leauthaud, Alexie, Lupton, Robert H., Medezinski, Elinor, Mineo, Sogo, Miyama, Shoken, Miyazaki, Satoshi, Murata, Ryoma, Murayama, Hitoshi, Shirasaki, Masato, Sifón, Cristóbal, Simet, Melanie, Speagle, Joshua, Spergel, David N., Strauss, Michael A., Sugiyama, Naoshi, Tanaka, Masayuki, Utsumi, Yousuke, Wang, Shiang-Yu, and Yamada, Yoshihiko

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We measure cosmic weak lensing shear power spectra with the Subaru Hyper Suprime-Cam (HSC) survey first-year shear catalog covering 137deg$^2$ of the sky. Thanks to the high effective galaxy number density of $\sim$17 arcmin$^{-2}$ even after conservative cuts such as magnitude cut of $i<24.5$ and photometric redshift cut of $0.3\leq z \leq 1.5$, we obtain a high significance measurement of the cosmic shear power spectra in 4 tomographic redshift bins, achieving a total signal-to-noise ratio of 16 in the multipole range $300 \leq \ell \leq 1900$. We carefully account for various uncertainties in our analysis including the intrinsic alignment of galaxies, scatters and biases in photometric redshifts, residual uncertainties in the shear measurement, and modeling of the matter power spectrum. The accuracy of our power spectrum measurement method as well as our analytic model of the covariance matrix are tested against realistic mock shear catalogs. For a flat $\Lambda$ cold dark matter ($\Lambda$CDM) model, we find $S_8\equiv \sigma_8(\Omega_{\rm m}/0.3)^\alpha=0.800^{+0.029}_{-0.028}$ for $\alpha=0.45$ ($S_8=0.780^{+0.030}_{-0.033}$ for $\alpha=0.5$) from our HSC tomographic cosmic shear analysis alone. In comparison with Planck cosmic microwave background constraints, our results prefer slightly lower values of $S_8$, although metrics such as the Bayesian evidence ratio test do not show significant evidence for discordance between these results. We study the effect of possible additional systematic errors that are unaccounted in our fiducial cosmic shear analysis, and find that they can shift the best-fit values of $S_8$ by up to $\sim 0.6\sigma$ in both directions. The full HSC survey data will contain several times more area, and will lead to significantly improved cosmological constraints., Comment: 43 pages, 21 figures, accepted for publication in PASJ

Published
2018
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2. Performance of a continuously rotating half-wave plate on the POLARBEAR telescope

Author

Takakura, Satoru, Aguilar, Mario, Akiba, Yoshiki, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beckman, Shawn, Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Cukierman, Ari, Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Fujino, Takuro, Galitzki, Nicholas, Goeckner-Wald, Neil, Halverson, Nils W., Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Hill, Charles, Howe, Logan, Inoue, Yuki, Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Katayama, Nobuhiko, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Lee, Adrian T., Leon, David, Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Navaroli, Martin, Nishino, Haruki, Paar, Hans, Peloton, Julien, Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Ross, Colin, Siritanasak, Praween, Suzuki, Aritoki, Tajima, Osamu, Takatori, Sayuri, and Teply, Grant

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Physics - Instrumentation and Detectors
Abstract

A continuously rotating half-wave plate (CRHWP) is a promising tool to improve the sensitivity to large angular scales in cosmic microwave background (CMB) polarization measurements. With a CRHWP, single detectors can measure three of the Stokes parameters, $I$, $Q$ and $U$, thereby avoiding the set of systematic errors that can be introduced by mismatches in the properties of orthogonal detector pairs. We focus on the implementation of CRHWPs in large aperture telescopes (i.e. the primary mirror is larger than the current maximum half-wave plate diameter of $\sim$0.5 m), where the CRHWP can be placed between the primary mirror and focal plane. In this configuration, one needs to address the intensity to polarization ($I{\rightarrow}P$) leakage of the optics, which becomes a source of 1/f noise and also causes differential gain systematics that arise from CMB temperature fluctuations. In this paper, we present the performance of a CRHWP installed in the POLARBEAR experiment, which employs a Gregorian telescope with a 2.5 m primary illumination pattern. The CRHWP is placed near the prime focus between the primary and secondary mirrors. We find that the $I{\rightarrow}P$ leakage is larger than the expectation from the physical properties of our primary mirror, resulting in a 1/f knee of 100 mHz. The excess leakage could be due to imperfections in the detector system, i.e. detector non-linearity in the responsivity and time-constant. We demonstrate, however, that by subtracting the leakage correlated with the intensity signal, the 1/f noise knee frequency is reduced to 32 mHz ($\ell \sim$39 for our scan strategy), which is very promising to probe the primordial B-mode signal. We also discuss methods for further noise subtraction in future projects where the precise temperature control of instrumental components and the leakage reduction will play a key role., Comment: 27 pages, 5 figures, 3 tables, published version in JCAP. Includes some minor corrections

Published
2017
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3. Making maps of Cosmic Microwave Background polarization for B-mode studies: the POLARBEAR example

Author

Poletti, Davide, Fabbian, Giulio, Jeune, Maude Le, Peloton, Julien, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beckman, Shawn, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Cukierman, Ari, Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Feeney, Stephen, Goeckner-Wald, Neil, Groh, John, Hall, Grantland, Hasegawa, Masaya, Hazumi, Masashi, Hill, Charles, Howe, Logan, Inoue, Yuki, Jaffe, Andrew H., Jeong, Oliver, Katayama, Nobuhiko, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Kusaka, Akito, Lee, Adrian T., Leon, David, Linder, Eric, Lowry, Lindsay, Matsuda, Frederick, Navaroli, Martin, Paar, Hans, Puglisi, Giuseppe, Reichardt, Christian L., Ross, Colin, Siritanasak, Praween, Stebor, Nathan, Steinbach, Bryan, Stompor, Radek, Suzuki, Aritoki, Tajima, Osamu, Teply, Grant, and Whitehorn, Nathan

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Analysis of cosmic microwave background (CMB) datasets typically requires some filtering of the raw time-ordered data. Filtering is frequently used to minimize the impact of low frequency noise, atmospheric contributions and/or scan synchronous signals on the resulting maps. In this work we explicitly construct a general filtering operator, which can unambiguously remove any set of unwanted modes in the data, and then amend the map-making procedure in order to incorporate and correct for it. We show that such an approach is mathematically equivalent to the solution of a problem in which the sky signal and unwanted modes are estimated simultaneously and the latter are marginalized over. We investigate the conditions under which this amended map-making procedure can render an unbiased estimate of the sky signal in realistic circumstances. We then study the effects of time-domain filtering on the noise correlation structure in the map domain, as well as impact it may have on the performance of the popular pseudo-spectrum estimators. We conclude that although maps produced by the proposed estimators arguably provide the most faithful representation of the sky possible given the data, they may not straightforwardly lead to the best constraints on the power spectra of the underlying sky signal and special care may need to be taken to ensure this is the case. By contrast, simplified map-makers which do not explicitly correct for time-domain filtering, but leave it to subsequent steps in the data analysis, may perform equally well and be easier and faster to implement. We focus on polarization-sensitive measurements targeting the B-mode component of the CMB signal and apply the proposed methods to realistic simulations based on characteristics of an actual CMB polarization experiment, POLARBEAR., Comment: 26 pages

Published
2016
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4. Making maps of cosmic microwave background polarization for B-mode studies: the POLARBEAR example

Author

Poletti, Davide, Fabbian, Giulio, Le Jeune, Maude, Peloton, Julien, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beckman, Shawn, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Cukierman, Ari, Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Feeney, Stephen, Goeckner-Wald, Neil, Groh, John, Hall, Grantland, Hasegawa, Masaya, Hazumi, Masashi, Hill, Charles, Howe, Logan, Inoue, Yuki, Jaffe, Andrew H, Jeong, Oliver, Katayama, Nobuhiko, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Kusaka, Akito, Lee, Adrian T, Leon, David, Linder, Eric, Lowry, Lindsay, Matsuda, Frederick, Navaroli, Martin, Paar, Hans, Puglisi, Giuseppe, Reichardt, Christian L, Ross, Colin, Siritanasak, Praween, Stebor, Nathan, Steinbach, Bryan, Stompor, Radek, Suzuki, Aritoki, Tajima, Osamu, Teply, Grant, and Whitehorn, Nathan

Subjects
Space Sciences, Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, cosmic background radiation, cosmology: observations, astro-ph.IM, astro-ph.CO, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract

Analysis of cosmic microwave background (CMB) datasets typically requires some filtering of the raw time-ordered data. For instance, in the context of ground-based observations, filtering is frequently used to minimize the impact of low frequency noise, atmospheric contributions and/or scan synchronous signals on the resulting maps. In this work we have explicitly constructed a general filtering operator, which can unambiguously remove any set of unwanted modes in the data, and then amend the map-making procedure in order to incorporate and correct for it. We show that such an approach is mathematically equivalent to the solution of a problem in which the sky signal and unwanted modes are estimated simultaneously and the latter are marginalized over. We investigated the conditions under which this amended map-making procedure can render an unbiased estimate of the sky signal in realistic circumstances. We then discuss the potential implications of these observations on the choice of map-making and power spectrum estimation approaches in the context of B-mode polarization studies. Specifically, we have studied the effects of time-domain filtering on the noise correlation structure in the map domain, as well as impact it may haveon the performance of the popular pseudo-spectrum estimators. We conclude that although maps produced by the proposed estimators arguably provide the most faithful representation of the sky possible given the data, they may not straightforwardly lead to the best constraints on the power spectra of the underlying sky signal and special care may need to be taken to ensure this is the case. By contrast, simplified map-makers which do not explicitly correct for time-domain filtering, but leave it to subsequent steps in the data analysis, may perform equally well and be easier and faster to implement. We focused on polarization-sensitive measurements targeting the B-mode component of the CMB signal and apply the proposed methods to realistic simulations based on characteristics of an actual CMB polarization experiment, POLARBEAR. Our analysis and conclusions are however more generally applicable.

Published
2017

5. POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields

Author

POLARBEAR Collaboration, Ade, Peter A. R., Arnold, Kam, Atlas, Matt, Baccigalupi, Carlo, Barron, Darcy, Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Cukierman, Ari, Dobbs, Matt, Ducout, Anne, Dunner, Rolando, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, Stephen, Feng, Chang, Gilbert, Adam, Goeckner-Wald, Neil, Groh, John, Hall, Grantland, Halverson, Nils W., Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Hill, Charles, Holzapfel, William L., Hori, Yasuto, Howe, Logan, Inoue, Yuki, Jaehnig, Gregory C., Jaffe, Andrew H., Jeong, Oliver, Katayama, Nobuhiko, Kaufman, Jonathan P., Keating, Brian, Kermish, Zigmund, Keskitalo, Reijo, Kisner, Theodore, Kusaka, Akito, Jeune, Maude Le, Lee, Adrian T., Leitch, Erik M., Leon, David, Li, Yun, Linder, Eric, Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Miller, Nathan, Montgomery, Josh, Myers, Michael J., Navaroli, Martin, Nishino, Haruki, Okamura, Takahiro, Paar, Hans, Peloton, Julien, Pogosian, Levon, Poletti, Davide, Puglisi, Giuseppe, Raum, Christopher, Rebeiz, Gabriel, Reichardt, Christian L., Richards, Paul L., Ross, Colin, Rotermund, Kaja M., Schenck, David E., Sherwin, Blake D., Shimon, Meir, Shirley, Ian, Siritanasak, Praween, Smecher, Graeme, Stebor, Nathan, Steinbach, Bryan, Suzuki, Aritoki, Suzuki, Jun-ichi, Tajima, Osamu, Takakura, Satoru, Tikhomirov, Alexei, Tomaru, Takayuki, Whitehorn, Nathan, Wilson, Brandon, Yadav, Amit, Zahn, Alex, and Zahn, Oliver

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We constrain anisotropic cosmic birefringence using four-point correlations of even-parity $E$-mode and odd-parity $B$-mode polarization in the cosmic microwave background measurements made by the POLARization of the Background Radiation (POLARBEAR) experiment in its first season of observations. We find that the anisotropic cosmic birefringence signal from any parity-violating processes is consistent with zero. The Faraday rotation from anisotropic cosmic birefringence can be compared with the equivalent quantity generated by primordial magnetic fields if they existed. The POLARBEAR nondetection translates into a 95% confidence level (C.L.) upper limit of 93 nanogauss (nG) on the amplitude of an equivalent primordial magnetic field inclusive of systematic uncertainties. This four-point correlation constraint on Faraday rotation is about 15 times tighter than the upper limit of 1380 nG inferred from constraining the contribution of Faraday rotation to two-point correlations of $B$-modes measured by Planck in 2015. Metric perturbations sourced by primordial magnetic fields would also contribute to the $B$-mode power spectrum. Using the POLARBEAR measurements of the $B$-mode power spectrum (two-point correlation), we set a 95% C.L. upper limit of 3.9 nG on primordial magnetic fields assuming a flat prior on the field amplitude. This limit is comparable to what was found in the Planck 2015 two-point correlation analysis with both temperature and polarization. We perform a set of systematic error tests and find no evidence for contamination. This work marks the first time that anisotropic cosmic birefringence or primordial magnetic fields have been constrained from the ground at subdegree scales., Comment: 10 pages, 5 figures. Phys. Rev. D Editors' Suggestion

Published
2015
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6. POLARBEAR constraints on cosmic birefringence and primordial magnetic fields

Author

Ade, Peter AR, Arnold, Kam, Atlas, Matt, Baccigalupi, Carlo, Barron, Darcy, Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Cukierman, Ari, Dobbs, Matt, Ducout, Anne, Dunner, Rolando, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, Stephen, Feng, Chang, Gilbert, Adam, Goeckner-Wald, Neil, Groh, John, Hall, Grantland, Halverson, Nils W, Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Hill, Charles, Holzapfel, William L, Hori, Yasuto, Howe, Logan, Inoue, Yuki, Jaehnig, Gregory C, Jaffe, Andrew H, Jeong, Oliver, Katayama, Nobuhiko, Kaufman, Jonathan P, Keating, Brian, Kermish, Zigmund, Keskitalo, Reijo, Kisner, Theodore, Kusaka, Akito, Le Jeune, Maude, Lee, Adrian T, Leitch, Erik M, Leon, David, Li, Yun, Linder, Eric, Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Miller, Nathan, Montgomery, Josh, Myers, Michael J, Navaroli, Martin, Nishino, Haruki, Okamura, Takahiro, Paar, Hans, Peloton, Julien, Pogosian, Levon, Poletti, Davide, Puglisi, Giuseppe, Raum, Christopher, Rebeiz, Gabriel, Reichardt, Christian L, Richards, Paul L, Ross, Colin, Rotermund, Kaja M, Schenck, David E, Sherwin, Blake D, Shimon, Meir, Shirley, Ian, Siritanasak, Praween, Smecher, Graeme, Stebor, Nathan, Steinbach, Bryan, Suzuki, Aritoki, Suzuki, Jun-ichi, Tajima, Osamu, Takakura, Satoru, Tikhomirov, Alexei, Tomaru, Takayuki, Whitehorn, Nathan, Wilson, Brandon, Yadav, Amit, Zahn, Alex, and Zahn, Oliver

Subjects
Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, astro-ph.CO, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract

We constrain anisotropic cosmic birefringence using four-point correlations of even-parity E-mode and odd-parity B-mode polarization in the cosmic microwave background measurements made by the POLARization of the Background Radiation (POLARBEAR) experiment in its first season of observations. We find that the anisotropic cosmic birefringence signal from any parity-violating processes is consistent with zero. The Faraday rotation from anisotropic cosmic birefringence can be compared with the equivalent quantity generated by primordial magnetic fields if they existed. The POLARBEAR nondetection translates into a 95% confidence level (C.L.) upper limit of 93 nanogauss (nG) on the amplitude of an equivalent primordial magnetic field inclusive of systematic uncertainties. This four-point correlation constraint on Faraday rotation is about 15 times tighter than the upper limit of 1380 nG inferred from constraining the contribution of Faraday rotation to two-point correlations of B-modes measured by Planck in 2015. Metric perturbations sourced by primordial magnetic fields would also contribute to the B-mode power spectrum. Using the POLARBEAR measurements of the B-mode power spectrum (two-point correlation), we set a 95% C.L. upper limit of 3.9 nG on primordial magnetic fields assuming a flat prior on the field amplitude. This limit is comparable to what was found in the Planck 2015 two-point correlation analysis with both temperature and polarization. We perform a set of systematic error tests and find no evidence for contamination. This work marks the first time that anisotropic cosmic birefringence or primordial magnetic fields have been constrained from the ground at subdegree scales.

Published
2015

7. Non Gaussianity and Minkowski Functionals: forecasts for Planck

Author

Ducout, Anne, Bouchet, François, Colombi, Stéphane, Pogosyan, Dmitri, and Prunet, Simon

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We study Minkowski Functionals as probes of primordial non-Gaussianity in the Cosmic Microwave Background, specifically for the estimate of the primordial `local' bi-spectrum parameter f_NL, with instrumental parameters which should be appropriate for the Planck experiment. We use a maximum likelihood approach, which we couple with various filtering methods and test thoroughly for convergence. We included the effect of inhomogeneous noise as well as astrophysical biases induced by point sources and by the contamination from the Galaxy. We find that, when Wiener filtered maps are used (rather than simply smoothed with Gaussian), the expected error on the measurement of f_NL should be as small as \Delta f_NL \simeq 10 when combining the 3 channels at 100, 143 and 217 GHz in the Planck extended mission setup. This result is fairly insensitive to the non homogeneous nature of the noise, at least for realistic hit-maps expected from Planck. We then estimate the bias induced on the measurement of f_NL by point sources in those 3 channels. With the appropriate masking of the bright sources, this bias can be reduced to a negligible level in the 100 and 143 GHz channels. It remains significant in the 217 GHz channel, but can be corrected for. The galactic foreground biases are quite important and present a complex dependence on sky coverage: making them negligible will depend strongly on the quality of the component separation methods., Comment: 26 pages, 12 figures

Published
2012
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8. Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

Author

Hikage, Chiaki, primary, Oguri, Masamune, primary, Hamana, Takashi, primary, More, Surhud, primary, Mandelbaum, Rachel, primary, Takada, Masahiro, primary, Köhlinger, Fabian, primary, Miyatake, Hironao, primary, Nishizawa, Atsushi J, primary, Aihara, Hiroaki, primary, Armstrong, Robert, primary, Bosch, James, primary, Coupon, Jean, primary, Ducout, Anne, primary, Ho, Paul, primary, Hsieh, Bau-Ching, primary, Komiyama, Yutaka, primary, Lanusse, François, primary, Leauthaud, Alexie, primary, Lupton, Robert H, primary, Medezinski, Elinor, primary, Mineo, Sogo, primary, Miyama, Shoken, primary, Miyazaki, Satoshi, primary, Murata, Ryoma, primary, Murayama, Hitoshi, primary, Shirasaki, Masato, primary, Sifón, Cristóbal, primary, Simet, Melanie, primary, Speagle, Joshua, primary, Spergel, David N, primary, Strauss, Michael A, primary, Sugiyama, Naoshi, primary, Tanaka, Masayuki, primary, Utsumi, Yousuke, primary, Wang, Shiang-Yu, primary, and Yamada, Yoshihiko, primary

Published
2019
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9. Concept design of the LiteBIRD satellite for CMB B-mode polarization

Author

Sekimoto, Yutaro, primary, Noviello, Fabio, primary, Ota, Izumi, primary, Winter, B., primary, Ade, Peter, primary, Mangilli, Anna, primary, Aumont, Jonathan, primary, Austermann, Jason, primary, Baccigalupi, Carlo, primary, Banday, Anthony, primary, Banerji, Ranajoy, primary, Basak, Soumen, primary, Beckman, Shawn, primary, Bersanelli, Marco, primary, Borill, Julian, primary, Boulanger, Francois, primary, Brown, Michael, primary, Bucher, Martin, primary, Calabrese, Erminia, primary, Challinor, Anthony, primary, Chinone, Yuji, primary, Columbro, Fabio, primary, Cukierman, Ari, primary, Curtis, David, primary, de Bernardis, Paolo, primary, de Petris, Marco, primary, Dobbs, Matthieu, primary, Dotani, Tadayasu, primary, Duband, Lionel, primary, Ducout, Anne, primary, Ebisawa, Ken, primary, Elleflot, Tucker, primary, Eriksen, Hans Kristian, primary, Errand, Josquin, primary, Flauger, Raphael, primary, Franceschet, Cristian, primary, Fuskeland, Unni, primary, Ganga, Ken, primary, Gao, Jian-Rong, primary, Ghigna, Tommaso, primary, Grain, Julien, primary, Gruppuso, Alessandro, primary, Halverson, Nils, primary, Hargrave, Peter, primary, Hasebe, Takashi, primary, Hasegawa, Masaya, primary, Hattori, Makoto, primary, Hazumi, Masashi, primary, Henrot-Versille, Sophie, primary, Hill, Charles, primary, Hirota, Yukimasa, primary, Hivon, Eric, primary, Hoang, Duc Thuong, primary, Hubmayr, Johannes, primary, Ichiki, Kiyotomo, primary, Imada, Hiroaki, primary, Ishino, Hirokazu, primary, Jaehnig, Greg, primary, Arnold, Kam, primary, Kanai, Hiroaki, primary, Kashima, Shingo, primary, Katayama, Nobu, primary, Kawasaki, Takeo, primary, Keskitalo, Rijo, primary, Kibayashi, Atsuko, primary, Kikuchi, Takahiro, primary, Kimura, Kimihiro, primary, Kisner, Theodore, primary, Kobayashi, Yohei, primary, Kogiso, Nozomu, primary, Kohri, Kazunori, primary, Komatsu, Eiichiro, primary, Komatsu, Kunimoto, primary, Konishi, Kuniaki, primary, Krachmalnicoff, Nicoletta, primary, Kuo, Chao Lin, primary, Kurinsky, Noah, primary, Kushino, Akihiro, primary, Lamagna, Luca, primary, Lee, Adrian, primary, Linder, Eric, primary, Maffei, Buruno, primary, Maki, Muneyoshi, primary, Martinez-Gonzalez, Enrique, primary, Masi, Silvia, primary, Matsumura, Tomotakake, primary, Mennella, Aniello, primary, Minami, Yuto, primary, Mitsuda, Kazuhisa, primary, Molinari, Diego, primary, Montier, Ludovic, primary, Morgante, Gianluca, primary, Mot, Baptiste, primary, Murata, Yasuhiro, primary, Murphy, Anthony, primary, Nagai, Makoto, primary, Nagata, Ryo, primary, Nakamura, Shogo, primary, Namikawa, Toshiya, primary, Natoli, Paolo, primary, Nishibori, Toshiyuki, primary, Nishino, Haruki, primary, O'Sullivan, Creidhe, primary, Ochi, Hiroki, primary, Ogawa, Hideo, primary, Ogawa, Hiroyuki, primary, Ohsaki, Hiroyuki, primary, Okada, Nozomi, primary, Piacentini, Francesco, primary, Pisano, Giampaolo, primary, Polenta, Gianluca, primary, Poletti, Davide, primary, Puglisi, Giuseppe, primary, Raum, Christopher, primary, Remazeilles, Mathieu, primary, Sakurai, Haruyuki, primary, Sakurai, Yuki, primary, Savini, Giorgio, primary, Sherwin, Blake, primary, Shinozaki, Keisuke, primary, Shiraishi, Maresuke, primary, Signorelli, Giovanni, primary, Smecher, Graeme, primary, Stompor, Radek, primary, Sugai, Hajime, primary, Sugiyama, Shinya, primary, Suzuki, Aritoki, primary, Suzuki, Junichi, primary, Takaku, Ryota, primary, Takakura, Hayato, primary, Takakura, Satoru, primary, Taylor, Ellen, primary, Terao, Yutaka, primary, Thompson, Keith L., primary, Thorne, Ben, primary, Tomasi, Maurizio, primary, Tomida, Hiroshi, primary, Trappe, Neil, primary, Tristram, Matthieu, primary, Tsuji, Masatoshi, primary, Tsujimoto, Masahiro, primary, Uozumi, Satoru, primary, Utsunomiya, Shin, primary, Vittorio, Nicola, primary, Watanabe, Naoki, primary, Wehus, Ingunn, primary, Westbrook, Benjamin, primary, Yamamoto, Ryo, primary, Yamasaki, Noriko, primary, Yanagisawa, Masato, primary, Yoshida, Tetsuya, primary, Yumoto, Junji, primary, Zannoni, Mario, primary, Zonca, Andrea, primary, Kataoka, Yuichiro, primary, Patanchon, Guillaume, primary, and Realini, S., primary

Published
2018
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10. Concept design of the LiteBIRD satellite for CMB B-mode polarization

Author

Realini, S, Patanchon, G, Kataoka, Y, Zonca, A, Zannoni, M, Yumoto, J, Yoshida, T, Yanagisawa, M, Yamasaki, N, Yamamoto, R, Westbrook, B, Wehus, I, Watanabe, N, Vittorio, N, Utsunomiya, S, Uozumi, S, Tsujimoto, M, Tsuji, M, Tristram, M, Trappe, N, Tomida, H, Tomasi, M, Thorne, B, Thompson, K, Terao, Y, Taylor, E, Takakura, S, Takakura, H, Takaku, R, Suzuki, J, Suzuki, A, Sugiyama, S, Sugai, H, Stompor, R, Smecher, G, Signorelli, G, Shiraishi, M, Shinozaki, K, Sherwin, B, Savini, G, Sakurai, Y, Sakurai, H, Remazeilles, M, Raum, C, Puglisi, G, Poletti, D, Polenta, G, Pisano, G, Piacentini, F, Okada, N, Ohsaki, H, Ogawa, H, Ochi, H, O'Sullivan, C, Nishino, H, Nishibori, T, Natoli, P, Namikawa, T, Nakamura, S, Nagata, R, Nagai, M, Murphy, A, Murata, Y, Mot, B, Morgante, G, Montier, L, Molinari, D, Mitsuda, K, Minami, Y, Mennella, A, Matsumura, T, Masi, S, Martinez-Gonzalez, E, Maki, M, Maffei, B, Linder, E, Lee, A, Lamagna, L, Kushino, A, Kurinsky, N, Kuo, C, Krachmalnicoff, N, Konishi, K, Komatsu, K, Komatsu, E, Kohri, K, Kogiso, N, Kobayashi, Y, Kisner, T, Kimura, K, Kikuchi, T, Kibayashi, A, Keskitalo, R, Kawasaki, T, Katayama, N, Kashima, S, Kanai, H, Arnold, K, Jaehnig, G, Ishino, H, Imada, H, Ichiki, K, Hubmayr, J, Hoang, D, Hivon, E, Hirota, Y, Hill, C, Henrot-Versille, S, Hazumi, M, Hattori, M, Hasegawa, M, Hasebe, T, Hargrave, P, Halverson, N, Gruppuso, A, Grain, J, Ghigna, T, Gao, J, Ganga, K, Fuskeland, U, Franceschet, C, Flauger, R, Errand, J, Eriksen, H, Elleflot, T, Ebisawa, K, Ducout, A, Duband, L, Dotani, T, Dobbs, M, de Petris, M, de Bernardis, P, Curtis, D, Cukierman, A, Columbro, F, Chinone, Y, Challinor, A, Calabrese, E, Bucher, M, Brown, M, Boulanger, F, Borill, J, Bersanelli, M, Beckman, S, Basak, S, Banerji, R, Banday, A, Baccigalupi, C, Austermann, J, Aumont, J, Mangilli, A, Ade, P, Winter, B, Ota, I, Noviello, F, Sekimoto, Y, Realini, S., Patanchon, Guillaume, Kataoka, Yuichiro, Zonca, Andrea, Zannoni, Mario, Yumoto, Junji, Yoshida, Tetsuya, Yanagisawa, Masato, Yamasaki, Noriko, Yamamoto, Ryo, Westbrook, Benjamin, Wehus, Ingunn, Watanabe, Naoki, Vittorio, Nicola, Utsunomiya, Shin, Uozumi, Satoru, Tsujimoto, Masahiro, Tsuji, Masatoshi, Tristram, Matthieu, Trappe, Neil, Tomida, Hiroshi, Tomasi, Maurizio, Thorne, Ben, Thompson, Keith L., Terao, Yutaka, Taylor, Ellen, Takakura, Satoru, Takakura, Hayato, Takaku, Ryota, Suzuki, Junichi, Suzuki, Aritoki, Sugiyama, Shinya, Sugai, Hajime, Stompor, Radek, Smecher, Graeme, Signorelli, Giovanni, Shiraishi, Maresuke, Shinozaki, Keisuke, Sherwin, Blake, Savini, Giorgio, Sakurai, Yuki, Sakurai, Haruyuki, Remazeilles, Mathieu, Raum, Christopher, Puglisi, Giuseppe, Poletti, Davide, Polenta, Gianluca, Pisano, Giampaolo, Piacentini, Francesco, Okada, Nozomi, Ohsaki, Hiroyuki, Ogawa, Hiroyuki, Ogawa, Hideo, Ochi, Hiroki, O'Sullivan, Creidhe, Nishino, Haruki, Nishibori, Toshiyuki, Natoli, Paolo, Namikawa, Toshiya, Nakamura, Shogo, Nagata, Ryo, Nagai, Makoto, Murphy, Anthony, Murata, Yasuhiro, Mot, Baptiste, Morgante, Gianluca, Montier, Ludovic, Molinari, Diego, Mitsuda, Kazuhisa, Minami, Yuto, Mennella, Aniello, Matsumura, Tomotakake, Masi, Silvia, Martinez-Gonzalez, Enrique, Maki, Muneyoshi, Maffei, Buruno, Linder, Eric, Lee, Adrian, Lamagna, Luca, Kushino, Akihiro, Kurinsky, Noah, Kuo, Chao Lin, Krachmalnicoff, Nicoletta, Konishi, Kuniaki, Komatsu, Kunimoto, Komatsu, Eiichiro, Kohri, Kazunori, Kogiso, Nozomu, Kobayashi, Yohei, Kisner, Theodore, Kimura, Kimihiro, Kikuchi, Takahiro, Kibayashi, Atsuko, Keskitalo, Rijo, Kawasaki, Takeo, Katayama, Nobu, Kashima, Shingo, Kanai, Hiroaki, Arnold, Kam, Jaehnig, Greg, Ishino, Hirokazu, Imada, Hiroaki, Ichiki, Kiyotomo, Hubmayr, Johannes, Hoang, Duc Thuong, Hivon, Eric, Hirota, Yukimasa, Hill, Charles, Henrot-Versille, Sophie, Hazumi, Masashi, Hattori, Makoto, Hasegawa, Masaya, Hasebe, Takashi, Hargrave, Peter, Halverson, Nils, Gruppuso, Alessandro, Grain, Julien, Ghigna, Tommaso, Gao, Jian-Rong, Ganga, Ken, Fuskeland, Unni, Franceschet, Cristian, Flauger, Raphael, Errand, Josquin, Eriksen, Hans Kristian, Elleflot, Tucker, Ebisawa, Ken, Ducout, Anne, Duband, Lionel, Dotani, Tadayasu, Dobbs, Matthieu, de Petris, Marco, de Bernardis, Paolo, Curtis, David, Cukierman, Ari, Columbro, Fabio, Chinone, Yuji, Challinor, Anthony, Calabrese, Erminia, Bucher, Martin, Brown, Michael, Boulanger, Francois, Borill, Julian, Bersanelli, Marco, Beckman, Shawn, Basak, Soumen, Banerji, Ranajoy, Banday, Anthony, Baccigalupi, Carlo, Austermann, Jason, Aumont, Jonathan, Mangilli, Anna, Ade, Peter, Winter, B., Ota, Izumi, Noviello, Fabio, Sekimoto, Yutaro, Realini, S, Patanchon, G, Kataoka, Y, Zonca, A, Zannoni, M, Yumoto, J, Yoshida, T, Yanagisawa, M, Yamasaki, N, Yamamoto, R, Westbrook, B, Wehus, I, Watanabe, N, Vittorio, N, Utsunomiya, S, Uozumi, S, Tsujimoto, M, Tsuji, M, Tristram, M, Trappe, N, Tomida, H, Tomasi, M, Thorne, B, Thompson, K, Terao, Y, Taylor, E, Takakura, S, Takakura, H, Takaku, R, Suzuki, J, Suzuki, A, Sugiyama, S, Sugai, H, Stompor, R, Smecher, G, Signorelli, G, Shiraishi, M, Shinozaki, K, Sherwin, B, Savini, G, Sakurai, Y, Sakurai, H, Remazeilles, M, Raum, C, Puglisi, G, Poletti, D, Polenta, G, Pisano, G, Piacentini, F, Okada, N, Ohsaki, H, Ogawa, H, Ochi, H, O'Sullivan, C, Nishino, H, Nishibori, T, Natoli, P, Namikawa, T, Nakamura, S, Nagata, R, Nagai, M, Murphy, A, Murata, Y, Mot, B, Morgante, G, Montier, L, Molinari, D, Mitsuda, K, Minami, Y, Mennella, A, Matsumura, T, Masi, S, Martinez-Gonzalez, E, Maki, M, Maffei, B, Linder, E, Lee, A, Lamagna, L, Kushino, A, Kurinsky, N, Kuo, C, Krachmalnicoff, N, Konishi, K, Komatsu, K, Komatsu, E, Kohri, K, Kogiso, N, Kobayashi, Y, Kisner, T, Kimura, K, Kikuchi, T, Kibayashi, A, Keskitalo, R, Kawasaki, T, Katayama, N, Kashima, S, Kanai, H, Arnold, K, Jaehnig, G, Ishino, H, Imada, H, Ichiki, K, Hubmayr, J, Hoang, D, Hivon, E, Hirota, Y, Hill, C, Henrot-Versille, S, Hazumi, M, Hattori, M, Hasegawa, M, Hasebe, T, Hargrave, P, Halverson, N, Gruppuso, A, Grain, J, Ghigna, T, Gao, J, Ganga, K, Fuskeland, U, Franceschet, C, Flauger, R, Errand, J, Eriksen, H, Elleflot, T, Ebisawa, K, Ducout, A, Duband, L, Dotani, T, Dobbs, M, de Petris, M, de Bernardis, P, Curtis, D, Cukierman, A, Columbro, F, Chinone, Y, Challinor, A, Calabrese, E, Bucher, M, Brown, M, Boulanger, F, Borill, J, Bersanelli, M, Beckman, S, Basak, S, Banerji, R, Banday, A, Baccigalupi, C, Austermann, J, Aumont, J, Mangilli, A, Ade, P, Winter, B, Ota, I, Noviello, F, Sekimoto, Y, Realini, S., Patanchon, Guillaume, Kataoka, Yuichiro, Zonca, Andrea, Zannoni, Mario, Yumoto, Junji, Yoshida, Tetsuya, Yanagisawa, Masato, Yamasaki, Noriko, Yamamoto, Ryo, Westbrook, Benjamin, Wehus, Ingunn, Watanabe, Naoki, Vittorio, Nicola, Utsunomiya, Shin, Uozumi, Satoru, Tsujimoto, Masahiro, Tsuji, Masatoshi, Tristram, Matthieu, Trappe, Neil, Tomida, Hiroshi, Tomasi, Maurizio, Thorne, Ben, Thompson, Keith L., Terao, Yutaka, Taylor, Ellen, Takakura, Satoru, Takakura, Hayato, Takaku, Ryota, Suzuki, Junichi, Suzuki, Aritoki, Sugiyama, Shinya, Sugai, Hajime, Stompor, Radek, Smecher, Graeme, Signorelli, Giovanni, Shiraishi, Maresuke, Shinozaki, Keisuke, Sherwin, Blake, Savini, Giorgio, Sakurai, Yuki, Sakurai, Haruyuki, Remazeilles, Mathieu, Raum, Christopher, Puglisi, Giuseppe, Poletti, Davide, Polenta, Gianluca, Pisano, Giampaolo, Piacentini, Francesco, Okada, Nozomi, Ohsaki, Hiroyuki, Ogawa, Hiroyuki, Ogawa, Hideo, Ochi, Hiroki, O'Sullivan, Creidhe, Nishino, Haruki, Nishibori, Toshiyuki, Natoli, Paolo, Namikawa, Toshiya, Nakamura, Shogo, Nagata, Ryo, Nagai, Makoto, Murphy, Anthony, Murata, Yasuhiro, Mot, Baptiste, Morgante, Gianluca, Montier, Ludovic, Molinari, Diego, Mitsuda, Kazuhisa, Minami, Yuto, Mennella, Aniello, Matsumura, Tomotakake, Masi, Silvia, Martinez-Gonzalez, Enrique, Maki, Muneyoshi, Maffei, Buruno, Linder, Eric, Lee, Adrian, Lamagna, Luca, Kushino, Akihiro, Kurinsky, Noah, Kuo, Chao Lin, Krachmalnicoff, Nicoletta, Konishi, Kuniaki, Komatsu, Kunimoto, Komatsu, Eiichiro, Kohri, Kazunori, Kogiso, Nozomu, Kobayashi, Yohei, Kisner, Theodore, Kimura, Kimihiro, Kikuchi, Takahiro, Kibayashi, Atsuko, Keskitalo, Rijo, Kawasaki, Takeo, Katayama, Nobu, Kashima, Shingo, Kanai, Hiroaki, Arnold, Kam, Jaehnig, Greg, Ishino, Hirokazu, Imada, Hiroaki, Ichiki, Kiyotomo, Hubmayr, Johannes, Hoang, Duc Thuong, Hivon, Eric, Hirota, Yukimasa, Hill, Charles, Henrot-Versille, Sophie, Hazumi, Masashi, Hattori, Makoto, Hasegawa, Masaya, Hasebe, Takashi, Hargrave, Peter, Halverson, Nils, Gruppuso, Alessandro, Grain, Julien, Ghigna, Tommaso, Gao, Jian-Rong, Ganga, Ken, Fuskeland, Unni, Franceschet, Cristian, Flauger, Raphael, Errand, Josquin, Eriksen, Hans Kristian, Elleflot, Tucker, Ebisawa, Ken, Ducout, Anne, Duband, Lionel, Dotani, Tadayasu, Dobbs, Matthieu, de Petris, Marco, de Bernardis, Paolo, Curtis, David, Cukierman, Ari, Columbro, Fabio, Chinone, Yuji, Challinor, Anthony, Calabrese, Erminia, Bucher, Martin, Brown, Michael, Boulanger, Francois, Borill, Julian, Bersanelli, Marco, Beckman, Shawn, Basak, Soumen, Banerji, Ranajoy, Banday, Anthony, Baccigalupi, Carlo, Austermann, Jason, Aumont, Jonathan, Mangilli, Anna, Ade, Peter, Winter, B., Ota, Izumi, Noviello, Fabio, and Sekimoto, Yutaro

Published
2018

11. A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of POLARBEAR Data

Author

The POLARBEAR Collaboration: Ade, P. A. R., Aguilar, Mario, Akiba, Yoshiki, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beck, D., Bianchini, F., Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Crowley, K., Cukierman, Ari, Dunner, R., Dobbs, M., Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, S. M., Feng, C., Fujino, Takuro, Galitzki, Nicholas, Gilbert, A., Goeckner-Wald, Neil, Groh, J. C., Hall, G., Halverson, Nils W., Hamada, T., Hasegawa, Masaya, Hazumi, Masashi, Hill, Charles, Howe, Logan, Inoue, Yuki, Jaehnig, G., Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Katayama, Nobuhiko, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Le Jeune, M., Lee, Adrian T., Leitch, E. M., Leon, David, Linder, E., Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Minami, Y., Montgomery, J., Navaroli, Martin, Nishino, Haruki, Paar, Hans, Peloton, Julien, Pham, A. T. P., Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Richards, P. L., Ross, Colin, Segawa, Y., Sherwin, B. D., Silva-Feaver, M., Siritanasak, Praween, Stebor, N., Stompor, R., Suzuki, Aritoki, Tajima, Osamu, Takakura, S., Takatori, Sayuri, Tanabe, D., Teply, Grant P., Tomaru, T., Tucker, C., Whitehorn, N., Zahn, A., 秋葉, 祥希, 茅根, 裕司, 長谷川, 雅也, 羽澄, 昌史, 井上, 優貴, 片山, 伸彦, 松村, 知岳, 西野, 玄記, 鈴木, 有春, 田島, 治, The POLARBEAR Collaboration: Ade, P. A. R., Aguilar, Mario, Akiba, Yoshiki, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beck, D., Bianchini, F., Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Crowley, K., Cukierman, Ari, Dunner, R., Dobbs, M., Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, S. M., Feng, C., Fujino, Takuro, Galitzki, Nicholas, Gilbert, A., Goeckner-Wald, Neil, Groh, J. C., Hall, G., Halverson, Nils W., Hamada, T., Hasegawa, Masaya, Hazumi, Masashi, Hill, Charles, Howe, Logan, Inoue, Yuki, Jaehnig, G., Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Katayama, Nobuhiko, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Le Jeune, M., Lee, Adrian T., Leitch, E. M., Leon, David, Linder, E., Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Minami, Y., Montgomery, J., Navaroli, Martin, Nishino, Haruki, Paar, Hans, Peloton, Julien, Pham, A. T. P., Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Richards, P. L., Ross, Colin, Segawa, Y., Sherwin, B. D., Silva-Feaver, M., Siritanasak, Praween, Stebor, N., Stompor, R., Suzuki, Aritoki, Tajima, Osamu, Takakura, S., Takatori, Sayuri, Tanabe, D., Teply, Grant P., Tomaru, T., Tucker, C., Whitehorn, N., Zahn, A., 秋葉, 祥希, 茅根, 裕司, 長谷川, 雅也, 羽澄, 昌史, 井上, 優貴, 片山, 伸彦, 松村, 知岳, 西野, 玄記, 鈴木, 有春, and 田島, 治

Abstract

著者人数: 81名, Accepted: 2017-09-20

Published
2018

12. Performance of a continuously rotating half-wave plate on the POLARBEAR telescope

Author

Aguilar, Mario, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beckman, Shawn, Boettger, David, Borrill, Julian, Chapman, Scott, Cukierman, Ari, Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Fujino, Takuro, Galitzki, Nicholas, Goeckner-Wald, Neil, Halverson, Nils W., Hill, Charles, Howe, Logan, Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Lee, Adrian T., Leon, David, Lowry, Lindsay, Matsuda, Frederick, Navaroli, Martin, Paar, Hans, Peloton, Julien, Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Ross, Colin, Siritanasak, Praween, Takatori, Sayuri, Teply, Grant, Takakura, Satoru, Akiba, Yoshiki, Chinone, Yuji, Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Inoue, Yuki, Katayama, Nobuhiko, Matsumura, Tomotake, Nishino, Haruki, Suzuki, Aritoki, Tajima, Osamu, Institut Lagrange de Paris, Sorbonne Universités, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Takakura, S, Aguilar, M, Akiba, Y, Arnold, K, Baccigalupi, C, Barron, D, Beckman, S, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Cukierman, A, Ducout, A, Elleflot, T, Errard, J, Fabbian, G, Fujino, T, Galitzki, N, Goeckner-Wald, N, Halverson, N, Hasegawa, M, Hattori, K, Hazumi, M, Hill, C, Howe, L, Inoue, Y, Jaffe, A, Jeong, O, Kaneko, D, Katayama, N, Keating, B, Keskitalo, R, Kisner, T, Krachmalnicoff, N, Kusaka, A, Lee, A, Leon, D, Lowry, L, Matsuda, F, Matsumura, T, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Poletti, D, Puglisi, G, Reichardt, C, Ross, C, Siritanasak, P, Suzuki, A, Tajima, O, Takatori, S, Teply, G, Sorbonne Université (SU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Institut d'astrophysique spatiale ( IAS ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)

Subjects
Physics - Instrumentation and Detectors, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Cosmic microwave background, measurement methods, cosmic background radiation, 01 natural sciences, Waveplate, Atomic, law.invention, Particle and Plasma Physics, law, CMBR experiments, Stokes parameters, 010303 astronomy & astrophysics, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], physics.ins-det, Leakage (electronics), Physics, Settore FIS/05, Detector, Instrumentation and Detectors (physics.ins-det), Nuclear & Particles Physics, Cardinal point, symbols, astro-ph.CO, CMBR experiment, Astrophysics - Instrumentation and Methods for Astrophysics, Astronomical and Space Sciences, performance, Astrophysics - Cosmology and Nongalactic Astrophysics, noise, Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, temperature: fluctuation, 010309 optics, Primary mirror, Telescope, symbols.namesake, Optics, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Nuclear, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), detector: design, polarization, business.industry, Molecular, Astronomy and Astrophysics, sensitivity, optics, gravitational waves and CMBR polarization, astro-ph.IM, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

著者人数: 53名, Accepted: 2017-04-15, 資料番号: SA1170067000

Published
2017
Full Text
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13. Performance of a continuously rotating half-wave plate on the POLARBEAR telescope

Author

Takakura, Satoru, primary, Aguilar, Mario, additional, Akiba, Yoshiki, additional, Arnold, Kam, additional, Baccigalupi, Carlo, additional, Barron, Darcy, additional, Beckman, Shawn, additional, Boettger, David, additional, Borrill, Julian, additional, Chapman, Scott, additional, Chinone, Yuji, additional, Cukierman, Ari, additional, Ducout, Anne, additional, Elleflot, Tucker, additional, Errard, Josquin, additional, Fabbian, Giulio, additional, Fujino, Takuro, additional, Galitzki, Nicholas, additional, Goeckner-Wald, Neil, additional, Halverson, Nils W., additional, Hasegawa, Masaya, additional, Hattori, Kaori, additional, Hazumi, Masashi, additional, Hill, Charles, additional, Howe, Logan, additional, Inoue, Yuki, additional, Jaffe, Andrew H., additional, Jeong, Oliver, additional, Kaneko, Daisuke, additional, Katayama, Nobuhiko, additional, Keating, Brian, additional, Keskitalo, Reijo, additional, Kisner, Theodore, additional, Krachmalnicoff, Nicoletta, additional, Kusaka, Akito, additional, Lee, Adrian T., additional, Leon, David, additional, Lowry, Lindsay, additional, Matsuda, Frederick, additional, Matsumura, Tomotake, additional, Navaroli, Martin, additional, Nishino, Haruki, additional, Paar, Hans, additional, Peloton, Julien, additional, Poletti, Davide, additional, Puglisi, Giuseppe, additional, Reichardt, Christian L., additional, Ross, Colin, additional, Siritanasak, Praween, additional, Suzuki, Aritoki, additional, Tajima, Osamu, additional, Takatori, Sayuri, additional, and Teply, Grant, additional

Published
2017
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14. Making maps of cosmic microwave background polarization for B-mode studies: the POLARBEAR example

Author

Poletti, Davide, primary, Fabbian, Giulio, additional, Le Jeune, Maude, additional, Peloton, Julien, additional, Arnold, Kam, additional, Baccigalupi, Carlo, additional, Barron, Darcy, additional, Beckman, Shawn, additional, Borrill, Julian, additional, Chapman, Scott, additional, Chinone, Yuji, additional, Cukierman, Ari, additional, Ducout, Anne, additional, Elleflot, Tucker, additional, Errard, Josquin, additional, Feeney, Stephen, additional, Goeckner-Wald, Neil, additional, Groh, John, additional, Hall, Grantland, additional, Hasegawa, Masaya, additional, Hazumi, Masashi, additional, Hill, Charles, additional, Howe, Logan, additional, Inoue, Yuki, additional, Jaffe, Andrew H., additional, Jeong, Oliver, additional, Katayama, Nobuhiko, additional, Keating, Brian, additional, Keskitalo, Reijo, additional, Kisner, Theodore, additional, Kusaka, Akito, additional, Lee, Adrian T., additional, Leon, David, additional, Linder, Eric, additional, Lowry, Lindsay, additional, Matsuda, Frederick, additional, Navaroli, Martin, additional, Paar, Hans, additional, Puglisi, Giuseppe, additional, Reichardt, Christian L., additional, Ross, Colin, additional, Siritanasak, Praween, additional, Stebor, Nathan, additional, Steinbach, Bryan, additional, Stompor, Radek, additional, Suzuki, Aritoki, additional, Tajima, Osamu, additional, Teply, Grant, additional, and Whitehorn, Nathan, additional

Published
2017
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15. Concept design of the LiteBIRD satellite for CMB B-mode polarization

Author

Lystrup, Makenzie, MacEwen, Howard A., Fazio, Giovanni G., Siegler, Nicholas, Tong, Edward C., Batalha, Natalie, Realini, S., Patanchon, Guillaume, Kataoka, Yuichiro, Zonca, Andrea, Zannoni, Mario, Yumoto, Junji, Yoshida, Tetsuya, Yanagisawa, Masato, Yamasaki, Noriko, Yamamoto, Ryo, Westbrook, Benjamin, Wehus, Ingunn, Watanabe, Naoki, Vittorio, Nicola, Utsunomiya, Shin, Uozumi, Satoru, Tsujimoto, Masahiro, Tsuji, Masatoshi, Tristram, Matthieu, Trappe, Neil, Tomida, Hiroshi, Tomasi, Maurizio, Thorne, Ben, Thompson, Keith L., Terao, Yutaka, Taylor, Ellen, Takakura, Satoru, Takakura, Hayato, Takaku, Ryota, Suzuki, Junichi, Suzuki, Aritoki, Sugiyama, Shinya, Sugai, Hajime, Stompor, Radek, Smecher, Graeme, Signorelli, Giovanni, Shiraishi, Maresuke, Shinozaki, Keisuke, Sherwin, Blake, Savini, Giorgio, Sakurai, Yuki, Sakurai, Haruyuki, Remazeilles, Mathieu, Raum, Christopher, Puglisi, Giuseppe, Poletti, Davide, Polenta, Gianluca, Pisano, Giampaolo, Piacentini, Francesco, Okada, Nozomi, Ohsaki, Hiroyuki, Ogawa, Hiroyuki, Ogawa, Hideo, Ochi, Hiroki, O'Sullivan, Creidhe, Nishino, Haruki, Nishibori, Toshiyuki, Natoli, Paolo, Namikawa, Toshiya, Nakamura, Shogo, Nagata, Ryo, Nagai, Makoto, Murphy, Anthony, Murata, Yasuhiro, Mot, Baptiste, Morgante, Gianluca, Montier, Ludovic, Molinari, Diego, Mitsuda, Kazuhisa, Minami, Yuto, Mennella, Aniello, Matsumura, Tomotakake, Masi, Silvia, Martinez-Gonzalez, Enrique, Maki, Muneyoshi, Maffei, Buruno, Linder, Eric, Lee, Adrian, Lamagna, Luca, Kushino, Akihiro, Kurinsky, Noah, Kuo, Chao Lin, Krachmalnicoff, Nicoletta, Konishi, Kuniaki, Komatsu, Kunimoto, Komatsu, Eiichiro, Kohri, Kazunori, Kogiso, Nozomu, Kobayashi, Yohei, Kisner, Theodore, Kimura, Kimihiro, Kikuchi, Takahiro, Kibayashi, Atsuko, Keskitalo, Rijo, Kawasaki, Takeo, Katayama, Nobu, Kashima, Shingo, Kanai, Hiroaki, Arnold, Kam, Jaehnig, Greg, Ishino, Hirokazu, Imada, Hiroaki, Ichiki, Kiyotomo, Hubmayr, Johannes, Hoang, Duc Thuong, Hivon, Eric, Hirota, Yukimasa, Hill, Charles, Henrot-Versille, Sophie, Hazumi, Masashi, Hattori, Makoto, Hasegawa, Masaya, Hasebe, Takashi, Hargrave, Peter, Halverson, Nils, Gruppuso, Alessandro, Grain, Julien, Ghigna, Tommaso, Gao, Jian-Rong, Ganga, Ken, Fuskeland, Unni, Franceschet, Cristian, Flauger, Raphael, Errand, Josquin, Eriksen, Hans Kristian, Elleflot, Tucker, Ebisawa, Ken, Ducout, Anne, Duband, Lionel, Dotani, Tadayasu, Dobbs, Matthieu, de Petris, Marco, de Bernardis, Paolo, Curtis, David, Cukierman, Ari, Columbro, Fabio, Chinone, Yuji, Challinor, Anthony, Calabrese, Erminia, Bucher, Martin, Brown, Michael, Boulanger, Francois, Borill, Julian, Bersanelli, Marco, Beckman, Shawn, Basak, Soumen, Banerji, Ranajoy, Banday, Anthony, Baccigalupi, Carlo, Austermann, Jason, Aumont, Jonathan, Mangilli, Anna, Ade, Peter, Winter, B., Ota, Izumi, Noviello, Fabio, Sekimoto, Yutaro, Lystrup, Makenzie, MacEwen, Howard A., Fazio, Giovanni G., Siegler, Nicholas, Tong, Edward C., Batalha, Natalie, Realini, S., Patanchon, Guillaume, Kataoka, Yuichiro, Zonca, Andrea, Zannoni, Mario, Yumoto, Junji, Yoshida, Tetsuya, Yanagisawa, Masato, Yamasaki, Noriko, Yamamoto, Ryo, Westbrook, Benjamin, Wehus, Ingunn, Watanabe, Naoki, Vittorio, Nicola, Utsunomiya, Shin, Uozumi, Satoru, Tsujimoto, Masahiro, Tsuji, Masatoshi, Tristram, Matthieu, Trappe, Neil, Tomida, Hiroshi, Tomasi, Maurizio, Thorne, Ben, Thompson, Keith L., Terao, Yutaka, Taylor, Ellen, Takakura, Satoru, Takakura, Hayato, Takaku, Ryota, Suzuki, Junichi, Suzuki, Aritoki, Sugiyama, Shinya, Sugai, Hajime, Stompor, Radek, Smecher, Graeme, Signorelli, Giovanni, Shiraishi, Maresuke, Shinozaki, Keisuke, Sherwin, Blake, Savini, Giorgio, Sakurai, Yuki, Sakurai, Haruyuki, Remazeilles, Mathieu, Raum, Christopher, Puglisi, Giuseppe, Poletti, Davide, Polenta, Gianluca, Pisano, Giampaolo, Piacentini, Francesco, Okada, Nozomi, Ohsaki, Hiroyuki, Ogawa, Hiroyuki, Ogawa, Hideo, Ochi, Hiroki, O'Sullivan, Creidhe, Nishino, Haruki, Nishibori, Toshiyuki, Natoli, Paolo, Namikawa, Toshiya, Nakamura, Shogo, Nagata, Ryo, Nagai, Makoto, Murphy, Anthony, Murata, Yasuhiro, Mot, Baptiste, Morgante, Gianluca, Montier, Ludovic, Molinari, Diego, Mitsuda, Kazuhisa, Minami, Yuto, Mennella, Aniello, Matsumura, Tomotakake, Masi, Silvia, Martinez-Gonzalez, Enrique, Maki, Muneyoshi, Maffei, Buruno, Linder, Eric, Lee, Adrian, Lamagna, Luca, Kushino, Akihiro, Kurinsky, Noah, Kuo, Chao Lin, Krachmalnicoff, Nicoletta, Konishi, Kuniaki, Komatsu, Kunimoto, Komatsu, Eiichiro, Kohri, Kazunori, Kogiso, Nozomu, Kobayashi, Yohei, Kisner, Theodore, Kimura, Kimihiro, Kikuchi, Takahiro, Kibayashi, Atsuko, Keskitalo, Rijo, Kawasaki, Takeo, Katayama, Nobu, Kashima, Shingo, Kanai, Hiroaki, Arnold, Kam, Jaehnig, Greg, Ishino, Hirokazu, Imada, Hiroaki, Ichiki, Kiyotomo, Hubmayr, Johannes, Hoang, Duc Thuong, Hivon, Eric, Hirota, Yukimasa, Hill, Charles, Henrot-Versille, Sophie, Hazumi, Masashi, Hattori, Makoto, Hasegawa, Masaya, Hasebe, Takashi, Hargrave, Peter, Halverson, Nils, Gruppuso, Alessandro, Grain, Julien, Ghigna, Tommaso, Gao, Jian-Rong, Ganga, Ken, Fuskeland, Unni, Franceschet, Cristian, Flauger, Raphael, Errand, Josquin, Eriksen, Hans Kristian, Elleflot, Tucker, Ebisawa, Ken, Ducout, Anne, Duband, Lionel, Dotani, Tadayasu, Dobbs, Matthieu, de Petris, Marco, de Bernardis, Paolo, Curtis, David, Cukierman, Ari, Columbro, Fabio, Chinone, Yuji, Challinor, Anthony, Calabrese, Erminia, Bucher, Martin, Brown, Michael, Boulanger, Francois, Borill, Julian, Bersanelli, Marco, Beckman, Shawn, Basak, Soumen, Banerji, Ranajoy, Banday, Anthony, Baccigalupi, Carlo, Austermann, Jason, Aumont, Jonathan, Mangilli, Anna, Ade, Peter, Winter, B., Ota, Izumi, Noviello, Fabio, and Sekimoto, Yutaro

16. A Measurement of the Cosmic Microwave Background B -mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data

Author

The, POLARBEAR Collaboration, Ade, P. A. R., Aguilar, Mario, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beck, D., Bianchini, F., Boettger, David, Borrill, Julian, Chapman, Scott, Crowley, K., Cukierman, Ari, Dunner, R., Dobbs, M., Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, S. M., Feng, C., Fujino, Takuro, Galitzki, Nicholas, Gilbert, A., Goeckner-Wald, Neil, Groh, J. C., Hall, G., Halverson, Nils W., Hamada, T., Hill, Charles, Howe, Logan, Jaehnig, G., Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Le, Jeune M., Lee, Adrian T., Leitch, E. M., Leon, David, Linder, E., Lowry, Lindsay, Matsuda, Frederick, Minami, Y., Montgomery, J., Navaroli, Martin, Paar, Hans, Peloton, Julien, Pham, A. T. P., Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Richards, P. L., Ross, Colin, Segawa, Y., Sherwin, B. D., Silva-Feaver, M., Siritanasak, Praween, Stebor, N., Stompor, R., Takakura, S., Takatori, Sayuri, Tanabe, D., Teply, Grant P., Tomaru, T., Tucker, C., Whitehorn, N., Zahn, A., Akiba, Yoshiki, Chinone, Yuji, Hasegawa, Masaya, Hazumi, Masashi, Inoue, Yuki, Katayama, Nobuhiko, Matsumura, Tomotake, Nishino, Haruki, Suzuki, Aritoki, Tajima, Osamu, Ade, P, 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, Dunner, R, Dobbs, M, Ducout, A, Elleflot, T, Errard, J, Fabbian, G, Feeney, S, Feng, C, Fujino, T, Galitzki, N, Gilbert, A, Goeckner-Wald, N, Groh, J, Hall, G, Halverson, N, Hamada, T, Hasegawa, M, Hazumi, M, Hill, C, Howe, L, Inoue, Y, Jaehnig, G, Jaffe, A, Jeong, O, Kaneko, D, Katayama, N, Keating, B, Keskitalo, R, Kisner, T, Krachmalnicoff, N, Kusaka, A, Jeune, M, Lee, A, Leitch, E, Leon, D, Linder, E, Lowry, L, Matsuda, F, Matsumura, T, Minami, Y, Montgomery, J, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Pham, A, Poletti, D, Puglisi, G, Reichardt, C, Richards, P, Ross, C, Segawa, Y, Sherwin, B, Silva-Feaver, M, Siritanasak, P, Stebor, N, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Takatori, S, Tanabe, D, Teply, G, Tomaru, T, Tucker, C, Whitehorn, N, and Zahn, A

Subjects
Cold dark matter, 0306 Physical Chemistry (Incl. Structural), Cosmic microwave background, Cosmic background radiation, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, cosmic background radiation, Astronomy & Astrophysics, 01 natural sciences, 0305 Organic Chemistry, Atomic, Physical Chemistry, symbols.namesake, Particle and Plasma Physics, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Nuclear, Planck, 010303 astronomy & astrophysics, QC, QB, Physics, large-scale structure of universe, Science & Technology, cosmology: observation, 010308 nuclear & particles physics, Settore FIS/05, Spectral density, Molecular, Astronomy and Astrophysics, Polarization (waves), observations [cosmology], 0201 Astronomical And Space Sciences, Amplitude, Gravitational lens, Space and Planetary Science, cosmology: observations, Physical Sciences, symbols, astro-ph.CO, High Energy Physics::Experiment, Astronomical and Space Sciences, Physical Chemistry (incl. Structural)
Abstract

著者人数: 81名, Accepted: 2017-09-20, 資料番号: SA1170175000

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