Search Results - "SUZUKI, L"

Coincident Phosphatidic Acid Interaction Restrains Drp1 in Mitochondrial Division by Adachi, Yoshihiro, Itoh, Kie, Yamada, Tatsuya, Cerveny, Kara L., Suzuki, Takamichi L., Macdonald, Patrick, Frohman, Michael A., Ramachandran, Rajesh, Iijima, Miho, Sesaki, Hiromi

“…Mitochondria divide to control their size, distribution, turnover, and function. Dynamin-related protein 1 (Drp1) is a critical mechanochemical GTPase that…”
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Molecular Gas Reservoirs in Cluster Galaxies at z = 1.46 by Hayashi, Masao, Tadaki, Ken-ichi, Kodama, Tadayuki, Kohno, Kotaro, Yamaguchi, Yuki, Hatsukade, Bunyo, Koyama, Yusei, Shimakawa, Rhythm, Tamura, Yoichi, Suzuki, Tomoko L.

“…We present molecular gas reservoirs of 18 galaxies associated with the XMMXCS J2215.9-1738 cluster at z = 1.46. From Band 7 and Band 3 data of the Atacama…”
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Structural Evolution in Massive Galaxies at z ∼ 2 by Tadaki, Ken-ichi, Belli, Sirio, Burkert, Andreas, Dekel, Avishai, Förster Schreiber, Natascha M., Genzel, Reinhard, Hayashi, Masao, Herrera-Camus, Rodrigo, Kodama, Tadayuki, Kohno, Kotaro, Koyama, Yusei, Lee, Minju M., Lutz, Dieter, Mowla, Lamiya, Nelson, Erica J., Renzini, Alvio, Suzuki, Tomoko L., Tacconi, Linda J., Übler, Hannah, Wisnioski, Emily, Wuyts, Stijn

“…We present 0 2 resolution Atacama Large Millimeter/submillimeter Array (ALMA) observations at 870 m in a stellar mass-selected sample of 85 massive ( )…”
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Correlation between star formation activity and electron density of ionized gas at z = 2.5 by Shimakawa, Rhythm, Kodama, Tadayuki, Steidel, Charles C., Tadaki, Ken-ichi, Tanaka, Ichi, Strom, Allison L., Hayashi, Masao, Koyama, Yusei, Suzuki, Tomoko L., Yamamoto, Moegi

“…In the redshift interval of 2 < z < 3, the physical conditions of the interstellar medium (ISM) in star-forming galaxies are likely to be different from those…”
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MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z = 2.2 by Shimakawa, Rhythm, Koyama, Yusei, Röttgering, Huub J A, Kodama, Tadayuki, Hayashi, Masao, Hatch, Nina A, Dannerbauer, Helmut, Tanaka, Ichi, Tadaki, Ken-ichi, Suzuki, Tomoko L, Fukagawa, Nao, Cai, Zheng, Kurk, Jaron D

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MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z = 2.5 by Shimakawa, Rhythm, Kodama, Tadayuki, Hayashi, Masao, Prochaska, J. Xavier, Tanaka, Ichi, Cai, Zheng, Suzuki, Tomoko L., Tadaki, Ken-ichi, Koyama, Yusei

“…Abstract We carried out deep H α narrowband imaging with 10 h net integrations towards the young protocluster, USS1558−003 at z = 2.53 with the Subaru…”
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A Massive Quiescent Galaxy in a Group Environment at z = 4.53 by Kakimoto, Takumi, Tanaka, Masayuki, Onodera, Masato, Shimakawa, Rhythm, Wu, Po-Feng, Gould, Katriona M. L., Ito, Kei, Jin, Shuowen, Kubo, Mariko, Suzuki, Tomoko L., Toft, Sune, Valentino, Francesco, Yabe, Kiyoto

“…We report on the spectroscopic confirmation of a massive quiescent galaxy at z spec = 4.53 in the COSMOS field. The object was first identified as a galaxy…”
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Broadband Selection, Spectroscopic Identification, and Physical Properties of a Population of Extreme Emission-line Galaxies at 3 < z < 3.7 by Onodera, Masato, Shimakawa, Rhythm, Suzuki, Tomoko L., Tanaka, Ichi, Harikane, Yuichi, Hayashi, Masao, Kodama, Tadayuki, Koyama, Yusei, Nakajima, Kimihiko, Shibuya, Takatoshi

“…We present the selection, spectroscopic identification, and physical properties of extreme emission-line galaxies (EELGs) at 3 <  z  < 3.7, aiming at studying…”
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Attention focus modulates afferent input to motor cortex during skilled action by Suzuki, L.Y., Meehan, S.K.

“…Psychomotor studies have identified a key role for attention in skill performance and acquisition. However, the neural mechanisms that underpin attention's…”
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ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field by Suzuki, Tomoko L., van Mierlo, Sophie E., Caputi, Karina I.

“…Submillimeter observations reveal the star formation activity obscured by dust in the young Universe. It still remains unclear how galaxies detected at…”
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Signs of environmental effects on star-forming galaxies in the Spiderweb protocluster at z  = 2.16 by Pérez-Martínez, J M, Dannerbauer, H, Kodama, T, Koyama, Y, Shimakawa, R, Suzuki, T L, Calvi, R, Chen, Z, Daikuhara, K, Hatch, N A, Laza-Ramos, A, Sobral, D, Stott, J P, Tanaka, I

“…We use multi-object near-infrared spectroscopy with VLT/KMOS to investigate the role of the environment in the evolution of the ionized gas properties of…”
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Environmental impacts on molecular gas in protocluster galaxies at z ∼ 2 by Tadaki, Ken-ichi, Kodama, Tadayuki, Hayashi, Masao, Shimakawa, Rhythm, Koyama, Yusei, Lee, Minju, Tanaka, Ichi, Hatsukade, Bunyo, Iono, Daisuke, Kohno, Kotaro, Matsuda, Yuichi, Suzuki, Tomoko L, Tamura, Yoichi, Toshikawa, Jun, Umehata, Hideki

“…We present the results from ALMA CO(3–2) observations of 66 Hα-selected galaxies in three protoclusters around radio galaxies: PKS 1138−262 ($z$ = 2.16), USS…”
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Spatial Extent of Molecular Gas, Dust, and Stars in Massive Galaxies at z ∼ 2.2–2.5 Determined with ALMA and JWST by Tadaki, Ken-ichi, Kodama, Tadayuki, Koyama, Yusei, Suzuki, Tomoko L., Mitsuhashi, Ikki, Ikeda, Ryota

“…We present the results of 0.″6-resolution observations of CO J = 3 − 2 line emission in 10 massive star-forming galaxies at z ∼ 2.2–2.5 with the Atacama Large…”
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High-resolution ALMA Study of CO J = 2–1 Line and Dust Continuum Emissions in Cluster Galaxies at z = 1.46 by Ikeda, Ryota, Tadaki, Ken-ichi, Iono, Daisuke, Kodama, Tadayuki, Chan, Jeffrey C. C., Hatsukade, Bunyo, Hayashi, Masao, Izumi, Takuma, Kohno, Kotaro, Koyama, Yusei, Shimakawa, Rhythm, Suzuki, Tomoko L., Tamura, Yoichi, Tanaka, Ichi

“…We present new Atacama Large Millimeter/submillimeter Array (ALMA) results obtained from spatially resolved CO J = 2–1 line (0.″4 resolution) and 870 μ m…”
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A genetic screen in C. elegans reveals roles for KIN17 and PRCC in maintaining 5' splice site identity by Suzuki, Jessie M N G L, Osterhoudt, Kenneth, Cartwright-Acar, Catiana H, Gomez, Destiny R, Katzman, Sol, Zahler, Alan M

“…Pre-mRNA splicing is an essential step of eukaryotic gene expression carried out by a series of dynamic macromolecular protein/RNA complexes, known…”
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A Universal Correlation between Star Formation Activity and Molecular Gas Properties Across Environments by Koyama, Shuhei, Koyama, Yusei, Yamashita, Takuji, Morokuma-Matsui, Kana, Matsuhara, Hideo, Nakagawa, Takao, Hayashi, Masao, Kodama, Tadayuki, Shimakawa, Rhythm, Suzuki, Tomoko L., Tadaki, Ken-ichi, Tanaka, Ichi, Yamamoto, Moegi

“…We present the molecular gas mass fraction ( ) and star formation efficiency (SFE) of local galaxies on the basis of our new CO( ) observations with the…”
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Do Galaxy Morphologies Really Affect the Efficiency of Star Formation During the Phase of Galaxy Transition? by Koyama, Shuhei, Koyama, Yusei, Yamashita, Takuji, Hayashi, Masao, Matsuhara, Hideo, Nakagawa, Takao, Namiki, Shigeru V., Suzuki, Tomoko L., Fukagawa, Nao, Kodama, Tadayuki, Lin, Lihwai, Morokuma-Matsui, Kana, Shimakawa, Rhythm, Tanaka, Ichi

“…Recent simulations predict that the presence of the stellar bulge suppress the efficiency of star formation (SF) in early-type galaxies, and this…”
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Attention modulates specific motor cortical circuits recruited by transcranial magnetic stimulation by Mirdamadi, J.L., Suzuki, L.Y., Meehan, S.K.

“…•SAI evoked by monophasic AP but not PA stimulation is reduced by increasing the attention load of a visual detection task.•Differential sensitivity to…”
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A GENERAL RETURN-MAPPING FRAMEWORK FOR FRACTIONAL VISCO-ELASTO-PLASTICITY by Suzuki, Jorge L, Naghibolhosseini, Maryam, Zayernouri, Mohsen

“…We develop a fractional return-mapping framework for power-law visco-elasto-plasticity. In our approach, the fractional viscoelasticity is accounted through…”
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Modulation of formin processivity by profilin and mechanical tension by Cao, Luyan, Kerleau, Mikael, Suzuki, Emiko L, Wioland, Hugo, Jouet, Sandy, Guichard, Berengere, Lenz, Martin, Romet-Lemonne, Guillaume, Jegou, Antoine

“…Formins are major regulators of actin networks. They enhance actin filament dynamics by remaining processively bound to filament barbed ends. How biochemical…”
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