1,981 results on '"S. S. Sasaki"'
Search Results
2. A Photometric Survey for Lyα–He<scp>ii</scp>Dual Emitters: Searching for Population III Stars in High‐Redshift Galaxies
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Matthew A. Malkan, Yasuhiro Shioya, Celestine Grady, Daniel Schaerer, Chun Ly, Takashi Murayama, Nobunari Kashikawa, Kentaro Motohara, Tohru Nagao, Yoshiaki Taniguchi, S. S. Sasaki, Roberto Maiolino, Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), and Université Fédérale Toulouse Midi-Pyrénées
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Hubble Deep Field ,Metallicity ,Population ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,01 natural sciences ,Cosmology: Early Universe ,Stars: Early-Type ,Galaxies: Evolution ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,education ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Physics ,education.field_of_study ,010308 nuclear & particles physics ,Astrophysics (astro-ph) ,Galaxies: Formation ,Astronomy and Astrophysics ,Galaxy ,Redshift ,Galaxies: Starburst ,Stars ,Star cluster ,Space and Planetary Science ,[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] ,Astrophysics::Earth and Planetary Astrophysics ,Subaru Telescope - Abstract
We present a new photometric search for high-z galaxies hosting Population III (PopIII) stars based on deep intermediate-band imaging observations obtained in the Subaru Deep Field (SDF), by using Suprime-Cam on the Subaru Telescope. By combining our new data with the existing broad-band and narrow-band data, we searched for galaxies which emit strongly both in Ly_alpha and in HeII 1640 (``dual emitters'') that are promising candidates for PopIII-hosting galaxies, at 3.93 2 Msun/yr was found by our photometric search in 4.03 x 10^5 Mpc^3 in the SDF. This result disfavors low feedback models for PopIII star clusters, and implies an upper-limit of the PopIII SFR density of SFRD_PopIII < 5 x 10^-6 Msun/yr/Mpc^3. This new selection method to search for PopIII-hosting galaxies should be useful in future narrow-band surveys to achieve the first observational detection of PopIII-hosting galaxies at high redshifts., Comment: 24 pages, 10 figures, accepted for publication in ApJ
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- 2008
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3. The Hα Luminosity Function and Star Formation Rate atz≈ 0.24 in the COSMOS 2 Square Degree Field
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A. Leauthaud, A. Nakajima, Nick Scoville, J. P. Kneib, Takashi Murayama, Y. Taniguchi, Richard Massey, Eva Schinnerer, S. J. Lilly, Patrick L. Shopbell, S. Mihara, D. B. Sanders, Masaru Ajiki, G. Hasinger, Alvio Renzini, M. Giavalisco, Jason Rhodes, H. Aussel, M. I. Takahashi, S. S. Sasaki, Y. Shioya, Y. Ideue, M. Rich, Chris Impey, Bahram Mobasher, Luigi Guzzo, Tohru Nagao, and O. LeFevre
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Physics ,010308 nuclear & particles physics ,Astronomy and Astrophysics ,Astrophysics ,Correlation function (quantum field theory) ,Lambda ,01 natural sciences ,Power law ,Redshift ,Galaxy ,Luminosity ,Square degree ,Space and Planetary Science ,0103 physical sciences ,010303 astronomy & astrophysics ,Luminosity function (astronomy) - Abstract
To derive a new H$\alpha$ luminosity function and to understand the clustering properties of star-forming galaxies at $z \approx 0.24$, we have made a narrow-band imaging survey for H$\alpha$ emitting galaxies in the HST COSMOS 2 square degree field. We used the narrow-band filter NB816 ($\lambda_c = 8150$ \AA, $\Delta \lambda = 120$ \AA) and sampled H$\alpha$ emitters with $EW_{\rm obs}(\rm H\alpha + [N\textsc{ii}]) > 12$ \AA in a redshift range between $z=0.233$ and $z=0.251$ corresponding to a depth of 70 Mpc. We obtained 980 H$\alpha$ emitting galaxies in a sky area of 5540 arcmin$^2$, corresponding to a survey volume of $3.1 \times 10^4 {\rm Mpc^3}$. We derive a H$\alpha$ luminosity function with a best-fit Schechter function parameter set of $\alpha = -1.35^{+0.11}_{-0.13}$, $\log\phi_* = -2.65^{+0.27}_{-0.38}$, and $\log L_* ({\rm erg s^{-1}}) = 41.94^{+0.38}_{-0.23}$. The H$\alpha$ luminosity density is $2.7^{+0.7}_{-0.6} \times 10^{39}$ ergs s$^{-1}$ Mpc$^{-3}$. After subtracting the AGN contribution (15 %) to the H$\alpha$ luminosity density, the star formation rate density is evaluated as $1.8^{+0.7}_{-0.4} \times 10^{-2}$ $M_{\sun}$ yr$^{-1}$ Mpc$^{-3}$. The angular two-point correlation function of H$\alpha$ emitting galaxies of $\log L({\rm H\alpha}) > 39.8$ is well fit by a power law form of $w(\theta) = 0.013^{+0.002}_{-0.001} \theta^{-0.88 \pm 0.03}$, corresponding to the correlation function of $\xi(r) = (r/1.9{\rm Mpc})^{-1.88}$. We also find that the H$\alpha$ emitters with higher H$\alpha$ luminosity are more strongly clustered than those with lower luminosity.
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- 2008
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4. COSMOS Morphological Classification with the Zurich Estimator of Structural Types (ZEST) and the Evolution Since z = 1 of the Luminosity Function of Early, Disk, and Irregular Galaxies
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A. Leauthaud, Christian Maier, Yasuhiro Shioya, Cristiano Porciani, Masaru Ajiki, Herve Aussel, Nick Scoville, Kartik Sheth, M. T. Sargent, Richard Massey, P. Kampczyk, C. M. Carollo, Robert Feldmann, Jean-Paul Kneib, H. J. McCracken, Anton M. Koekemoer, D. Thompson, Simon J. Lilly, Yoshiaki Taniguchi, L. A. M. Tasca, Peter Capak, D. B. Sanders, Claudia Scarlata, T. Murayama, Alvio Renzini, S. S. Sasaki, Jason Rhodes, Bahram Mobasher, M. I. Takahashi, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), and Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
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Physics ,Zest ,Cosmology: Dark Matter ,Galaxies: Formation ,Dark matter ,Astrophysics::Instrumentation and Methods for Astrophysics ,Estimator ,Astronomy ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Surveys ,Cosmology: Observations ,Galaxy ,Redshift ,Cosmology: Large-Scale Structure of Universe ,[SDU]Sciences of the Universe [physics] ,Space and Planetary Science ,Galaxies: Evolution ,Galaxy formation and evolution ,Surface brightness ,Irregular galaxy ,Astrophysics::Galaxy Astrophysics - Abstract
International audience; Motivated by the desire to reliably and automatically classify structure of thousands of COSMOS galaxies, we present ZEST, the Zurich Estimator of Structural Types. To classify galaxy structure, ZEST uses (1) five nonparametric diagnostics: asymmetry, concentration, Gini coefficient, second-order moment of the brightest 20% of galaxy pixels, and ellipticity; and (2) the exponent n of single-Sérsic fits to the two-dimensional surface brightness distributions. To fully exploit the wealth of information while reducing the redundancy present in these diagnostics, ZEST performs a principal component (PC) analysis. We use a sample of ~56,000 IAB1, PC2, and PC3. We demonstrate the robustness of the ZEST grid on the z=0 sample of Frei et al. The ZEST classification breaks most of the degeneracy between different galaxy populations that affects morphological classifications based on only some of the diagnostics included in ZEST. As a first application, we present the evolution since z~1 of the luminosity functions (LFs) of COSMOS galaxies of early, disk, and irregular galaxies and, for disk galaxies, of different bulge-to-disk ratios. Overall, we find that the LF up to a redshift z=1 is consistent with a pure luminosity evolution (of about 0.95 mag at z~0.7). We highlight, however, two trends that are in general agreement with a downsizing scenario for galaxy formation, i.e., (1) a deficit of a factor of about 2 at z~0.7 of MB>-20.5 structurally classified early-type galaxies and (2) an excess of a factor of about 3, at a similar redshift, of irregular galaxies. Based on observations with the NASA/ESA Hubble Space Telescope , obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy (AURA), Inc., under NASA contract NAS 5-26555 also based on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan; Kitt Peak National Observatory, Cerro Tololo Inter-American Observatory, and the National Optical Astronomy Observatory, which are operated by AURA, Inc., under cooperative agreement with the National Science Foundation; and the Canada-France-Hawaii Telescope operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique de France, and the University of Hawaii.
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- 2007
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5. Radio and Millimeter Properties of z ∼ 5.7 Lyα Emitters in the COSMOS Field: Limits on Radio AGNs, Submillimeter Galaxies, and Dust Obscuration
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Y. Shioya, Y. Taniguchi, Masaru Ajiki, S. S. Sasaki, James E. Aguirre, Frank Bertoldi, Andrew Blain, Tohru Nagao, D. B. Sanders, T. Murayam, Nick Scoville, V. Smolcic, Chris Carilli, R. Wang, and Eva Schinnerer
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Physics ,Field (physics) ,Space and Planetary Science ,Star formation ,Astronomy and Astrophysics ,Millimeter ,Astrophysics ,Full sample ,Galaxy ,Noise (radio) - Abstract
We present observations at 1.4 and 250 GHz of the $z\sim 5.7$ Ly$\alpha$ emitters (LAE) in the COSMOS field found by Murayama et al.. At 1.4 GHz there are 99 LAEs in the lower noise regions of the radio field. We do not detect any individual source down to 3$\sigma$ limits of $\sim 30\mu$Jy beam$^{-1}$ at 1.4 GHz, nor do we detect a source in a stacking analysis, to a 2$\sigma$ limit of $2.5\mu$Jy beam$^{-1}$. At 250 GHz we do not detect any of the 10 LAEs that are located within the central regions of the COSMOS field covered by MAMBO ($20' \times 20'$) to a typical 2$\sigma$ limit of $S_{250} 6\times 10^{24}$ W Hz$^{-1}$ in the LAE sample. The radio and millimeter observations also rule out any highly obscured, extreme starbursts in the sample, ie. any galaxies with massive star formation rates $> 1500$ M$_\odot$ year$^{-1}$ in the full sample (based on the radio data), or 500 M$_\odot$ year$^{-1}$ for the 10% of the LAE sample that fall in the central MAMBO field. The stacking analysis implies an upper limit to the mean massive star formation rate of $\sim 100$ M$_\odot$ year$^{-1}$.
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- 2007
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6. Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field
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T. Murayama, Y. Taniguchi, N. Z. Scoville, M. Ajiki, D. B. Sanders, B. Mobasher, H. Aussel, P. Capak, A. Koekemoer, Y. Shioya, T. Nagao, C. Carilli, R. S. Ellis, B. Garilli, M. Giavalisco, M. G. Kitzbichler, O. LeFevre, D. Maccagni, E. Schinnerer, V. Smolcic, S. Tribiano, Y. Komiyama, S. Miyazaki, S. S. Sasaki, J. Koda, H. Karoji, CIMATTI, ANDREA, T. Murayama, Y. Taniguchi, N. Z. Scoville, M. Ajiki, D. B. Sander, B. Mobasher, H. Aussel, P. Capak, A. Koekemoer, Y. Shioya, T. Nagao, C. Carilli, R. S. Elli, B. Garilli, M. Giavalisco, M. G. Kitzbichler, O. LeFevre, D. Maccagni, E. Schinnerer, V. Smolcic, S. Tribiano, A. Cimatti, Y. Komiyama, S. Miyazaki, S. S. Sasaki, J. Koda, and H. Karoji
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Cosmology: Early Universe ,Cosmology: Observation ,Galaxies: Evolution ,Galaxies: Formation ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
We present results from a narrow-band optical survey of a contiguous area of 1.95 deg^2, covered by the Cosmic Evolution Survey (COSMOS). Both optical narrow-band (lambda_c = 8150 AA and Delta_lambda = 120 AA) and broad-band (B, V, g', r', i', and z') imaging observations were performed with the Subaru prime-focus camera, Suprime-Cam on the Subaru Telescope. We provide the largest contiguous narrow-band survey, targetting Ly alpha emitters (LAEs) at z~5.7. We find a total of 119 LAE candidates at z~5.7. Over the wide-area covered by this survey, we find no strong evidence for large scale clustering of LAEs. We estimate a star formation rate (SFR) density of ~7*10^-4 M_sun yr^-1 Mpc^-3 for LAEs at z~5.7, and compare it with previous measurements., 26 pages, 19 figures. to appear in the ApJ Supplement COSMOS Special Issue
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- 2007
7. Erratum: 'Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field' (2009, ApJ, 696, 546)
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Vernesa Smolčić, Tohru Nagao, B. Garilli, Takashi Murayama, Herve Aussel, Yoshi Taniguchi, T. Saito, O. LeFevre, Peter Capak, A. Nakajima, D. B. Sanders, Y. Ideue, Eva Schinnerer, Richard S. Ellis, Chris Carilli, Kenta Matsuoka, Mauro Giavalisco, Nick Scoville, Jeyhan S. Kartaltepe, Anton M. Koekemoer, S. S. Sasaki, Chris Impey, Yasuhiro Shioya, Jonathan R. Trump, Bahram Mobasher, and Manfred G. Kitzbichler
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Physics ,Field (physics) ,Space and Planetary Science ,Astronomy and Astrophysics ,Astrophysics ,photometric properties ,Square degree - Abstract
This is an erratum for the article 2009 ApJ 696 546.
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- 2009
8. Photometric properties of Ly alpha emitters at z=4.86 in the COSMOS 2 square degree field
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Anton M. Koekemoer, T. Saito, Y. Shioya, Jonathan R. Trump, M. Giavalisco, Peter Capak, O. LeFevre, D. B. Sanders, H. Aussel, A. Nakajima, Bahram Mobasher, Chris Carilli, Manfred G. Kitzbichler, Tohru Nagao, Nick Scoville, V. Smolcic, Eva Schinnerer, Chris Impey, S. S. Sasaki, J. Kartaltepe, K. Matsuoka, Takashi Murayama, Y. Ideue, Richard S. Ellis, B. Garilli, and Yoshiaki Taniguchi
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Physics ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Field (physics) ,PRIRODNE ZNANOSTI. Fizika. Astronomija i astrofizika ,Flux ,FOS: Physical sciences ,Astronomy and Astrophysics ,Cosmic variance ,Astrophysics ,Correlation function (astronomy) ,Lambda ,Square degree ,galaxies: distances and redshifts ,galaxies: evolution ,galaxies: luminosity function ,mass function ,Space and Planetary Science ,NATURAL SCIENCES. Physics. Astronomy and Astrophysics ,distances and redshifts [galaxies] ,Luminosity function ,evolution [galaxies] ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Line (formation) ,luminosity function [galaxies] - Abstract
We present results of a survey for Ly alpha emitters at z=4.86 based on optical narrowband (lambda_c=7126 angstrom, Delta lambda=73 angstrom) and broadband (B, V, r', i', and z') observations of the Cosmic Evolution Survey (COSMOS) field using Suprime-Cam on the Subaru Telescope. We find 79 LAE candidates at z=4.86 over a contiguous survey area of 1.83 deg^2, down to the Ly alpha line flux of 1.47 x 10^-17 ergs s^-1 cm^-2. We obtain the Ly alpha luminosity function with a best-fit Schechter parameters of log L^*=42.9^+0.5_-0.3 ergs s^-1 and phi^* = 1.2^+8.0_-1.1 x 10^-4 Mpc^-3 for alpha=-1.5 (fixed). The two-point correlation function for our LAE sample is xi(r) = (r/4.4^+5.7_-2.9 Mpc)^-1.90+/-0.22. In order to investigate the field-to-field variations of the properties of Ly alpha emitters, we divide the survey area into nine tiles of 0.5^circ x 0.5^circ each. We find that the number density varies with a factor of ~ 2 from field to field with high statistical significance. However, we find no significant field-to-field variance when we divide the field into four tiles with 0.7^circ x 0.7^circ each. We conclude that at least 0.5 deg^2 survey area is required to derive averaged properties of LAEs at z~5, and our survey field is wide enough to overcome the cosmic variance., Comment: 24 pages, 13 figures, 4 tables, uses emulateapj sty, accepted for publication in ApJ
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- 2009
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9. Hubble Space Telescope/Advanced Camera for Surveys Morphology of Lyα Emitters at Redshift 5.7 in the COSMOS Field
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Tohru Nagao, O. Le Fevre, Herve Aussel, Peter Capak, Yoshi Taniguchi, Takashi Murayama, Claudia Scarlata, Bahram Mobasher, S. Tribiano, Nick Scoville, Y. Ideue, Jonathan R. Trump, Richard S. Ellis, Anton M. Koekemoer, O. Ilbert, Mara Salvato, H. J. McCracken, B. Garilli, Andrea Cimatti, Chris Carilli, David B. Sanders, Mauro Giavalisco, Kenta Matsuoka, Eva Schinnerer, Vernesa Smolčić, S. S. Sasaki, Chris Impey, Yasuhiro Shioya, T. Saito, A. Nakajima, Manfred G. Kitzbichler, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), and Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
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Physics ,Brightness ,Astronomy ,Astronomy and Astrophysics ,Astrophysics ,Advanced Camera for Surveys ,early universe ,Cosmology ,Galaxy ,Redshift ,galaxies: high-redshift ,[SDU]Sciences of the Universe [physics] ,Space and Planetary Science ,cosmology: observations ,Hubble space telescope ,Galaxy formation and evolution ,galaxies: formation ,Surface brightness ,galaxies: evolution - Abstract
International audience; We present detailed morphological properties of Lyα emitters (LAEs) at z ≈ 5.7 in the COSMOS field based on Hubble Space Telescope Advanced Camera for Surveys (ACS) data. The ACS imaging in the F814W filter covered 85 LAEs of the 119 LAEs identified in the full two square degree field, and 47 LAEs of them are detected in the ACS images. Nearly half of them are spatially extended with a size larger than 0.15 arcsec (~0.88 kpc at z = 5.7) and up to 0.4 arcsec (~2.5 kpc at z = 5.7). The others are nearly unresolved compact objects. Two LAEs show double-component structures indicating interaction or merging of building components to form more massive galaxies. By stacking the ACS images of all the detected sources, we obtain a Sersic parameter of n ~ 0.7 with a half-light radius of 0.13 arcsec (0.76 kpc), suggesting that the majority of ACS detected LAEs have not spheroidal-like but disk-like or irregular light profiles. Comparing ACS F814W magnitudes (I 814) with Subaru/Suprime-Cam magnitudes in the NB816, i', and z' bands, we find that the ACS imaging in the F814W band mainly probes UV continuum rather than Lyα line emission. UV continuum sizes tend to be larger for LAEs with larger Lyα emission regions as traced by the NB816 imaging. The nondetection of 38 LAEs in the ACS images is likely due to the fact that their surface brightness is too low both in the UV continuum and Lyα emission. Estimating I 814 for the ACS-undetected LAEs from the z' and NB816 magnitudes, we find that 16 of these are probably LAEs with a size larger than 0.15 arcsec in UV continuum. All these results suggest that our LAE sample contains systematically larger LAEs in UV continuum size than those previously studied at z ~ 6. Based on observations with NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555; and also based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.
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- 2009
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10. Photometric redshift and classification for the XMM-COSMOS sources
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M. Mignoli, J. Silvermann, Jeyhan S. Kartaltepe, A. Rau, A. Buongiorno, Mara Salvato, M. Bolzonella, David Schiminovich, Roberto Gilli, H. J. McCracken, Knud Jahnke, G. Zamorani, Patrick J. McCarthy, R. Cook, Y. Shioya, Stephane Arnouts, Nico Cappelluti, Yoshiaki Taniguchi, Karina Caputi, M. Zamojski, Peter Capak, D. B. Sanders, Jonathan R. Trump, Chris Impey, E. Le Floc'h, G. Hasinger, Vernesa Smolčić, T. Murayama, Nick Scoville, F. Lamareille, S. J. Lilly, Francesca Civano, O. Ilbert, Jason Surace, Bahram Mobasher, Martin Elvis, David R. Thompson, Meg Urry, Marcella Brusa, H. Aussel, S. S. Sasaki, Patrick L. Shopbell, Vincenzo Mainieri, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), M. Salvato, G. Hasinger, O. Ilbert, G. Zamorani, M. Brusa, N. Z. Scoville, A. Rau, P. Capak, S. Arnout, H. Aussel, M. Bolzonella, A. Buongiorno, N. Cappelluti, K. Caputi, F. Civano, R. Cook, M. Elvi, R. Gilli, K. Jahnke, J. S. Kartaltepe, C. D. Impey, F. Lamareille, E. L. Floc'h, S. Lilly, V. Mainieri, P. McCarthy, H. McCracken, M. Mignoli, B. Mobasher, T. Murayama, S. Sasaki, D. B. Sander, D. Schiminovich, Y. Shioya, P. Shopbell, J. Silverman, V. Smolčić, J. Surace, Y. Taniguchi, D. Thompson, J. R. Trump, M. Urry, M. Zamojski, and Beaussier, Catherine
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QSOS ,catalog ,Astrophysics::High Energy Astrophysical Phenomena ,galaxies: active ,FOS: Physical sciences ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Photometry (optics) ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,catalogs ,methods: miscellaneous ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Photometric redshift ,Physics ,010308 nuclear & particles physics ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,Sigma ,Astronomy and Astrophysics ,Galaxy ,Redshift ,Stars ,[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Space and Planetary Science ,Spectral energy distribution ,Astrophysics::Earth and Planetary Astrophysics - Abstract
We present photometric redshifts and spectral energy distribution (SED) classifications for a sample of 1542 optically identified sources detected with XMM in the COSMOS field. Our template fitting classifies 46 sources as stars and 464 as non-active galaxies, while the remaining 1032 require templates with an AGN contribution. High accuracy in the derived photometric redshifts was accomplished as the result of 1) photometry in up to 30 bands with high significance detections, 2) a new set of SED templates including 18 hybrids covering the far-UV to mid-infrared, which have been constructed by the combination of AGN and non-active galaxies templates, and 3) multi-epoch observations that have been used to correct for variability (most important for type 1 AGN). The reliability of the photometric redshifts is evaluated using the sub-sample of 442 sources with measured spectroscopic redshifts. We achieved an accuracy of $\sigma_{\Delta z/(1+z_{spec})} = 0.014$ for i$_{AB}^*, Comment: Accepted for publication in ApJ
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- 2008
11. COSMOS Photometric Redshifts with 30-bands for 2-deg2
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Peter Capak, A. Leauthaud, V. Le Brun, Herve Aussel, Daniela Vergani, David Schiminovich, H. J. McCracken, M. Zamojski, Mara Salvato, F. Lamareille, O. Le Fèvre, G. Zamorani, Masayuki Tanaka, Stéphane Arnouts, Lidia Tasca, David B. Sanders, Yasuhiro Shioya, S. de la Torre, E. Le Floc'h, P. Franzetti, P. Kampczyk, Yoshiaki Taniguchi, C. Knobel, Marcella Brusa, Olga Cucciati, M. Bolzonella, Bianca Garilli, S. Bardelli, Simon J. Lilly, Olivier Ilbert, Guenther Hasinger, Karina Caputi, Alvio Renzini, A. Iovino, Bahram Mobasher, C. M. Carollo, David R. Thompson, A. Bongiorno, N. Z. Scoville, Christian Maier, T. Murayama, S. S. Sasaki, Jean-Paul Kneib, Jeyhan S. Kartaltepe, E. Perez-Montero, Graziano Coppa, R. Pello, E. Zucca, M. Mignoli, Vincenzo Mainieri, Marco Scodeggio, Yannick Mellier, L. de Ravel, Laurence Tresse, E. Ricciardelli, Yingjie Peng, K. Kovac, Dagny L. Looper, J. F. Le Borgne, T. Contini, John D. Silverman, R. Cook, Jason Surace, Institut d'Astrophysique et de Géophysique [Liège], Université de Liège, INAF - Osservatorio Astronomico di Bologna (OAB), Istituto Nazionale di Astrofisica (INAF), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), California Institute of Technology (CALTECH), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, AUTRES, Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Observatoire de Paris - Site de Paris (OP), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Space Telescope Science Institute (STSci), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées (LATT), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Statistique de l'ENS (LPS), Université Paris Diderot - Paris 7 (UPD7)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), School of Biological Sciences, University of Liverpool, National Institute of Water and Atmospheric Research [Christchurch] (NIWA), National Institute of Water and Atmospheric Research [Wellington] (NIWA), INAF - Osservatorio Astronomico di Capodimonte (OAC), INAF - Osservatorio Astronomico di Brera (OAB), INAF - Osservatorio Astronomico di Bologna (OABO), Università di Bologna, Dipartimento di Astronomia, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), University of Chicago, Dipartimento di Fisica, Università degli Studi di Milano-Bicocca [Milano] (UNIMIB)-Università degli Studi di Milano [Milano] (UNIMI), Services communs OMP (UMS 831), Departement de Radioastronomie Millimétrique (DEMIRM), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Institute of Astronomy [ETH Zürich], Department of Physics [ETH Zürich] (D-PHYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)- Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Information Science Laboratory, Tokai University, Japan Atomic Energy Agency, INAF - Osservatorio Astrofisico di Arcetri (OAA), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB)-Università degli Studi di Milano = University of Milan (UNIMI), Beaussier, Catherine, Ilbert O., Capak P., Salvato M., Aussel H., McCracken H. J., Sanders D. B., Scoville N., Kartaltepe J., Arnouts S., Le Floc'h E., Mobasher B., Taniguchi Y., Lamareille F., Leauthaud A., Sasaki S., Thompson D., Zamojski M., Zamorani G., Bardelli S., Bolzonella M., Bongiorno A., Brusa M., Caputi K. I., Carollo C. M., Contini T., Cook R., Coppa G., Cucciati O., de la Torre S., de Ravel L., Franzetti P., Garilli B., Hasinger G., Iovino A., Kampczyk P., Kneib J.-P., Knobel C., Kovac K., Le Borgne J. F., Le Brun V., Fèvre O. Le, Lilly S., Looper D., Maier C., Mainieri V., Mellier Y., Mignoli M., Murayama T., Pellò R., Peng Y., Pérez-Montero E., Renzini A., Ricciardelli E., Schiminovich D., Scodeggio M., Shioya Y., Silverman J., Surace J., Tanaka M., Tasca L., Tresse L., Vergani D., and Zucca E.
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Physics ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,010308 nuclear & particles physics ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Sigma ,Spectral density ,Astronomy and Astrophysics ,Astrophysics ,[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph] ,7. Clean energy ,01 natural sciences ,Redshift ,Galaxy ,GALAXIES: SURVEYS ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,galaxies: luminosity function ,Space and Planetary Science ,[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,0103 physical sciences ,Scale structure ,Emission spectrum ,galaxies: evolution ,010303 astronomy & astrophysics - Abstract
We present accurate photometric redshifts in the 2-deg2 COSMOS field. The redshifts are computed with 30 broad, intermediate, and narrow bands covering the UV (GALEX), Visible-NIR (Subaru, CFHT, UKIRT and NOAO) and mid-IR (Spitzer/IRAC). A chi2 template-fitting method (Le Phare) was used and calibrated with large spectroscopic samples from VLT-VIMOS and Keck-DEIMOS. We develop and implement a new method which accounts for the contributions from emission lines (OII, Hbeta, Halpha and Ly) to the spectral energy distributions (SEDs). The treatment of emission lines improves the photo-z accuracy by a factor of 2.5. Comparison of the derived photo-z with 4148 spectroscopic redshifts (i.e. Delta z = zs - zp) indicates a dispersion of sigma_{Delta z/(1+zs)}=0.007 at i, Comment: 21 pages, 14 figures, and 3 tables ; accepted for publication in ApJ
- Published
- 2008
12. High-redshift Ly alpha emitters with a large equivalent width: Properties of i-dropout galaxies with an NB921-band depression in the Subaru Deep Field
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Masaru Ajiki, Yoshi Taniguchi, Takashi Murayama, M. A. Malkan, Kentaro Motohara, Alessandro Marconi, Tohru Nagao, Kunihiro Ohta, Yasuhiro Shioya, Chun Ly, S. S. Sasaki, Nobunari Kashikawa, Roberto Maiolino, and Takashi Hattori
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Physics ,Stellar population ,Hubble Deep Field ,Metallicity ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Redshift ,Galaxy ,Space and Planetary Science ,Galaxy formation and evolution ,Emission spectrum ,Equivalent width ,Astrophysics::Galaxy Astrophysics - Abstract
We report new follow-up spectroscopy of i-dropout galaxies with an NB921-band depression found in the Subaru Deep Field. The NB921-depressed i-dropout selection method is expected to select galaxies with large equivalent width Ly alpha emission over a wide redshift range, 6.0, Comment: 9 pages, 5 figures, accepted for publication in A&A
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- 2007
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13. The Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA) and its first application: COSMOS
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H. J. McCracken, Nick Scoville, Y. Taniguchi, O. Le Fevre, G. Zamorani, Takashi Murayama, T. Contini, S. J. Lilly, Bahram Mobasher, C. M. Carollo, Marco Scodeggio, David R. Thompson, Alvio Renzini, M. I. Takahashi, H. Aussel, Y. Shioya, S. S. Sasaki, Masaru Ajiki, Peter Capak, D. B. Sanders, John D. Silverman, Robert Feldmann, C. Scarlata, Cristiano Porciani, Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Institute for Astronomy, Department of Physics, ETH Zürich, Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Subaru Telescope, Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Università degli Studi di Padova = University of Padua (Unipd), Astronomical Institute, Tohoku University, Institute for Astronomy, University of Hawaii, Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Space Telescope Science Institute (STScI), Istituto di Astrofisica Spaziale e Fisica Cosmica (IASF-Milano), Physics Department, Graduate School of Science, Ehime University, Max-Planck-Institut für Extraterrestriche Physik (MPE), INAF-Osservatorio Astronomico di Bologna (OABO), and Beaussier, Catherine
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Spectrum analyzer ,Maximum likelihood ,Bayesian probability ,statistical ,galaxies: distances and redshifts ,galaxies: evolution ,galaxies: formation ,galaxies: photometry [methods] ,FOS: Physical sciences ,Probability density function ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Photometry (optics) ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,0103 physical sciences ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Physics ,methods: statistical ,Training set ,010308 nuclear & particles physics ,Astrophysics (astro-ph) ,Astronomy and Astrophysics ,Galaxy ,Redshift ,galaxies: photometry ,[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Space and Planetary Science ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] - Abstract
Monthly Notices of the Royal Astronomical Society, 372 (2), ISSN:0035-8711, ISSN:1365-2966, ISSN:1365-8711
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- 2006
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14. The Intermediate-band Dropout Method: A New Method to Search for High-Redshift Galaxies
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Takashi Murayama, Ryoko Sumiya, Tohru Nagao, Yuichiro Hatakeyama, Masaru Ajiki, S. S. Sasaki, Yoshiaki Taniguchi, and Yasuhiro Shioya
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Physics ,Dropout (communications) ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Imaging data ,Galaxy ,Redshift ,Stars ,Wavelength ,Intermediate band ,Space and Planetary Science ,Subaru Telescope ,Astrophysics::Galaxy Astrophysics - Abstract
We propose a new method to search for high-redshift galaxies that is based on an intermediate-band dropout technique rather than the usual broad-band dropout one. In this method, we use an intermediate-band filter whose central wavelength is longer than 7000 \AA. This new method makes it possible to distinguish both very late-type stars such as L and T dwarfs and dusty galaxies at intermediate redshift from real high-$z$ Lyman break galaxies. The reason for this is that such interlopers do not show strong intermediate-band depression although they have very red broad-band colors that are indicative of Lyman break galaxies. Applying our new method to imaging data sets obtained with the Suprime-Cam on the Subaru Telescope, we find a new sample of Lyman break galaxies at $z \simeq 5$., Comment: 15 pages, 5 figures, PASJ, Vol.57, No.2, in press
- Published
- 2005
15. P-selectin blockade does not impair leukocyte host defense against bacterial peritonitis and soft tissue infection in rabbits
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S R, Sharar, S S, Sasaki, L C, Flaherty, J C, Paulson, J M, Harlan, and R K, Winn
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P-Selectin ,Antigens, CD ,Neutrophils ,CD18 Antigens ,Animals ,Antibodies, Monoclonal ,Bacterial Infections ,Platelet Membrane Glycoproteins ,Rabbits ,Peritonitis ,Staphylococcal Infections ,Abscess ,Escherichia coli Infections - Abstract
Adhesion molecules are responsible for PMN-endothelial cell interactions involved in both PMN-mediated endothelial injury (e.g., after ischemia-reperfusion injury) and PMN-mediated host defense against bacterial infection. Inhibition of PMN-endothelial adherence with CD18 and P-selectin mAb has been shown to ameliorate the tissue injury resulting from ischemia and reperfusion under a variety of experimental conditions. However, interference with PMN function may result in an increased risk of bacterial infection. Previous investigations suggest that CD18 blockade can lead to increased infectious risk. Little is known of the infectious risks associated with selectin blockade. We report the effects of P-selectin blockade (using mAb PB1.3) on bacteria-induced PMN emigration into the peritoneum and subcutaneous (s.c.) tissue in rabbits. Leukocyte and PMN emigration into the peritoneum 4 h after inoculation with 10 ml of 10(9) CFU/ml Escherichia coli was significant in saline-treated animals, and not different in animals pretreated with mAb PB1.3. Similarly, the incidence and severity of abscess formation 7 days after s.c. inoculation with Staphylococcus aureus (10(7), 10(8), or 10(9) CFU) was not increased in rabbits pretreated with mAb PB1.3 compared to saline. PMN emigration to the s.c. S. aureus was also similar in both saline and mAb PB1.3-treated animals, as determined by light microscopy. We conclude that P-selectin blockade with mAb PB1.3: 1) does not interfere with acute, E. coli-induced PMN emigration into the peritoneum, 2) does not increase the incidence or severity of S. aureus abscess formation in s.c. tissue, and 3) interferes less with PMN antibacterial host defense mechanisms than inhibition of CD18-mediated PMN adherence.
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- 1993
16. A Potential Galaxy Threshing System in the Cosmos Field
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Anton M. Koekemoer, Martin Elvis, Y. Shioya, M. Rich, Hiroshi Karoji, Bahram Mobasher, Masaru Ajiki, M. Giavalisco, S. J. Lilly, Kartik Sheth, Chris Impey, Alvio Renzini, Tohru Nagao, S. S. Sasaki, Kouji Ohta, L. Hainline, Yutaka Komiyama, Nobuo Arimoto, D. B. Sanders, Satoshi Miyazaki, H. Aussel, Jin Koda, Y. Taniguchi, N. Kaifu, Eva Schinnerer, Sadanori Okamura, Nick Scoville, O. LeFevre, and T. Murayama
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Physics ,010308 nuclear & particles physics ,media_common.quotation_subject ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Galaxy ,Redshift ,Luminosity ,Space and Planetary Science ,Sky ,0103 physical sciences ,Elliptical galaxy ,Satellite galaxy ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Subaru Telescope ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Photometric redshift ,media_common - Abstract
We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system consists of a giant elliptical galaxy with $M_V \approx -21.6$ and a tidally disrupted satellite galaxy with $M_V \approx -17.7$ at a photometric redshift of $z \approx 0.08$. This redshift is consistent with the spectroscopic redshift of 0.079 for the giant elliptical galaxy obtained from the Sloan Digital Sky Survey (SDSS) archive. The luminosity masses of the two galaxies are $3.7 \times 10^{12} \cal{M}_{\odot}$ and $3.1 \times 10^{9} \cal{M}_{\odot}$, respectively. The distance between the two galaxies is greater than 100 kpc. The two tidal tails emanating from the satellite galaxy extend over 150 kpc. This system would be the second well-defined galaxy threshing system found so far., 17 pages, 7 figures, accepted for the COSMOS special issue of ApJS
17. COMPARATIVE HEMODYNAMIC AND OXYGEN TRANSPORT STUDIES DURING INDUCED HYPOTENSION WITH ATP, ADENOSINE, NITROPRUSSIDE, AND HALOTHANE
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A. F. Fukunaga, K. Murata, S. S. Sasaki, and P. J. Morgan
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Anesthesiology and Pain Medicine ,business.industry ,Anesthesia ,Oxygen transport ,medicine ,Hemodynamics ,Halothane ,business ,Adenosine ,Induced Hypotension ,medicine.drug - Published
- 1988
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18. [Avascular necrosis of the femoral head after COVID-19: clinical presentation and management. Clinical-functional outcomes of decompression and supplementation with bone marrow cell aspirate].
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Godoy-Monzón D, Cid-Casteulani A, Svarzchtein S, Sasaki S, and Pascual-Espinosa JM
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- Humans, Male, Female, Middle Aged, Prospective Studies, Adult, Treatment Outcome, Bone Marrow Transplantation methods, Adrenal Cortex Hormones therapeutic use, Adrenal Cortex Hormones administration & dosage, Magnetic Resonance Imaging, Follow-Up Studies, Femur Head Necrosis surgery, Femur Head Necrosis etiology, COVID-19 complications, Decompression, Surgical methods
- Abstract
Introduction: the pandemic of COVID-19 has led to clinical complications such as avascular necrosis of the femoral head (AVNFH) associated with the use of corticosteroids. The aim of the study is to report the functional and radiographic results of 13 patients with post-COVID-19 ANFH after decompression using Forage and bone marrow aspirate concentrate (BMAC)., Material and Methods: single-center, prospective, uncontrolled clinical study. From April 2020 to September 2021, 13 patients (21 hips) with post-COVID-19 ANFH were treated. All received corticosteroids during infection (average daily dose: 480 mg). Clinical, radiographic and magnetic resonance imaging evaluations were performed; the Ficat classification was applied for the classification of AVNFH. The surgical technique used was decompression with Forage and ACMO., Results: the mean age was 47 years, with a follow-up of 30.4 months. Symptoms appeared with a mean of 4.2 months after COVID-19 infection. Harris score improved from 41.2 ± 5.2 to 86.6 ± 3.4. Radiographic evaluation showed that 14.3% of the sample experienced femoral head collapse and underwent total hip arthroplasty., Conclusions: post-COVID-19 ANFH is a clinical entity with rapid progression and different degrees of severity. Decompression with Forage and ACMO seems a promising initial treatment, however, the variable response and the probability of collapse emphasize the importance of long-term follow-up and identification of patients who may require additional interventions.
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- 2024
19. Evaluation of QSAR models for predicting mutagenicity: outcome of the Second Ames/QSAR international challenge project.
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Furuhama A, Kitazawa A, Yao J, Matos Dos Santos CE, Rathman J, Yang C, Ribeiro JV, Cross K, Myatt G, Raitano G, Benfenati E, Jeliazkova N, Saiakhov R, Chakravarti S, Foster RS, Bossa C, Battistelli CL, Benigni R, Sawada T, Wasada H, Hashimoto T, Wu M, Barzilay R, Daga PR, Clark RD, Mestres J, Montero A, Gregori-Puigjané E, Petkov P, Ivanova H, Mekenyan O, Matthews S, Guan D, Spicer J, Lui R, Uesawa Y, Kurosaki K, Matsuzaka Y, Sasaki S, Cronin MTD, Belfield SJ, Firman JW, Spînu N, Qiu M, Keca JM, Gini G, Li T, Tong W, Hong H, Liu Z, Igarashi Y, Yamada H, Sugiyama KI, and Honma M
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- Mutagenicity Tests, Mutagenesis, Japan, Mutagens toxicity, Mutagens chemistry, Quantitative Structure-Activity Relationship
- Abstract
Quantitative structure-activity relationship (QSAR) models are powerful in silico tools for predicting the mutagenicity of unstable compounds, impurities and metabolites that are difficult to examine using the Ames test. Ideally, Ames/QSAR models for regulatory use should demonstrate high sensitivity, low false-negative rate and wide coverage of chemical space. To promote superior model development, the Division of Genetics and Mutagenesis, National Institute of Health Sciences, Japan (DGM/NIHS), conducted the Second Ames/QSAR International Challenge Project (2020-2022) as a successor to the First Project (2014-2017), with 21 teams from 11 countries participating. The DGM/NIHS provided a curated training dataset of approximately 12,000 chemicals and a trial dataset of approximately 1,600 chemicals, and each participating team predicted the Ames mutagenicity of each trial chemical using various Ames/QSAR models. The DGM/NIHS then provided the Ames test results for trial chemicals to assist in model improvement. Although overall model performance on the Second Project was not superior to that on the First, models from the eight teams participating in both projects achieved higher sensitivity than models from teams participating in only the Second Project. Thus, these evaluations have facilitated the development of QSAR models.
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- 2023
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20. A potent allele marker related to low bull conception rate in Japanese Black bulls.
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Kinukawa M, Ito M, Uemoto Y, Ogino A, Haruta S, Kurogi K, Watanabe T, Sasaki S, Naniwa Y, Uchiyama K, and Togashi K
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- Cattle genetics, Animals, Male, Alleles, Genotype, Fertility genetics, Polymorphism, Single Nucleotide, Genome-Wide Association Study veterinary, Fertilization genetics
- Abstract
Over the years, there has been considerable variation in the bull conception rate (BCR) of Japanese Black cattle; moreover, several Japanese Black bulls with a low BCR of ≤10% have been identified. However, the alleles responsible for the low BCR are not determined yet. Therefore, in this study, we aimed to identify single-nucleotide polymorphisms (SNPs) for predicting low BCR. To this end, the genome of Japanese Black bulls was comprehensively examined by a genome-wide association study with whole-exome sequencing (WES), and the effect of the identified marker regions on BCR was determined. The WES analysis of six sub-fertile bulls with a BCR of ≤10% and 73 normal bulls with a BCR of ≥40% identified a homozygous genotype for low BCR in Bos taurus autosome 5 in the region between 116.2 and 117.9 Mb. The g.116408653G > A SNP in this region had the most significant effect on the BCR (P-value = 1.0 × 10
-23 ), and the GG (55.4 ± 11.2%) and AG (54.4 ± 9.4%) genotypes in the SNP had a higher phenotype than the AA (9.5 ± 6.1%) genotype for the BCR. The mixed model analysis revealed that g.116408653G > A was related to approximately 43% of the total genetic variance. In conclusion, the AA genotype of g.116408653G > A is a useful index for identifying sub-fertile Japanese Black bulls. Some positive and negative effects of SNP on the BCR were presumed to identify the causative mutations, which can help evaluate bull fertility., (Copyright © 2023 The Author(s). Published by Elsevier B.V. All rights reserved.)- Published
- 2023
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21. Post-Disaster Mental Health and Dietary Patterns among Older Survivors of an Earthquake and Tsunami.
- Author
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Yazawa A, Shiba K, Hikichi H, Okuzono SS, Aida J, Kondo K, Sasaki S, and Kawachi I
- Subjects
- Male, Humans, Female, Tsunamis, Mental Health, Prospective Studies, Survivors psychology, Japan, Earthquakes, Disasters
- Abstract
Objectives: Research suggests that cardiometabolic disease risks are elevated among survivors of natural disasters, possibly mediated by changes in diet. Using the Brief Dietary History Questionnaire, we examined (1) dietary patterns among older survivors of the 2011 Great East Japan Earthquake and Tsunami, and (2) the contribution of posttraumatic stress symptoms (PTSS)/depressive symptoms, as well as relocation to temporary housing on dietary patterns and (3) gender differences in the associations., Design, Setting and Participants: Data came from a prospective cohort study of 1,375 survivors aged 65-89 years (44.6% male)., Measurements: PTSS/depression onset was evaluated in 2013, 2.5 years after the disaster. Dietary data was collected with a self-administered brief-type diet history questionnaire in 2020. A principal component analysis identified three posterior dietary patterns., Results: Diet 1 consisted of high intake of vegetables, soy products, and fruits; Diet 2 consisted of carbohydrate-rich foods and snacks/sweets; Diet 3 consisted of high intake of alcoholic beverages, meat, and seafood. Least-squares linear regression revealed that individuals with PTSS/depression were less likely to exhibit Diet 1, while individuals with PTSS were more likely to exhibit Diet 2 and 3. Especially, males who had depression showed an unhealthy dietary pattern. Those who have lived in a trailer-style temporary housing reported less consumption of Diet 3., Conclusion: Survivors of disaster with symptoms of mental illness tended to exhibit less healthy dietary patterns after 9 years. Diet varied by type of post-disaster mental illness, gender, and current social circumstances. We lacked pre-disaster BDHQ data, which is a limitation., Competing Interests: None.
- Published
- 2023
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22. The prognostic value of 18 F-FDG PET/CT taken immediately after completion of radiotherapy for lung cancer treated with concurrent chemoradiotherapy: A pilot study.
- Author
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Harigai A, Saito AI, Inoue T, Suzuki M, Namba Y, Suzuki Y, Makino F, Nagashima O, Sasaki S, and Sasai K
- Subjects
- Chemoradiotherapy, Humans, Pilot Projects, Positron Emission Tomography Computed Tomography methods, Prognosis, Radiopharmaceuticals, Fluorodeoxyglucose F18, Lung Neoplasms radiotherapy, Lung Neoplasms therapy
- Abstract
Purpose: The prognostic value of F-18 fluorodeoxyglucose positron emission tomography/computed tomography (PET/CT) taken immediately after completion of radiotherapy in lung cancer patients is not well known. The purpose of this study is to assess the prognostic value of PET/CT taken immediately after completion of radiotherapy in lung cancer patients., Materials and Methods: Patients with primary lung cancer planned to undergo concurrent chemoradiotherapy were enrolled. Patients underwent PET/CT scans at 3 time points: before radiotherapy, within 24hours of completing radiotherapy (im-PET/CT), and 2-9 months after radiotherapy (post-PET/CT). Maximum standardized uptake value (SUV
max ) was obtained. A post-PET/CT-SUVmax cut-off of 2.5 was determined as radiotherapy success., Results: Nineteen patients were enrolled. im-PET/CT-SUVmax for patients in the high post-PET/CT-SUVmax group was significantly higher than that of the low group (P=0.004). Receiver operator curve analysis indicated that im-PET/CT-SUVmax of 4.35 was an optimal cut-off value to discriminate between the two groups. Multivariable analysis showed that a high im-PET/CT-SUVmax was significantly associated with a high post-PET/CT-SUVmax (P=0.003)., Conclusion: PET/CT-SUVmax taken immediately following radiotherapy was associated with that evaluated 2-9 months after radiotherapy., (Copyright © 2022 Société française de radiothérapie oncologique (SFRO). Published by Elsevier Masson SAS. All rights reserved.)- Published
- 2022
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23. Minocycline and black thyroid.
- Author
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Goto Y, Ohba K, Sasaki S, and Nishino N
- Subjects
- Anti-Bacterial Agents adverse effects, Humans, Minocycline adverse effects, Thyroid Gland diagnostic imaging
- Published
- 2022
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24. Gastrointestinal: Extramammary Paget disease of the esophagus.
- Author
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Yada S, Sasaki S, Tokuno K, Yamashita Y, and Sakaida I
- Subjects
- Humans, Esophageal Neoplasms, Paget Disease, Extramammary
- Published
- 2022
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25. Andreev reflection of fractional quantum Hall quasiparticles.
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Hashisaka M, Jonckheere T, Akiho T, Sasaki S, Rech J, Martin T, and Muraki K
- Abstract
Electron correlation in a quantum many-body state appears as peculiar scattering behaviour at its boundary, symbolic of which is Andreev reflection at a metal-superconductor interface. Despite being fundamental in nature, dictated by the charge conservation law, however, the process has had no analogues outside the realm of superconductivity so far. Here, we report the observation of an Andreev-like process originating from a topological quantum many-body effect instead of superconductivity. A narrow junction between fractional and integer quantum Hall states shows a two-terminal conductance exceeding that of the constituent fractional state. This remarkable behaviour, while theoretically predicted more than two decades ago but not detected to date, can be interpreted as Andreev reflection of fractionally charged quasiparticles. The observed fractional quantum Hall Andreev reflection provides a fundamental picture that captures microscopic charge dynamics at the boundaries of topological quantum many-body states.
- Published
- 2021
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26. A genome-wide association study reveals a quantitative trait locus for calf mortality on chromosome 9 in Japanese Black cattle.
- Author
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Sasaki S and Ibi T
- Subjects
- Alleles, Animals, Breeding, Genetic Association Studies veterinary, Japan, Molecular Chaperones genetics, Polymorphism, Single Nucleotide, Cattle genetics, Death, Quantitative Trait Loci
- Abstract
Calf mortality is a major problem affecting cattle production. To identify genetic variants associated with calf mortality in Japanese Black cattle, we evaluated calf mortality as a categorical trait using a threshold model and conducted a GWAS. We identified two SNPs between 32 549 297 and 32 606 924 bp on bovine chromosome 9 that were significantly associated with calf mortality from 61 to 180 days after birth. The SNP showing the highest association was localized at a region 624 bp downstream of exon 4 of the anti-silencing function 1A histone chaperone gene (ASF1A) that promotes DNA damage repair, and the null mice, which exhibit pre- and postnatal lethality. This association was also detected using the breeding value of 334 sires. The frequency of the risk allele in Japanese Black cattle from locations across Japan was 0.013; although the frequency of ASF1A risk allele was low, it is widespread in the Japanese Black cattle population. Thus, it may be necessary to routinely monitor the cattle population for the presence of this allele., (© 2021 Stichting International Foundation for Animal Genetics.)
- Published
- 2021
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27. S-1 and oxaliplatin versus tegafur-uracil and leucovorin as post-operative adjuvant chemotherapy in patients with high-risk stage III colon cancer: updated 5-year survival of the phase III ACTS-CC 02 trial.
- Author
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Watanabe J, Sasaki S, Kusumoto T, Sakamoto Y, Yoshida K, Tomita N, Maeda A, Teshima J, Yokota M, Tanaka C, Yamauchi J, Uetake H, Itabashi M, Takahashi K, Baba H, Kotake K, Boku N, Aiba K, Morita S, Takenaka N, and Sugihara K
- Subjects
- Antineoplastic Combined Chemotherapy Protocols therapeutic use, Chemotherapy, Adjuvant, Humans, Neoplasm Staging, Colonic Neoplasms drug therapy, Colonic Neoplasms pathology, Leucovorin therapeutic use, Oxaliplatin therapeutic use, Tegafur therapeutic use, Uracil therapeutic use
- Abstract
Background: The ACTS-CC 02 trial demonstrated that S-1 plus oxaliplatin (SOX) was not superior to tegafur-uracil and leucovorin (UFT/LV) in terms of disease-free survival (DFS) as adjuvant chemotherapy for high-risk stage III colon cancer (any T, N2, or positive nodes around the origin of the feeding arteries). We now report the final overall survival (OS) and subgroup analysis according to the pathological stage (TNM 7th edition) for treatment efficacy., Patients and Methods: Patients who underwent curative resection for pathologically confirmed high-risk stage III colon cancer were randomly assigned to receive either UFT/LV (300 mg/m
2 of UFT and 75 mg/day of LV on days 1-28, every 35 days, five cycles) or SOX (100 mg/m2 of oxaliplatin on day 1 and 80 mg/m2 /day of S-1 on days 1-14, every 21 days, eight cycles). The primary endpoint was DFS and the patients' data were updated in February 2020., Results: A total of 478 patients in the UFT/LV group and 477 patients in the SOX group were included in the final analysis. With a median follow-up time of 74.3 months, the 5-year DFS rate was 55.2% in the UFT/LV group and 58.1% in the SOX group [stratified hazard ratio (HR) 0.92; 95% confidence interval (CI) 0.76-1.11; P = 0.3973], and the 5-year OS rates were 78.3% and 79.1%, respectively (stratified HR 0.97; 95% CI 0.76-1.24; P = 0.8175). In the subgroup analysis, the 5-year OS rates in patients with T4N2b disease were 51.0% and 64.1% in the UFT/LV and SOX groups, respectively (HR 0.72; 95% CI 0.40-1.31)., Conclusion: Our final analysis reconfirmed that SOX as adjuvant chemotherapy is not superior to UFT/LV in terms of DFS in patients with high-risk stage III colon cancer. The 5-year OS rate was similar in the UFT/LV and SOX groups., Competing Interests: Disclosure JW reports personal fees from Johnson and Johnson and Medtronic Co., Ltd., outside the submitted work. KY reports personal fees and research grants from Asahi Kasei, Chugai Pharmaceutical Co., Ltd., Covidien, Daiichi Sankyo, Eli Lilly Japan K.K., Johnson & Johnson, Merc Serono, MSD K.K., Nippon Kayaku, Novartis, Ono Pharmaceutical Co., Ltd., Sanofi, Taiho Pharmaceutical Co., Ltd., Takeda, Tsumura, Yakult Honsha Co., Ltd., Eisai, and Otsuka outside the submitted work. NTo reports personal fees from Taiho Pharmaceutical Co., Ltd., and Chugai Pharmaceutical Co., Ltd., and research grants from Taiho Pharmaceutical Co., Ltd., Chugai Pharmaceutical Co., Ltd., Eli Lilly Japan K.K., and Sysmex outside the submitted work. HU reports personal fees from Taiho Pharmaceutical Co., Ltd., Chugai Pharmaceutical Co., Ltd., Takeda, Daiichi Sankyo, and Bayer. MI reports research grants from Taiho Pharmaceutical Co., Ltd., Pfizer, Astellas Pharma, Chugai Pharmaceutical Co., Ltd., and Takeda outside the submitted work. KT reports personal fees from Taiho Pharmaceutical Co., Ltd., Chugai Pharmaceutical Co., Ltd., and Eli Lilly Japan K.K. outside the submitted work. HB reports personal fees from Taiho Pharmaceutical Co., Ltd., and research grants from Taiho Pharmaceutical Co., Ltd., Chugai Pharmaceutical Co., Ltd., Ono Pharmaceutical Co., Ltd., MSD K.K., and Shin Nippon Biomedical outside the submitted work. NB reports personal fees from Taiho Pharmaceutical Co., Ltd., Ono Pharmaceutical Co., Ltd., Bristol-Myers Squibb, and research grants from Taiho Pharmaceutical Co., Ltd., Ono Pharmaceutical Co., Ltd., Bristol-Myers Squibb, and Takeda outside the submitted work. SM reports personal fees from Taiho Pharmaceutical Co., Ltd., Chugai Pharmaceutical Co., Ltd., Bristol-Myers Squibb, Yakult Honsha Co., Ltd., Eli Lilly Japan K.K., and Ono Pharmaceutical Co., Ltd. outside the submitted work. NTa reports personal fees from Taiho Pharmaceutical Co., Ltd. during the conduct of the study and outside the submitted work, and is an employee of Taiho Pharmaceutical Co., Ltd., the manufacturer of UFT/LV and S-1. KS reports personal fees and research grants from Taiho Pharmaceutical Co., Ltd. and Chugai Pharmaceutical Co., Ltd. outside the submitted work. All other authors have declared no conflicts of interest., (Copyright © 2021 The Author(s). Published by Elsevier Ltd.. All rights reserved.)- Published
- 2021
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28. A highly multiplexed melt-curve assay for detecting the most prevalent carbapenemase, ESBL, and AmpC genes.
- Author
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Edwards T, Williams C, Teethaisong Y, Sealey J, Sasaki S, Hobbs G, Cuevas LE, Evans K, and Adams ER
- Subjects
- Anti-Bacterial Agents pharmacology, Carbapenems pharmacology, Cephalosporins pharmacology, Gram-Negative Bacteria classification, Gram-Negative Bacteria genetics, Gram-Negative Bacteria isolation & purification, Gram-Negative Bacterial Infections diagnosis, Humans, Sensitivity and Specificity, Bacterial Proteins genetics, Drug Resistance, Bacterial genetics, Molecular Diagnostic Techniques methods, Multiplex Polymerase Chain Reaction methods, beta-Lactamases genetics
- Abstract
Resistance to third-generation cephalosporins and carbapenems in Gram-negative bacteria is chiefly mediated by beta-lactamases including extended-spectrum beta-lactamase (ESBL), AmpC, and carbapenemase enzymes. Routine phenotypic detection methods do not provide timely results, and there is a lack of comprehensive molecular panels covering all important markers. An ESBL/carbapenemase high-resolution melt analysis (HRM) assay (SHV, TEM, CTX-M ESBL families, and NDM, IMP, KPC, VIM and OXA-48-like carbapenemases) and an AmpC HRM assay (16S rDNA control, FOX, MOX, ACC, EBC, CIT, and DHA) were designed and evaluated on 111 Gram-negative isolates with mixed resistance patterns. The sensitivity for carbapenemase, ESBL, and AmpC genes was 96.7% (95% confidence interval [CI]: 82.8-99.9%), 93.6% (95% CI: 85.7-97.9%), and 93.8% (95% CI: 82.8-98.7%), respectively, with a specificity of 100% (95% CI: 95.6-100%), 93.9% (95% CI: 79.8-99.3%), and 93.7% (95% CI: 84.5-98.2%). The HRM assays enable the simultaneous detection of the 14 most important ESBL, carbapenemase, and AmpC genes and could be used as a molecular surveillance tool or to hasten detection of antimicrobial resistance for treatment management., (Copyright © 2020 The Author(s). Published by Elsevier Inc. All rights reserved.)
- Published
- 2020
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29. A high-power, high-repetition-rate THz source for pump-probe experiments at Linac Coherent Light Source II.
- Author
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Zhang Z, Fisher AS, Hoffmann MC, Jacobson B, Kirchmann PS, Lee WS, Lindenberg A, Marinelli A, Nanni E, Schoenlein R, Qian M, Sasaki S, Xu J, and Huang Z
- Abstract
Experiments using a THz pump and an X-ray probe at an X-ray free-electron laser (XFEL) facility like the Linac Coherent Light Source II (LCLS II) require frequency-tunable (3 to 20 THz), narrow bandwidth (∼10%), carrier-envelope-phase-stable THz pulses that produce high fields (>1 MV cm
-1 ) at the repetition rate of the X-rays and are well synchronized with them. In this paper, a two-bunch scheme to generate THz radiation at LCLS II is studied: the first bunch produces THz radiation in an electromagnet wiggler immediately following the LCLS II undulator that produces X-rays from the second bunch. The initial time delay between the two bunches is optimized to compensate for the path difference in THz transport. The two-bunch beam dynamics, the THz wiggler and radiation are described, as well as the transport system bringing the THz pulses from the wiggler to the experimental hall., (open access.)- Published
- 2020
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30. Sample collection from asteroid (162173) Ryugu by Hayabusa2: Implications for surface evolution.
- Author
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Morota T, Sugita S, Cho Y, Kanamaru M, Tatsumi E, Sakatani N, Honda R, Hirata N, Kikuchi H, Yamada M, Yokota Y, Kameda S, Matsuoka M, Sawada H, Honda C, Kouyama T, Ogawa K, Suzuki H, Yoshioka K, Hayakawa M, Hirata N, Hirabayashi M, Miyamoto H, Michikami T, Hiroi T, Hemmi R, Barnouin OS, Ernst CM, Kitazato K, Nakamura T, Riu L, Senshu H, Kobayashi H, Sasaki S, Komatsu G, Tanabe N, Fujii Y, Irie T, Suemitsu M, Takaki N, Sugimoto C, Yumoto K, Ishida M, Kato H, Moroi K, Domingue D, Michel P, Pilorget C, Iwata T, Abe M, Ohtake M, Nakauchi Y, Tsumura K, Yabuta H, Ishihara Y, Noguchi R, Matsumoto K, Miura A, Namiki N, Tachibana S, Arakawa M, Ikeda H, Wada K, Mizuno T, Hirose C, Hosoda S, Mori O, Shimada T, Soldini S, Tsukizaki R, Yano H, Ozaki M, Takeuchi H, Yamamoto Y, Okada T, Shimaki Y, Shirai K, Iijima Y, Noda H, Kikuchi S, Yamaguchi T, Ogawa N, Ono G, Mimasu Y, Yoshikawa K, Takahashi T, Takei Y, Fujii A, Nakazawa S, Terui F, Tanaka S, Yoshikawa M, Saiki T, Watanabe S, and Tsuda Y
- Abstract
The near-Earth asteroid (162173) Ryugu is thought to be a primitive carbonaceous object that contains hydrated minerals and organic molecules. We report sample collection from Ryugu's surface by the Hayabusa2 spacecraft on 21 February 2019. Touchdown images and global observations of surface colors are used to investigate the stratigraphy of the surface around the sample location and across Ryugu. Latitudinal color variations suggest the reddening of exposed surface material by solar heating and/or space weathering. Immediately after touchdown, Hayabusa2's thrusters disturbed dark, fine grains that originate from the redder materials. The stratigraphic relationship between identified craters and the redder material indicates that surface reddening occurred over a short period of time. We suggest that Ryugu previously experienced an orbital excursion near the Sun., (Copyright © 2020 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.)
- Published
- 2020
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31. The geomorphology, color, and thermal properties of Ryugu: Implications for parent-body processes.
- Author
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Sugita S, Honda R, Morota T, Kameda S, Sawada H, Tatsumi E, Yamada M, Honda C, Yokota Y, Kouyama T, Sakatani N, Ogawa K, Suzuki H, Okada T, Namiki N, Tanaka S, Iijima Y, Yoshioka K, Hayakawa M, Cho Y, Matsuoka M, Hirata N, Hirata N, Miyamoto H, Domingue D, Hirabayashi M, Nakamura T, Hiroi T, Michikami T, Michel P, Ballouz RL, Barnouin OS, Ernst CM, Schröder SE, Kikuchi H, Hemmi R, Komatsu G, Fukuhara T, Taguchi M, Arai T, Senshu H, Demura H, Ogawa Y, Shimaki Y, Sekiguchi T, Müller TG, Hagermann A, Mizuno T, Noda H, Matsumoto K, Yamada R, Ishihara Y, Ikeda H, Araki H, Yamamoto K, Abe S, Yoshida F, Higuchi A, Sasaki S, Oshigami S, Tsuruta S, Asari K, Tazawa S, Shizugami M, Kimura J, Otsubo T, Yabuta H, Hasegawa S, Ishiguro M, Tachibana S, Palmer E, Gaskell R, Le Corre L, Jaumann R, Otto K, Schmitz N, Abell PA, Barucci MA, Zolensky ME, Vilas F, Thuillet F, Sugimoto C, Takaki N, Suzuki Y, Kamiyoshihara H, Okada M, Nagata K, Fujimoto M, Yoshikawa M, Yamamoto Y, Shirai K, Noguchi R, Ogawa N, Terui F, Kikuchi S, Yamaguchi T, Oki Y, Takao Y, Takeuchi H, Ono G, Mimasu Y, Yoshikawa K, Takahashi T, Takei Y, Fujii A, Hirose C, Nakazawa S, Hosoda S, Mori O, Shimada T, Soldini S, Iwata T, Abe M, Yano H, Tsukizaki R, Ozaki M, Nishiyama K, Saiki T, Watanabe S, and Tsuda Y
- Abstract
The near-Earth carbonaceous asteroid 162173 Ryugu is thought to have been produced from a parent body that contained water ice and organic molecules. The Hayabusa2 spacecraft has obtained global multicolor images of Ryugu. Geomorphological features present include a circum-equatorial ridge, east-west dichotomy, high boulder abundances across the entire surface, and impact craters. Age estimates from the craters indicate a resurfacing age of [Formula: see text] years for the top 1-meter layer. Ryugu is among the darkest known bodies in the Solar System. The high abundance and spectral properties of boulders are consistent with moderately dehydrated materials, analogous to thermally metamorphosed meteorites found on Earth. The general uniformity in color across Ryugu's surface supports partial dehydration due to internal heating of the asteroid's parent body., (Copyright © 2019, American Association for the Advancement of Science.)
- Published
- 2019
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32. Search for CP Violation in Neutrino and Antineutrino Oscillations by the T2K Experiment with 2.2×10^{21} Protons on Target.
- Author
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Abe K, Akutsu R, Ali A, Amey J, Andreopoulos C, Anthony L, Antonova M, Aoki S, Ariga A, Ashida Y, Azuma Y, Ban S, Barbi M, Barker GJ, Barr G, Barry C, Batkiewicz M, Bench F, Berardi V, Berkman S, Berner RM, Berns L, Bhadra S, Bienstock S, Blondel A, Bolognesi S, Bourguille B, Boyd SB, Brailsford D, Bravar A, Bronner C, Buizza Avanzini M, Calcutt J, Campbell T, Cao S, Cartwright SL, Catanesi MG, Cervera A, Chappell A, Checchia C, Cherdack D, Chikuma N, Christodoulou G, Coleman J, Collazuol G, Coplowe D, Cudd A, Dabrowska A, De Rosa G, Dealtry T, Denner PF, Dennis SR, Densham C, Di Lodovico F, Dokania N, Dolan S, Drapier O, Duffy KE, Dumarchez J, Dunne P, Emery-Schrenk S, Ereditato A, Fernandez P, Feusels T, Finch AJ, Fiorentini GA, Fiorillo G, Francois C, Friend M, Fujii Y, Fujita R, Fukuda D, Fukuda Y, Gameil K, Giganti C, Gizzarelli F, Golan T, Gonin M, Hadley DR, Haegel L, Haigh JT, Hamacher-Baumann P, Hansen D, Harada J, Hartz M, Hasegawa T, Hastings NC, Hayashino T, Hayato Y, Hiramoto A, Hogan M, Holeczek J, Hosomi F, Ichikawa AK, Ikeda M, Imber J, Inoue T, Intonti RA, Ishida T, Ishii T, Ishitsuka M, Iwamoto K, Izmaylov A, Jamieson B, Jiang M, Johnson S, Jonsson P, Jung CK, Kabirnezhad M, Kaboth AC, Kajita T, Kakuno H, Kameda J, Karlen D, Katori T, Kato Y, Kearns E, Khabibullin M, Khotjantsev A, Kim H, Kim J, King S, Kisiel J, Knight A, Knox A, Kobayashi T, Koch L, Koga T, Koller PP, Konaka A, Kormos LL, Koshio Y, Kowalik K, Kubo H, Kudenko Y, Kurjata R, Kutter T, Kuze M, Labarga L, Lagoda J, Lamoureux M, Lasorak P, Laveder M, Lawe M, Licciardi M, Lindner T, Liptak ZJ, Litchfield RP, Li X, Longhin A, Lopez JP, Lou T, Ludovici L, Lu X, Magaletti L, Mahn K, Malek M, Manly S, Maret L, Marino AD, Martin JF, Martins P, Maruyama T, Matsubara T, Matveev V, Mavrokoridis K, Ma WY, Mazzucato E, McCarthy M, McCauley N, McFarland KS, McGrew C, Mefodiev A, Metelko C, Mezzetto M, Minamino A, Mineev O, Mine S, Missert A, Miura M, Moriyama S, Morrison J, Mueller TA, Murphy S, Nagai Y, Nakadaira T, Nakahata M, Nakajima Y, Nakamura KG, Nakamura K, Nakamura KD, Nakanishi Y, Nakayama S, Nakaya T, Nakayoshi K, Nantais C, Nielsen C, Niewczas K, Nishikawa K, Nishimura Y, Nonnenmacher TS, Novella P, Nowak J, O'Keeffe HM, O'Sullivan L, Okumura K, Okusawa T, Oryszczak W, Oser SM, Owen RA, Oyama Y, Palladino V, Palomino JL, Paolone V, Paudyal P, Pavin M, Payne D, Pickering L, Pidcott C, Pinzon Guerra ES, Pistillo C, Popov B, Porwit K, Posiadala-Zezula M, Pritchard A, Quilain B, Radermacher T, Radicioni E, Ratoff PN, Reinherz-Aronis E, Riccio C, Rondio E, Rossi B, Roth S, Rubbia A, Ruggeri AC, Rychter A, Sakashita K, Sánchez F, Sasaki S, Scantamburlo E, Scholberg K, Schwehr J, Scott M, Seiya Y, Sekiguchi T, Sekiya H, Sgalaberna D, Shah R, Shaikhiev A, Shaker F, Shaw D, Shiozawa M, Smirnov A, Smy M, Sobczyk JT, Sobel H, Sonoda Y, Steinmann J, Stewart T, Stowell P, Suda Y, Suvorov S, Suzuki A, Suzuki SY, Suzuki Y, Sztuc AA, Tacik R, Tada M, Takeda A, Takeuchi Y, Tamura R, Tanaka HK, Tanaka HA, Thakore T, Thompson LF, Toki W, Touramanis C, Tsui KM, Tsukamoto T, Tzanov M, Uchida Y, Uno W, Vagins M, Vallari Z, Vasseur G, Vilela C, Vladisavljevic T, Volkov VV, Wachala T, Walker J, Wang Y, Wark D, Wascko MO, Weber A, Wendell R, Wilking MJ, Wilkinson C, Wilson JR, Wilson RJ, Wret C, Yamada Y, Yamamoto K, Yamasu S, Yanagisawa C, Yang G, Yano T, Yasutome K, Yen S, Yershov N, Yokoyama M, Yoshida T, Yu M, Zalewska A, Zalipska J, Zaremba K, Zarnecki G, Ziembicki M, Zimmerman ED, Zito M, Zsoldos S, and Zykova A
- Abstract
The T2K experiment measures muon neutrino disappearance and electron neutrino appearance in accelerator-produced neutrino and antineutrino beams. With an exposure of 14.7(7.6)×10^{20} protons on target in the neutrino (antineutrino) mode, 89 ν_{e} candidates and seven anti-ν_{e} candidates are observed, while 67.5 and 9.0 are expected for δ_{CP}=0 and normal mass ordering. The obtained 2σ confidence interval for the CP-violating phase, δ_{CP}, does not include the CP-conserving cases (δ_{CP}=0, π). The best-fit values of other parameters are sin^{2}θ_{23}=0.526_{-0.036}^{+0.032} and Δm_{32}^{2}=2.463_{-0.070}^{+0.071}×10^{-3} eV^{2}/c^{4}.
- Published
- 2018
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33. Endovascular Treatment for Very Early Hepatic Artery Stenosis Following Living-Donor Liver Transplantation: Report of Two Cases.
- Author
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Goto Y, Shirahama N, Sasaki S, Kawahara R, Sakai H, Ishikawa H, Hisaka T, Ogata T, Yasunaga M, Akagi Y, Tanaka H, and Okuda K
- Subjects
- Aged, Constriction, Pathologic surgery, Female, Humans, Liver Transplantation methods, Living Donors, Middle Aged, Retrospective Studies, Treatment Outcome, Endovascular Procedures methods, Hepatic Artery pathology, Hepatic Artery surgery, Liver Transplantation adverse effects, Postoperative Complications surgery
- Abstract
Background: Some literature has reported on endovascular treatment for very early hepatic artery stenosis (HAS; within 2 weeks after liver transplantation, and has deemed endovascular treatment to be a contraindication because out of serious complications associated with the procedure. We report on 2 cases of very early HAS successfully treated with endovascular treatment after living-donor liver transplantation (LDLT). CASE 1: A 54-year-old woman underwent LDLT with a left liver graft. The native right gastric artery and left hepatic artery (LHA) of the donor were anastomosed. On postoperative day (POD) 13, HAS was suspected and multidetector computerized tomographic angiography (MDCTA) was performed, which revealed 90% stenosis of the arterial anastomosis and 50% stenosis of the LHA in the graft. We performed percutaneous balloon arterioplasty (PBA) without any complications. The artery was patent with a postoperative follow-up of 60 months without the need for repeat intervention. CASE 2: A 67-year-old woman with a history of repeated transarterial chemoembolization for hepatocellular carcinoma underwent LDLT with a left liver graft. The native A4 and LHA of the donor were anastomosed. We performed MDCTA on POD 11, which revealed 70% stenosis of the native hepatic artery. We performed PBA followed by stent placement on POD 11 without complication. The artery was patent with a postoperative follow-up of 40 months without the need for repeated intervention., Conclusions: Endovascular treatment has the potential to avoid the need for repeated surgical interventions or retransplantation, and it can be safely performed in carefully selected patients., (Copyright © 2018 Elsevier Inc. All rights reserved.)
- Published
- 2018
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34. Evaluation of absolute measurement using a 4π plastic scintillator for the 4πβ-γ coincidence counting method.
- Author
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Unno Y, Sanami T, Sasaki S, Hagiwara M, and Yunoki A
- Abstract
Absolute measurement by the 4πβ-γ coincidence counting method was conducted by two photomultipliers facing across a plastic scintillator to be focused on β ray counting efficiency. The detector was held with a through-hole-type NaI(Tl) detector. The results include absolutely determined activity and its uncertainty especially about extrapolation. A comparison between the obtained and known activities showed agreement within their uncertainties., (Copyright © 2017 Elsevier Ltd. All rights reserved.)
- Published
- 2018
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35. Kinematic analysis of pressing situations in female collegiate football games: New insight into anterior cruciate ligament injury causation.
- Author
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Sasaki S, Koga H, Krosshaug T, Kaneko S, and Fukubayashi T
- Subjects
- Biomechanical Phenomena, Female, Hip Joint, Humans, Knee Joint, Rotation, Video Recording, Anterior Cruciate Ligament Injuries etiology, Athletic Injuries etiology, Range of Motion, Articular, Soccer injuries
- Abstract
The most common events during which anterior cruciate ligament (ACL) injuries occur in football are pressing situations. This study aimed to describe the knee and hip joint kinematics during pressing situations in football games to identify kinematic patterns in actions with a high risk for ACL injuries. We filmed 5 female collegiate football matches and identified 66 pressing situations. Five situations with a large distance between the trunk and foot placements in the sagittal plane were analyzed using a model-based image-matching technique. The mean knee flexion angle at initial contact (IC) was 13° (range, 8°-28°) and increased by 11° (95% confidence interval [CI], 3°-14°) at 40 ms after IC. As for knee adduction and rotation angles, the knee positions were close to neutral at IC, and only minor knee angular changes occurred later in the sequences. The mean hip flexion was 25° (range, 8°-43°) at IC and increased by 22° (95% CI, 11°-32°) after 100 ms. The hip was also externally rotated by 7° (range, -19° to 3°) at IC, and gradually rotated internally, reaching 10° of internal rotation (range, -5° to 27°) at 100 ms after IC. This study suggests that the observed knee valgus, internal hip and knee rotation, and static hip flexion previously reported in non-contact ACL injury events are unique to injury situations. In contrast, neither rapid knee valgus nor increased internal rotation was seen in non-injury pressing maneuvers., (© 2017 John Wiley & Sons A/S. Published by John Wiley & Sons Ltd.)
- Published
- 2018
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36. A genetic analysis of meat compositions in Japanese Black cattle: Genetic parameters and sex influence.
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Onogi A, Sasaki S, Kobayashi M, Ogino A, Nozaki T, Kurogi K, Yasumori T, Togashi K, and Iwata H
- Subjects
- Amino Acids analysis, Animals, Breeding, Fatty Acids analysis, Female, Food Quality, Male, Peptides analysis, Phenotype, Sex Factors, Sugars analysis, Cattle genetics, Genetic Association Studies veterinary, Meat analysis, Quantitative Trait, Heritable
- Abstract
Meat composition in beef is related to eating quality and food functionality. Genetic parameters for several meat compositions including free amino acid, peptide and sugar, however, remain poorly described. In this study, we estimated genetic parameters for 51 meat components, including free amino acids, peptides, sugars and fatty acid compositions, and two carcase traits in 1,354 heifers and 1,797 steers of Japanese Black cattle. Heritability estimates were generally equivalent to or moderately greater than those in previous studies of this breed. Genetic correlations between free amino acids, peptides and sugars and carcase traits were often negative, suggesting a trade-off between traits. Using two-trait animal models that treat records from the two sexes as different traits, we estimated sex-specific heritabilities and cross-sex genetic correlations which indicate the sex differences in genetic architecture. In these analyses, 12 traits showed significant heritability differences between sexes and cross-sex genetic correlations occasionally deviated from unity. These results could be used to inform future breeding schemes and investigations of the genetic architecture of meat compositions in beef., (© 2017 Blackwell Verlag GmbH.)
- Published
- 2017
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37. Crystallization and vitrification of electrons in a glass-forming charge liquid.
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Sasaki S, Hashimoto K, Kobayashi R, Itoh K, Iguchi S, Nishio Y, Ikemoto Y, Moriwaki T, Yoneyama N, Watanabe M, Ueda A, Mori H, Kobayashi K, Kumai R, Murakami Y, Müller J, and Sasaki T
- Abstract
Charge ordering (CO) is a phenomenon in which electrons in solids crystallize into a periodic pattern of charge-rich and charge-poor sites owing to strong electron correlations. This usually results in long-range order. In geometrically frustrated systems, however, a glassy electronic state without long-range CO has been observed. We found that a charge-ordered organic material with an isosceles triangular lattice shows charge dynamics associated with crystallization and vitrification of electrons, which can be understood in the context of an energy landscape arising from the degeneracy of various CO patterns. The dynamics suggest that the same nucleation and growth processes that characterize conventional glass-forming liquids guide the crystallization of electrons. These similarities may provide insight into our understanding of the liquid-glass transition., (Copyright © 2017 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.)
- Published
- 2017
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38. MSC/ECM Cellular Complexes Induce Periodontal Tissue Regeneration.
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Takewaki M, Kajiya M, Takeda K, Sasaki S, Motoike S, Komatsu N, Matsuda S, Ouhara K, Mizuno N, Fujita T, and Kurihara H
- Subjects
- Animals, Cell Differentiation, Cells, Cultured, Disease Models, Animal, Dogs, Ilium cytology, Mesenchymal Stem Cells cytology, X-Ray Microtomography, Cell- and Tissue-Based Therapy methods, Extracellular Matrix metabolism, Guided Tissue Regeneration, Periodontal methods, Mesenchymal Stem Cell Transplantation methods, Periodontal Diseases therapy, Tissue Engineering methods
- Abstract
Transplantation of mesenchymal stem cells (MSCs), which possess self-renewing properties and multipotency, into a periodontal defect is thought to be a useful option for periodontal tissue regeneration. However, developing more reliable and predictable implantation techniques is still needed. Recently, we generated clumps of an MSC/extracellular matrix (ECM) complex (C-MSC), which consisted of cells and self-produced ECM. C-MSCs can regulate their cellular functions in vitro and can be grafted into a defect site, without any artificial scaffold, to induce bone regeneration. Accordingly, this study aimed to evaluate the effect of C-MSC transplantation on periodontal tissue regeneration in beagle dogs. Seven beagle dogs were employed to generate a premolar class III furcation defect model. MSCs isolated from dog ilium were seeded at a density of 7.0 × 10
4 cells/well into 24-well plates and cultured in growth medium supplemented with 50 µg/mL ascorbic acid for 4 d. To obtain C-MSCs, confluent cells were scratched using a micropipette tip and were then torn off as a cellular sheet. The sheet was rolled up to make round clumps of cells. C-MSCs were maintained in growth medium or osteoinductive medium (OIM) for 5 or 10 d. The biological properties of C-MSCs were evaluated in vitro, and their periodontal tissue regenerative activity was tested by using a dog class III furcation defect model. Immunofluorescence analysis revealed that type I collagen fabricated the form of C-MSCs. OIM markedly elevated calcium deposition in C-MSCs at day 10, suggesting its osteogenic differentiation capacity. Both C-MSCs and C-MSCs cultured with OIM transplantation without an artificial scaffold into the dog furcation defect induced periodontal tissue regeneration successfully compared with no graft, whereas osteogenic-differentiated C-MSCs led to rapid alveolar bone regeneration. These findings suggested that the use of C-MSCs refined by self-produced ECM may represent a novel predictable periodontal tissue regenerative therapy.- Published
- 2017
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39. Helical Phase Structure of Radiation from an Electron in Circular Motion.
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Katoh M, Fujimoto M, Mirian NS, Konomi T, Taira Y, Kaneyasu T, Hosaka M, Yamamoto N, Mochihashi A, Takashima Y, Kuroda K, Miyamoto A, Miyamoto K, and Sasaki S
- Abstract
We theoretically show that a single free electron in circular motion radiates an electromagnetic wave possessing helical phase structure, which is closely related to orbital angular momentum carried by it. We experimentally demonstrate it by interference and double-slit diffraction experiments on radiation from relativistic electrons in spiral motion. Our results indicate that photons carrying orbital angular momentum should be created naturally by cyclotron/synchrotron radiations or Compton scatterings in various situations in cosmic space. We propose promising laboratory vortex photon sources in various wavelengths ranging from radio wave to gamma-rays.
- Published
- 2017
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40. Insular cortex and QT correction interval: an effect of hemispheric lateralization?
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Nagai M, Dote K, Kato M, Sasaki S, and Oda N
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- Electrocardiography, Heart Rate, Humans, Autonomic Nervous System, Cerebral Cortex
- Published
- 2017
- Full Text
- View/download PDF
41. Chromosomal anomalies and sperm retrieval outcomes of patients with non-obstructive azoospermia: a case series.
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Takeda T, Iwatsuki S, Hamakawa T, Mizuno K, Kamiya H, Umemoto Y, Kubota H, Kubota Y, Sasaki S, and Yasui T
- Subjects
- Abnormal Karyotype, Chromosome Aberrations, Humans, Karyotype, Male, Microdissection, Microsurgery, Retrospective Studies, Treatment Outcome, Azoospermia genetics, Azoospermia surgery, Sperm Retrieval
- Abstract
Some preoperative factors affecting the outcome of microdissection testicular sperm extraction (micro-TESE) have been previously evaluated. However, other than Klinefelter syndrome (KS), no other chromosomal anomalies have been discussed in the context of sperm retrieval outcomes. The objective of this study was to describe chromosomal anomalies and their relationship with sperm retrieval outcomes in patients with non-obstructive azoospermia (NOA). Of the 197 NOA patients whose clinical records were retrospectively reviewed, 144 (73.1%) had normal 46,XY karyotype, 40 (20.3%) had KS (47,XXY), and 13 (6.6%) had other chromosomal anomalies (autosomal in seven cases and sex-chromosomal anomalies in six). Of the seven patients with autosomal anomalies, two had the reportedly normal variant 46,XY,inv(9)(p12;q13). Testicular volume and serum hormone levels (luteinizing hormone, follicle-stimulating hormone, and total testosterone) of the patients with chromosomal anomalies other than KS were comparable to those of the patients with normal karyotype. The sperm retrieval rate of the patients with 46,XY karyotype, KS, or other chromosomal anomalies were 27.1%, 22.5%, and 15.4%, respectively, with no statistically significant difference. However, among the samples collected from the 13 patients with chromosomal anomalies other than KS, only those from the two patients with the normal variant 46,XY,inv(9)(p12;q13) contained spermatozoa. Among our series of NOA patients, the incidence of autosomal anomalies was higher than that generally noted among neonates, which suggests that not only sex-chromosomal anomalies but also autosomal anomalies may affect the development of NOA. Furthermore, our findings suggest that sperm retrieval outcome is more unfavorable in NOA patients with chromosomal anomalies than in NOA patients with 46,XY karyotype or KS, despite the use of micro-TESE., (© 2017 American Society of Andrology and European Academy of Andrology.)
- Published
- 2017
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42. Highly gate-tuneable Rashba spin-orbit interaction in a gate-all-around InAs nanowire metal-oxide-semiconductor field-effect transistor.
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Takase K, Ashikawa Y, Zhang G, Tateno K, and Sasaki S
- Abstract
III-V semiconductors have been intensively studied with the goal of realizing metal-oxide-semiconductor field-effect transistors (MOSFETs) with high mobility, a high on-off ratio, and low power consumption as next-generation transistors designed to replace current Si technology. Of these semiconductors, a narrow band-gap semiconductor InAs has strong Rashba spin-orbit interaction, thus making it advantageous in terms of both high field-effect transistor (FET) performance and efficient spin control. Here we report a high-performance InAs nanowire MOSFET with a gate-all-around (GAA) structure, where we simultaneously control the spin precession using the Rashba interaction. Our FET has a high on-off ratio (10
4 ~106 ) and a high field-effect mobility (1200 cm2 /Vs) and both values are comparable to those of previously reported nanowire FETs. Simultaneously, GAA geometry combined with high- κ dielectric enables the creation of a large and uniform coaxial electric field (>107 V/m), thereby achieving highly controllable Rashba coupling (1 × 10-11 eVm within a gate-voltage swing of 1 V), i.e. an operation voltage one order of magnitude smaller than those of back-gated nanowire MOSFETs. Our demonstration of high FET performance and spin controllability offers a new way of realizing low-power consumption nanoscale spin MOSFETs.- Published
- 2017
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43. Skipping breakfast and 5-year changes in body mass index and waist circumference in Japanese men and women.
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Sakurai M, Yoshita K, Nakamura K, Miura K, Takamura T, Nagasawa SY, Morikawa Y, Kido T, Naruse Y, Nogawa K, Suwazono Y, Sasaki S, Ishizaki M, and Nakagawa H
- Abstract
Objective: This study investigated the relationship between frequency of skipping breakfast and annual changes in body mass index (BMI) and waist circumference (WC)., Methods: The participants were 4,430 factory employees. BMI and WC were measured repeatedly at annual medical examinations over a 5-year period. The association between frequency of skipping breakfast at the baseline examination and annual changes in anthropometric indices was evaluated using the generalized estimating equation method., Results: The mean (standard deviation) BMI was 23.3 (3.0) kg m
-2 for men and 21.9 (3.6) kg m-2 for women; and the mean WC was 82.6 (8.7) cm for men and 77.8 (9.8) cm for women. During the follow-up period, mean BMI increased by 0.2 kg m-2 for men and women, and mean WC increased by 1.1 cm for men and 1.0 cm for women. The annual change in the BMI of men who skipped breakfast four to six times per week was 0.061 kg m-2 higher, and that of those who skipped breakfast seven times per week was 0.046 kg m-2 higher, compared with those who did not skip breakfast. Annual changes in the WC of male participants who skipped breakfast seven times per week was 0.248 cm higher than that of those who did not skip breakfast. Skipping breakfast was not associated with changes in BMI or WC in women., Conclusions: Skipping breakfast was closely associated with annual changes in BMI and WC among men, and eating breakfast more than four times per week may prevent the excessive body weight gain associated with skipping breakfast.- Published
- 2017
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44. Visit-to-visit blood pressure variability, average BP level and carotid arterial stiffness in the elderly: a prospective study.
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Nagai M, Dote K, Kato M, Sasaki S, Oda N, Kagawa E, Nakano Y, Yamane A, Kubo Y, Higashihara T, Miyauchi S, Harada W, and Masuda H
- Subjects
- Aged, Aged, 80 and over, Angiotensin Receptor Antagonists therapeutic use, Calcium Channel Blockers therapeutic use, Carotid Artery, Common diagnostic imaging, Carotid Intima-Media Thickness, Female, Humans, Hypertension drug therapy, Male, Prospective Studies, Angiotensin Receptor Antagonists pharmacology, Blood Pressure, Calcium Channel Blockers pharmacology, Carotid Artery, Common drug effects, Vascular Stiffness
- Abstract
In a cross-sectional study, visit-to-visit blood pressure (BP) variability was shown to be associated with artery remodelling. Here, we investigated the impact of visit-to-visit BP variability and average BP on the carotid artery remodelling progression in high-risk elderly according to different classes of antihypertension medication use/non-use. BP measurements and carotid ultrasound were performed in the common carotid artery in 164 subjects (mean age 79.7 years at baseline, 74.7% females) with one or more cardiovascular risk factors. Based on 12 visits (1 × /month for 1 year), we calculated visit-to-visit BP variability expressed as the standard deviation (s.d.), coefficient of variation (CV), maximum BP, minimum BP and delta (maximum-minimum) BP. We measured mean intima-media thickness (IMT) as well as stiffness parameter β were measured at baseline and at the mean 4.2-year follow-up. In a multiple regression analysis, the maximum, minimum, s.d. and average of systolic BP (SBP) were significantly associated with a change in β-values between the baseline and follow-up after adjustment for age, smoking, lower high-density lipoprotein level, baseline β-value and follow-up period. There were no significant associations between the visit-to-visit BP variability measures and the change in mean IMT. Significant associations of maximum, minimum, s.d. and average SBP were found with increased β-values in the subjects without calcium channel blocker (CCB) use and in the subjects using renin-angiotensin system inhibitors (RASIs). Thus, exaggerated visit-to-visit SBP variability and a high average SBP level were significant predictors of progression in carotid arterial stiffness in high-risk elderly without CCBs use and in those using a RASI.
- Published
- 2017
- Full Text
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45. Practical usefulness of atypical endometrial cell categories within the new classification of endometrial cytology when applied to conventional smears.
- Author
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Munakata S, Sasaki S, Takase M, Okatake R, Suzuki Y, Yamamoto T, and Yanoh K
- Subjects
- Biopsy, Endometrial Neoplasms diagnosis, Female, Humans, Uterine Cervical Neoplasms diagnosis, Vaginal Smears methods, Endometrial Hyperplasia diagnosis, Endometrial Hyperplasia pathology, Endometrial Neoplasms pathology, Endometrium pathology, Uterine Cervical Neoplasms pathology
- Abstract
Objective: Endometrial cytology has been widely used as a screening tool in Japan. Traditionally, a three-tier reporting system, consisting of 'negative', 'suspicious' and 'positive' categories, has been used. However, a more descriptive system, the New Terminology in Endometrial Cytology (NTEMC), which is based on the Bethesda System for uterine cervical cytology, was introduced recently. The objective of this study was to validate the NTEMC criteria., Methods: Endometrial cytology specimens that had been categorised as 'suspicious' were collected in our hospital between 2003 and 2013, and from these, 106 specimens with corresponding histological results, were re-evaluated according to the NTEMC criteria. Diagnostic categories were assigned based on that chosen by the majority of the examining members., Results: Negative, atypical endometrial cells, of undetermined significance (ATEC-US), atypical endometrial cells for which atypical endometrial hyperplasia or worse cannot be excluded (ATEC-A), endometrial hyperplasia, atypical endometrial hyperplasia and malignancy were selected as the diagnostic categories for 9 (8.5%), 34 (32.1%), 17 (16%), 34 (32.1%), 5 (4.7%) and 7 (6.6%) specimens, respectively. Corresponding histological categories of benign, endometrial hyperplasia, atypical endometrial hyperplasia and malignancy were established in 28 (82.4%), 1 (2.9%), 2 (5.9%) and 3 (8.8%) ATEC-US specimens, respectively, and in 6 (35.3%), 3 (17.6%), 2 (11.8%) and 6 (35.3%) ATEC-A specimens, respectively. The histological category distribution differed significantly (P = 0.001), and there was a significant correlation between corresponding cytological and histological categories (P = 0.005)., Conclusion: The ATEC category of NTEMC system works well in a practical setting and resembles the Bethesda reporting system ASC (atypical squamous cells) category for cervical cytology., (© 2016 John Wiley & Sons Ltd.)
- Published
- 2017
- Full Text
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46. The right insular cortex infarction: a critical factor for mortality?
- Author
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Nagai M, Dote K, Kato M, Sasaki S, and Oda N
- Subjects
- Brain Ischemia, Humans, Cerebral Cortex, Infarction
- Published
- 2017
- Full Text
- View/download PDF
47. Pituitary adenylate cyclase-activating polypeptide promotes eccrine gland sweat secretion.
- Author
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Sasaki S, Watanabe J, Ohtaki H, Matsumoto M, Murai N, Nakamachi T, Hannibal J, Fahrenkrug J, Hashimoto H, Watanabe H, Sueki H, Honda K, Miyazaki A, and Shioda S
- Subjects
- Adult, Animals, Female, Foot, Humans, Male, Mice, Inbred C57BL, Nerve Fibers metabolism, Pituitary Adenylate Cyclase-Activating Polypeptide metabolism, Pituitary Adenylate Cyclase-Activating Polypeptide pharmacology, RNA, Messenger metabolism, Receptors, Pituitary Adenylate Cyclase-Activating Polypeptide metabolism, Receptors, Pituitary Adenylate Cyclase-Activating Polypeptide physiology, Receptors, Vasoactive Intestinal Peptide, Type II metabolism, Receptors, Vasoactive Intestinal Peptide, Type II physiology, Receptors, Vasoactive Intestinal Polypeptide, Type I metabolism, Receptors, Vasoactive Intestinal Polypeptide, Type I physiology, Eccrine Glands metabolism, Pituitary Adenylate Cyclase-Activating Polypeptide physiology, Sweat metabolism
- Abstract
Background: Sweat secretion is the major function of eccrine sweat glands; when this process is disturbed (paridrosis), serious skin problems can arise. To elucidate the causes of paridrosis, an improved understanding of the regulation, mechanisms and factors underlying sweat production is required. Pituitary adenylate cyclase-activating polypeptide (PACAP) exhibits pleiotropic functions that are mediated via its receptors [PACAP-specific receptor (PAC1R), vasoactive intestinal peptide (VIP) receptor type 1 (VPAC1R) and VPAC2R]. Although some studies have suggested a role for PACAP in the skin and several exocrine glands, the effects of PACAP on the process of eccrine sweat secretion have not been examined., Objectives: To investigate the effect of PACAP on eccrine sweat secretion., Methods: Reverse transcriptase-polymerase chain reaction and immunostaining were used to determine the expression and localization of PACAP and its receptors in mouse and human eccrine sweat glands. We injected PACAP subcutaneously into the footpads of mice and used the starch-iodine test to visualize sweat-secreting glands., Results: Immunostaining showed PACAP and PAC1R expression by secretory cells from mouse and human sweat glands. PACAP immunoreactivity was also localized in nerve fibres around eccrine sweat glands. PACAP significantly promoted sweat secretion at the injection site, and this could be blocked by the PAC1R-antagonist PACAP6-38. VIP, an agonist of VPAC1R and VPAC2R, failed to induce sweat secretion., Conclusions: This is the first report demonstrating that PACAP may play a crucial role in sweat secretion via its action on PAC1R located in eccrine sweat glands. The mechanisms underlying the role of PACAP in sweat secretion may provide new therapeutic options to combat sweating disorders., (© 2016 British Association of Dermatologists.)
- Published
- 2017
- Full Text
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48. Inter-rater and intra-rater reliability outcomes of a rapid bacteria counting system with pressure ulcer samples.
- Author
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Nakagami G, Mori M, Yoshida M, Kitamura A, Hayashi A, Miyagaki T, Sasaki S, Sugama J, and Sanada H
- Subjects
- Aged, Aged, 80 and over, Cross-Sectional Studies, Female, Humans, Male, Middle Aged, Observer Variation, Reproducibility of Results, Bacterial Load, Pressure Ulcer microbiology, Wound Infection diagnosis
- Abstract
Objective: Evaluating bacterial load in pressure ulcers (PUs) is key to combat infection; therefore, using technologies to measure bacterial count can be particularly useful. A rapid bacteria counting system was recently developed and introduced to the wound care field. However, its reliability was not established. This cross-sectional study aimed to evaluate the inter-rater and intra-rater reliability of bacterial count using this rapid counting system., Method: We took bacterial swabs from patients with category I or greater PUs to assess inter- and intra-rater reliability. An assessor swabbed the longest axis of the PU once and bacterial counts were measured using a rapid bacteria counting system. To confirm the inter-rater and intra-rater reliability, intraclass correlation coefficients (ICCs) were calculated., Results: We took 63 and 57 pairs of bacterial counts from 13 patients with 16 category I or greater PUs to assess inter- and intra-rater reliability, respectively. Overall ICCs [95% confidence intervals (CI)] for the bacterial counts were 0.83 [0.73-0.90, p<0.001, inter-rater reliability, n=63], and 0.89 [0.82-0.94, p< 0.001, intra-rater reliability, n=57]., Conclusion: A high level of reliability for counting bacterial numbers in PU sites was confirmed. The results should encourage clinicians and researchers to use this type of device for the real-time assessment of wound bacterial bioburden at the patient's bedside.
- Published
- 2017
- Full Text
- View/download PDF
49. Effect of obesity on sperm retrieval outcome and reproductive hormone levels in Japanese azoospermic men with and without Klinefelter syndrome.
- Author
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Iwatsuki S, Sasaki S, Taguchi K, Hamakawa T, Mizuno K, Okada A, Kubota Y, Umemoto Y, Hayashi Y, and Yasui T
- Subjects
- Adult, Azoospermia blood, Body Mass Index, Humans, Japan, Klinefelter Syndrome blood, Male, Obesity blood, Semen Analysis, Sperm Retrieval, Azoospermia complications, Follicle Stimulating Hormone blood, Klinefelter Syndrome complications, Luteinizing Hormone blood, Obesity complications, Testosterone blood
- Abstract
Obesity is reported to have adverse effects on semen quality and the endocrine system. In this study, we evaluated the effect of obesity on sperm retrieval outcome and reproductive hormone levels in Japanese men with non-obstructive azoospermia (NOA). This study is based on the clinical records of 217 men [172 with a 46,XY karyotype, 45 with Klinefelter syndrome (KS)] with NOA who underwent microdissection testicular sperm extraction at Nagoya City University Hospital between January 2004 and December 2014. Body mass index (BMI) and serum levels of luteinizing hormone (LH), follicle-stimulating hormone (FSH), and total testosterone (TT) were measured in all patients. In a subset of patients, bioavailable testosterone (cBAT) also was calculated. Values were evaluated separately in patients with and without KS. Sperm retrieval rates (SRRs) in 46,XY men with a BMI <25 kg/m
2 and ≥25 kg/m2 were 29.3% and 18.4%, respectively (p = 0.142), while SRRs in KS men with a BMI <25 kg/m2 and ≥25 kg/m2 were 25.0% and 35.3%, respectively (p = 0.460). TT level in men with a BMI ≥25 kg/m2 was lower than that in men with a BMI <25 kg/m2 , regardless of KS status. According to Pearson product-moment correlation coefficients, TT and cBAT levels tended to have negative correlations with BMI; however, statistical significance was observed only for TT level in 46,XY men (r = 0.340, p < 0.001). LH and FSH levels were negatively correlated with BMI in KS men (r = -0.466, p = 0.001 and r = -0.647, p < 0.001, respectively), but not in 46,XY men. These results suggest that obesity may be irrelevant to sperm retrieval outcome in patients with NOA. The negative correlations between gonadotropins and BMI in patients with KS suggest an underlying suppressive effect on gonadotropin excretion, which is distinctive in obese patients with KS., (© 2016 American Society of Andrology and European Academy of Andrology.)- Published
- 2017
- Full Text
- View/download PDF
50. Effect of cooking classes for housewives on salt reduction in family members: a cluster randomized controlled trial.
- Author
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Takada T, Imamoto M, Fukuma S, Yamamoto Y, Sasaki S, Uchida M, Miura Y, Shimizu S, Nihata K, and Fukuhara S
- Subjects
- Aged, Cardiovascular Diseases prevention & control, Cluster Analysis, Female, Follow-Up Studies, Humans, Japan, Male, Middle Aged, Cooking, Family, Nutritional Sciences education, Sodium Chloride, Dietary administration & dosage
- Abstract
Objectives: Sodium reduction is very important in preventing cardiovascular diseases, especially in regions with high salt intake such as Japan. One strategy for salt reduction is to raise consumer awareness of the need to reduce daily salt intake. We investigated whether cooking classes given to housewives focussing on salt reduction would influence not only their own consumption behaviour but also that of their family members., Study Design: Single-blinded, cluster randomized trial., Methods: We randomly assigned housewives to participate in cooking classes focussing on salt reduction (intervention group) or lectures about a healthy lifestyle (control group). The main outcome measure was the difference in estimated daily salt intake by spot urine sampling of housewives and their family members 2 months after intervention between the groups., Results: A total of 35 housewives and 33 family members were randomized. The mean daily salt intake was 10.00 (standard deviation [SD] 1.75) g/day in the control group (17 housewives and 15 family members) and 9.57 (SD 2.45) g/day in the intervention group (18 housewives and 18 family members) at baseline. Two months after the intervention, the mean salt intake was 10.30 (SD 1.78) g/day in the control group and 8.95 (SD 2.45) g/day in the intervention group. The mean difference was -1.19 g/day (95% confidence interval -2.29, -0.09; P = 0.034). A similar tendency was observed in the subgroups of housewives and family members., Conclusions: Our trial suggested that the effects of cooking classes focussing on salt reduction for housewives could be transferred to family members (UMIN-CTR: 000018870)., (Copyright © 2016 The Royal Society for Public Health. Published by Elsevier Ltd. All rights reserved.)
- Published
- 2016
- Full Text
- View/download PDF
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