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Journal articles on the topic 'RM 12'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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1

Yamaji, Akihiro, Vladimir V. Kochurikhin, Shunsuke Kurosawa, Akira Suzuki, Yutaka Fujimoto, Yuui Yokota, and Akira Yoshikawa. "Luminescence Properties of ${\rm Gd}_{3}{\rm Ga}_{5}{\rm O}_{12}$:${\rm Cr}$ Single Crystals." IEEE Transactions on Nuclear Science 61, no. 1 (February 2014): 320–22. http://dx.doi.org/10.1109/tns.2013.2290550.

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2

Wei, Qinhua, Guanghui Liu, Zhenzhen Zhou, Hua Yang, Jiandong Zhuang, and Qian Liu. "Preparation and Luminescence Properties of ${\rm Bi}_{4}{\rm Si}_{3}{\rm O}_{12}\!:\!{\rm Zn}$ Powders." IEEE Transactions on Nuclear Science 61, no. 1 (February 2014): 328–31. http://dx.doi.org/10.1109/tns.2013.2272833.

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3

Kamada, Kei, Petr Prusa, Martin Nikl, Karel Blazek, Takanori Endo, Kousuke Tsutsumi, Shunsuke Kurosawa, Yuui Yokota, and Akira Yoshikawa. "Czochralski Growth and Scintillation Properties of ${\rm Ce}:({\rm Gd},{\rm Y},{\rm Lu})_3$$({\rm Al},{\rm Ga})_5{\rm O}_{12}$ Single Crystals." IEEE Transactions on Nuclear Science 61, no. 1 (February 2014): 293–96. http://dx.doi.org/10.1109/tns.2013.2285613.

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4

Drozdowski, Winicjusz, Pieter Dorenbos, Johan T. M. de Haas, Renata Drozdowska, Alan Owens, Kei Kamada, Kousuke Tsutsumi, Yoshiyuki Usuki, Takayuki Yanagida, and Akira Yoshikawa. "Scintillation Properties of Praseodymium Activated ${\rm Lu}_{3}{\rm Al}_{5}{\rm O} _{12}$ Single Crystals." IEEE Transactions on Nuclear Science 55, no. 4 (August 2008): 2420–24. http://dx.doi.org/10.1109/tns.2008.2000845.

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5

Kamada, Kei, Takayuki Yanagida, Kousuke Tsutsumi, Yoshiyuki Usuki, Mitsuhiro Sato, Hiraku Ogino, Andrey Novoselov, et al. "Scintillation Properties of 2-Inch-Diameter ${\rm Pr}:{\rm Lu}_{3}{\rm Al}_{5}{\rm O}_{12}$ (LuAG) Single Crystal." IEEE Transactions on Nuclear Science 56, no. 3 (June 2009): 570–73. http://dx.doi.org/10.1109/tns.2009.2019751.

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6

Yamaji, A., T. Yanagida, Y. Yokota, K. Kamada, A. Yoshikawa, and J. Pejchal. "Quantitive Research of the Crystallinity of Pr Doped ${\rm Lu}_{3}{\rm Al}_{5}{\rm O}_{12}$." IEEE Transactions on Nuclear Science 59, no. 5 (October 2012): 2135–40. http://dx.doi.org/10.1109/tns.2012.2189895.

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7

Yu, Haohai, Kui Wu, Bin Yao, Huaijin Zhang, Zhengping Wang, Jiyang Wang, Yongdong Zhang, et al. "Growth and Characteristics of Yb-doped ${\rm Y}_{3}{\rm Ga}_{5}{\rm O}_{12}$ Laser Crystal." IEEE Journal of Quantum Electronics 46, no. 12 (December 2010): 1689–95. http://dx.doi.org/10.1109/jqe.2010.2059373.

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8

Li, Changsheng, and Rong Zeng. "Optical Voltage Sensor Using Single Fresnel Rhomb ${\rm Bi}_{4}{\rm Ge}_{3}{\rm O}_{12}$ Crystal." IEEE Sensors Journal 14, no. 1 (January 2014): 79–84. http://dx.doi.org/10.1109/jsen.2013.2279919.

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9

Kamada, K., T. Yanagida, J. Pejchal, M. Nikl, T. Endo, K. Tsutsumi, Y. Fujimoto, A. Fukabori, and A. Yoshikawa. "Crystal Growth and Scintillation Properties of Ce Doped ${\rm Gd}_{3}({\rm Ga},{\rm Al})_{5}{\rm O}_{12}$ Single Crystals." IEEE Transactions on Nuclear Science 59, no. 5 (October 2012): 2112–15. http://dx.doi.org/10.1109/tns.2012.2197024.

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10

Jodoin, Danielle. "Rm 12, 1-2 une intrigue discursive." Études théologiques et religieuses 85, no. 4 (2010): 499. http://dx.doi.org/10.3917/etr.0854.0499.

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11

ISAKA, MASAHIRO, HIROAKI HONMA, MASAAKI KIMURA, AKINOBU DOTÉ, and AKIRA OHNISHI. "IMPURITY EFFECTS IN $_\Lambda^{12}{\rm{Be}}$ AND $_\Lambda^{21}{\rm{Ne}}$ HYPERNUCLEI." International Journal of Modern Physics E 20, no. 04 (April 2011): 859–62. http://dx.doi.org/10.1142/s0218301311018848.

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The structures of the ground and low-lying states of [Formula: see text] and [Formula: see text] hypernuclei are studied with AMD. By a Λ hyperon, the parity reversion of the [Formula: see text] ground state and binding of the unbound α + 16 O cluster state in [Formula: see text] are found. Furthermore, intra-band B(E2) reduction in the [Formula: see text] band of [Formula: see text] is larger than that in the [Formula: see text] band, because of the reduction of the inter-cluster distance between α and 16 O cluster of the [Formula: see text] band.

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12

Martin, Thierry, Paul-Antoine Douissard, Zachary Seeley, Nerine Cherepy, Stephen Payne, Eric Mathieu, and Jan Schuladen. "New High Stopping Power Thin Scintillators Based on ${\rm Lu}_{2}{\rm O}_{3}$ and ${\rm Lu}_{3}{\rm Ga}_{5-{\rm x}}{\rm In}_{\rm x}{\rm O}_{12}$ for High Resolution X-ray Imaging." IEEE Transactions on Nuclear Science 59, no. 5 (October 2012): 2269–74. http://dx.doi.org/10.1109/tns.2012.2189248.

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13

Tyagi, Mohit, Harold E. Rothfuss, Samuel B. Donnald, Merry Koschan, and Charles L. Melcher. "Effect of ${\rm Ca}^{2+}$ Co-Doping on the Scintillation Kinetics of Ce Doped ${\rm Gd}_{3}{\rm Ga}_{3}{\rm Al}_{2}{\rm O}_{12}$." IEEE Transactions on Nuclear Science 61, no. 1 (February 2014): 297–300. http://dx.doi.org/10.1109/tns.2013.2276101.

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14

Liu, Shande, Zhitai Jia, Jingliang He, Baitao Zhang, Xiuqin Yang, Fengqin Liu, Jinlong Xu, and Xu-Tang Tao. "Diode-Pumped Passively Q-Switched ${\rm Nd}{:}({\rm Lu}_{0.1}{\rm Gd}_{0.9})_{3}{\rm Ga}_{5}{\rm O}_{12}$ Laser at 1330 nm With ${\rm V}^{3+}{:}{\rm YAG}$ as Saturable Absorber." IEEE Photonics Technology Letters 24, no. 2 (January 2012): 146–48. http://dx.doi.org/10.1109/lpt.2011.2174353.

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15

Zorenko, Yuriy, Vitaliy Gorbenko, Volodymyr Savchyn, Tanya Zorenko, Alexander Fedorov, and Oleg Sidletskiy. "Novel Scintillating Screens Based on the Single Crystalline Films of Ce Doped Multi-Component $({\rm Gd},{\rm Y},{\rm Lu})_{3}({\rm Al},{\rm Sc})_{5}{\rm O}_{12}$ Garnets." IEEE Transactions on Nuclear Science 61, no. 1 (February 2014): 439–42. http://dx.doi.org/10.1109/tns.2013.2282260.

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16

Gargala, Gilles, Arnaud François, Loïc Favennec, and Jean-François Rossignol. "Activity of Halogeno-Thiazolides against Cryptosporidium parvum in Experimentally Infected Immunosuppressed Gerbils (Meriones unguiculatus)." Antimicrobial Agents and Chemotherapy 57, no. 6 (March 11, 2013): 2821–23. http://dx.doi.org/10.1128/aac.01538-12.

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ABSTRACTNitazoxanide and three halogeno-thiazolides, RM-4850, RM-4865, and RM-5038, were tested againstCryptosporidium parvumin experimentally infected immunosuppressed Mongolian gerbils. Daily 400-mg/kg doses of the four test drugs for 5 to 8 consecutive days produced similar reductions of oocyst shedding. Using early-infected gerbils, a shorter 4-day treatment with RM-5038 reduced oocyst shedding by 95%, compared to 47% for nitazoxanide (P= 0.02), suggesting that RM-5038 is more effective than nitazoxanide under the experimental conditions used.

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17

Tyagi, Mohit, Fang Meng, Merry Koschan, A. K. Singh, Charles L. Melcher, and S. C. Gadkari. "Effect of Co-doping On the Radiation Hardness of ${{\rm Gd}_3}{{\rm Ga}_3}{{\rm Al}_2}{{\rm O}_{12}}$: Ce Scintillators." IEEE Transactions on Nuclear Science 62, no. 1 (February 2015): 336–39. http://dx.doi.org/10.1109/tns.2014.2387834.

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18

Kamada, Kei, Kousuke Tsutsumi, Yoshiyuki Usuki, Hiraku Ogino, Takayuki Yanagida, and Akira Yoshikawa. "Crystal Growth and Scintillation Properties of 2-Inch-Diameter ${\rm Pr}:{\rm Lu}_{3}{\rm Al}_{5} {\rm O} _{12}$ (Pr:LuAG) Single Crystal." IEEE Transactions on Nuclear Science 55, no. 3 (June 2008): 1488–91. http://dx.doi.org/10.1109/tns.2008.924072.

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19

Castro González, A., E. Díez Alonso, J. Menéndez Blanco, John H. Livingston, Jerome P. de Leon, S. L. Suárez Gómez, C. González Gutiérrez, et al. "Planetary candidates transiting cool dwarf stars from campaigns 12 to 15 of K2." Monthly Notices of the Royal Astronomical Society 499, no. 4 (November 5, 2020): 5416–41. http://dx.doi.org/10.1093/mnras/staa2353.

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ABSTRACT We analysed the photometry of 20 038 cool stars from campaigns 12, 13, 14, and 15 of the K2 mission in order to detect, characterize, and validate new planetary candidates transiting low-mass stars. We present a catalogue of 25 new periodic transit-like signals in 22 stars, of which we computed the parameters of the stellar host for 19 stars and the planetary parameters for 21 signals. We acquired speckle and AO images, and also inspected archival Pan-STARRS1 images and Gaia DR2 to discard the presence of close stellar companions and to check possible transit dilutions due to nearby stars. False positive probability (FPP) was computed for 22 signals, obtaining FPP < $1{{\ \rm per\ cent}}$ for 17. We consider 12 of them as statistically validated planets. One signal is a false positive and the remaining 12 signals are considered as planet candidates. 20 signals have an orbital period of P$_{\rm orb} \lt 10\,\mathrm{ d}$, 2 have $10\, \mathrm{ d} \lt $ P$_{\rm orb} \lt 20\, \mathrm{ d}$, and 3 have P$_{\rm orb} \gt 20\, \mathrm{ d}$. Regarding radii, 11 candidates and validated planets have computed radius R < 2R⊕, 9 have 2R⊕ < R < 4R⊕, and 1 has R > 4R⊕. Two validated planets and two candidates are located in moderately bright stars ($\rm \mathit{ m}_{kep}\lt 13$) and two validated planets and three candidates have derived orbital radius within the habitable zone according to optimistic models. Of special interest is the validated warm super-Earth K2-323 b (EPIC 248616368 b) with T$_{\rm eq} = 318^{+24}_{-43} \, \mathrm{ K}$, S$_{\rm p} = 1.7\pm 0.2 \, \mathrm{ S}_{\oplus }$, and R$_{\rm p} = 2.1\pm 0.1 \, \mathrm{ R}_{\oplus }$, located in an m$\rm _{kep}$ = 14.13 star.

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20

Mengle, Kelsey A., Emily J. Longenecker, Matthias Zeller, and Curtis M. Zaleski. "One-Dimensional Coordination Polymers of 12-Metallacrown-4 Complexes: {Na2(L)2[12- $${\rm{M}}{{\rm{C}}_{{\rm{M}}{{\rm{n}}^{{\rm{III}}}}{\rm{(N)shi}}}}$$ M C M n III ( N ) shi -4]} n , where L is Either −O2CCH2CH3 or −O2CCH2CH2CH3." Journal of Chemical Crystallography 45, no. 1 (December 13, 2014): 36–43. http://dx.doi.org/10.1007/s10870-014-0560-0.

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21

Gude, Philipp, Claudia Rieckert, Nicolai Bissantz, Thomas Peter Weber, Heike Vogelsang, Stefan Dazert, and Jan Peter Thomas. "Analgetikabedarf bei Kindern im Alter zwischen 2 und 12 Jahren nach Tonsillenoperationen." Laryngo-Rhino-Otologie 97, no. 07 (April 16, 2018): 465–73. http://dx.doi.org/10.1055/a-0596-7675.

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Zusammenfassung Hintergrund Mandeloperationen bei Kindern zählen zu den schmerzhaftesten Eingriffen. Altersgerechte Schmerzskalen sind die Kindliche Unbehagens- und Schmerzskala (KUSS), die Faces Pain Scale–Revised (FPS-R) und der kaum bekannte PPPM-D-Fragebogen. Ziel war Evaluation der Analgesie bei durch Eltern angeforderter Nichtopioid-Medikation (NOM) mit Ibuprofen (IBU) und Paracetamol (PCM) nach intrakapsulärer Tonsillektomie (TO) oder extrakapsulärer Tonsillektomie (TE). Als Rescue-Medikation (RM) wurde nach Prüfung der Schmerzskalen Piritramid appliziert. Endpunkte waren Anteil der Patienten (PAT), der die RM benötigte, Menge applizierter NOM, Übereinstimmung der Indikation in verschiedenen Schmerzskalen, Korrelation von Schmerzen mit Prämedikation und Eingriffsdauer. Material/Methoden Postoperativ erfolgten 3 Messungen täglich mit KUSS bei PAT ≤ 4 Jahre bzw. FPS-R ≥ 5 Jahre. Eltern füllten den PPPM-D aus. Bei einem Wert ≥ 4 bei KUSS bzw. FPS-R oder ≥ 6 im PPPM-D wurde die RM indiziert. Ergebnisse 68 PAT wurden in eine Zwischenauswertung eingeschlossen. Durchschnittliche tägliche NOM in den ersten 3 Tagen: nach TE 14,1–16,3 mg/Kg IBU und 4,2–12,4 mg/Kg PCM bzw. nach TO 10,8–14,7 mg/Kg IBU und 5,2–8,8 mg/Kg PCM. Bei 212 Visiten wurde die RM indiziert, davon 121 Mal nur durch den PPPM-D. Nach Ausschluss eventuell falsch-positiver Indikationen benötigten 67 % der PAT nach TE und 48 % der PAT nach TO mindestens einmal die RM. Die Studie wurde wegen des hohen RM-Bedarfs abgebrochen. Schlussfolgerungen Der Bedarf an NOM wurde unterschätzt. Der PPPM-D kombiniert mit etablierten Skalen kann die postoperative Schmerztherapie verbessern.

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22

Sofue, Yoshiaki, and Mikito Kohno. "CO-to-H2 conversion and spectral column density in molecular clouds: the variability of the XCO factor." Monthly Notices of the Royal Astronomical Society 497, no. 2 (July 13, 2020): 1851–61. http://dx.doi.org/10.1093/mnras/staa2056.

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ABSTRACT Analysing the Galactic plane CO survey with the Nobeyama 45-m telescope, we compared the spectral column density (SCD) of $N_{\rm H_2}$ calculated for the 12CO (J = 1–0) line using the current conversion factor $X_{\rm ^{12}CO}$ to that for the 13CO (J = 1–0) line under the LTE (local thermal equilibrium) assumption in the M16 and W43 regions. Here, SCD is defined by $\mathrm{d}N_{\rm H_2}/\mathrm{d}v$ with $N_{\rm H_2}$ and v being the column density and radial velocity, respectively. It is found that the $X_{\rm ^{12}CO}$ method significantly underestimates the H2 density in a cloud or region, where SCD exceeds a critical value (∼3 × 1021 [H2 cm−2 (km s−1)−1]), but overestimates in lower SCD regions. We point out that the actual CO-to-H2 conversion factor varies with the H2 column density or with the CO line intensity: it increases in the inner and opaque parts of molecular clouds, whereas it decreases in the low-density envelopes. However, in so far as the current $X_{^{12}{\rm CO}}$ is used combined with the integrated 12CO intensity averaged over an entire cloud, it yields a consistent value with that calculated using the 13CO intensity by LTE. Based on the analysis, we propose a new CO-to-H2 conversion relation, $N_{\rm H_2}^* = \int X^*_{\rm CO} (T_{\rm B}) T_{\rm B}\ \mathrm{d}v$, where $X^*_{\rm CO} (T_{\rm B})=(T_{\rm B}/T_{\rm B}^*)^\beta X_{\rm ^{12}CO}$ is the modified spectral conversion factor as a function of the brightness temperature, TB, of the 12CO (J = 1–0) line, and β ∼ 1–2 and $T_{\rm B}^*=12\!-\!16$ K are empirical constants obtained by fitting to the observed data. The formula corrects for the over/underestimation of the column density at low/high CO line intensities, and is applicable to molecular clouds with TB ≥ 1 K (12CO (J = 1–0) line rms noise in the data) from envelope to cores at sub-parsec scales (spatial resolution).

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23

Yu, Bin, B. Q. Chen, B. W. Jiang, and A. Zijlstra. "Three-dimensional dust mapping of 12 supernovae remnants in the Galactic anticentre." Monthly Notices of the Royal Astronomical Society 488, no. 3 (July 22, 2019): 3129–42. http://dx.doi.org/10.1093/mnras/stz1940.

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ABSTRACT We present three-dimensional (3D) dust mapping of 12 supernova remnants (SNRs) in the Galactic anticentre (Galactic longitude l between 150○ and 210○) based on a recent 3D interstellar extinction map. The dust distribution of the regions, which cover the full extents in the radio continuum for the individual SNRs, is discussed. Four SNRs show significant spatial coincidences between molecular clouds (MCs) revealed from the 3D extinction mapping and the corresponding radio features. The results confirm the interactions between these SNRs and their surrounding MCs. Based on these correlations, we provide new distance estimates of the four SNRs, G189.1+3.0 (IC443, $d=1729^{+116}_{-94} \rm \, pc$), G190.9–2.2 ($d=1036^{+17}_{-81} \rm \, pc$), G205.5+0.5 ($d=941^{+96}_{-94}$ or $1257^{+92}_{-101} \rm \, pc$), and G213.0–0.6 ($d=1146^{+79}_{-80} \rm \, pc$). In addition, we find indirect evidences of potential interactions between SNRs and MCs for three other SNRs. New distance constraints are also given for these three SNRs.

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24

Moon, K. W., K. W. Jeon, and J. Kim. "Synthesis and Magnetic Properties of BaFe$_{12- {\rm x}}$Al$_{\rm x}$O$_{19}$ Nanopowders." IEEE Transactions on Magnetics 45, no. 10 (October 2009): 4405–8. http://dx.doi.org/10.1109/tmag.2009.2024125.

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25

da Silva, Jurandir Baptista, Vicente Pinheiro Lima, Gabriel Andrade Paz, Caroline Reis de Oliveira, Francisco D’urso, Rodolfo de Alkmim Moreira Nunes, Juliana Brandão Pinto de Castro, and Rodrigo Gomes de Souza Vale. "Determination and comparison of time under tension required to perform 8, 10 and 12-RM loads in the bench press exercise." Biomedical Human Kinetics 8, no. 1 (December 5, 2016): 153–58. http://dx.doi.org/10.1515/bhk-2016-0022.

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SummaryStudy aim: To determine and compare the time under tension (TUT) required to perform 8, 10 and 12 repetition maximum (RM) loads in the bench press exercise. Material and methods: Twenty men (24.17 ± 4.69 years) were selected intentionally and properly. We included in the study physically active individuals, with a weekly frequency of physical activity of at least two days for six months, and excluded individuals with injury or pain that could interfere with the correct execution of the exercise and individuals with positive PAR-Q. The 10-RM test consisted in performing ten consecutive repetitions with maximum overload and the highest speed in bench press exercise on the Smith machine. After 48 h, 10-RM sets were performed with the load obtained in the 10-RM load testing. The TUT in 10-RM was verified through kinematics using the timing technique of the Kinovea software. Results: The RM loads and TUT obtained during the retest session showed normal distribution between subjects. However, no significant differences were found between the loads 8, 10 and 12-RM within and between subjects (p < 0.05). The verified TUT showed a difference from 8 to 10-RM and from 8 to 12-RM, but no significant difference was found between TUT protocols for 10 and 12-RM (p < 0.05). Conclusion: The study results enable evaluation of TUT in bench press exercise on the Smith machine for the study sample, allowing, for this group, the prediction and control of training intensity through the TUT.

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26

Kamada, K., T. Yanagida, J. Pejchal, M. Nikl, T. Endo, K. Tsutumi, Y. Fujimoto, A. Fukabori, and A. Yoshikawa. "Crystal Growth of Ce Doped $({\rm Lu},{\rm Y})_{3}({\rm Ga},{\rm Al})_{5} {\rm O}_{12}$ Single Crystal by the Micro-Puling-Down Method and Their Scintillation Properties." IEEE Transactions on Nuclear Science 59, no. 5 (October 2012): 2116–19. http://dx.doi.org/10.1109/tns.2012.2184141.

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27

Hjort, Klas, Daniel Hellström, Stefan Karlsson, and Pejvak Oghazi. "Typology of practices for managing consumer returns in internet retailing." International Journal of Physical Distribution & Logistics Management 49, no. 7 (August 20, 2019): 767–90. http://dx.doi.org/10.1108/ijpdlm-12-2017-0368.

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Purpose The purpose of this paper is to explore, describe and categorise practices of managing product returns empirically in internet retailing. Design/methodology/approach A multiple case study was conducted involving 12 e-commerce firms and 4 logistics service providers. An integrative data collection approach of semi-structured interviews, documentation and observations was used to gain comprehensive managerial and operational descriptions of returns management (RM) processes. Findings The findings show inconsistent RM processes, with a plethora of practices implemented and organised differently across firms. RM processes are ambiguous; their design is a result of incremental changes over time, lacking strategy and goals. There is a mismatch between how they are described and understood in the literature and how they are actually used. Practices in gatekeeping, avoidance and reverse logistics are defined and categorised. These serve as a typology of practices for managers to (re)consider, along with 15 propositions on how RM is practised. Research limitations/implications The range of RM practices and the processes reflect a lack of scholarly attention and strategic view. Research is needed to develop clear goals on how the RM process can be better aligned with business strategies. Practical implications The typology of practices is a benchmark for internet retailers in their design of efficient RM processes. Originality/value Systematic and empirical research on RM is scarce compared to forward management. The study bridges this gap as one of the first to describe RM practices in depth, define service as a key activity, and identify a mismatch between theory and practice.

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28

Liu, Junhai, Qibiao Dai, Wenjuan Han, Kui Wu, Huaijin Zhang, and Shiwu Wang. "Efficient Q-Switched Miniature ${\rm Yb{:}Gd}_{3}{\rm Ga}_{5}{\rm O}_{12}$ Laser Generating 180 kW of Peak Power." IEEE Photonics Technology Letters 25, no. 21 (November 2013): 2078–80. http://dx.doi.org/10.1109/lpt.2013.2281411.

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29

Benayas, Antonio, Daniel Jaque, Carlos Jacinto, and Alexander A. Kaminskii. "Luminescence Quantum Efficiency of ${\rm Nd}^{3+}{\colon}{\rm Y}_{3}{\rm Al}_{5}{\rm O}_{12}$ Garnet Laser Ceramics Determined by Pump-Induced Line Broadening." IEEE Journal of Quantum Electronics 46, no. 12 (December 2010): 1870–76. http://dx.doi.org/10.1109/jqe.2010.2060315.

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30

Panchagnula, Sanjana, Jordy Bouwman, Jerry Kamer, Harold Linnartz, and Alexander Tielens. "Photofragmentation of coronene cations." Proceedings of the International Astronomical Union 15, S350 (April 2019): 402–3. http://dx.doi.org/10.1017/s1743921319008068.

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AbstractRecent laboratory studies have shown that PAH cations dehydrogenate to give charged molecules consisting of only carbon atoms. Our experiments using ion-trap time-of-flight mass spectrometry show that a key group of photodissociation fragments from the coronene cation $({{\rm{C}}_{24}}{\rm{H}}_{12}^ + )$ are carbon clusters of ${\rm{C}}_n^ +$ composition. Density functional theory calculations shed light onto potential dissociation pathways leading up to the main ${\rm{C}}_{11}^ +$ and ${\rm{C}}_{12}^ +$ clusters, and highlight the importance of pentagon formations in the carbon backbone of the precursor molecule in generating certain fragments.

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31

Fedotov, S. I., O. I. Kartavtsev, and A. V. Malykh. "Consistent Description of the $${^{12}{\rm C}(0_2^+)}$$ State." Few-Body Systems 45, no. 2-4 (March 7, 2009): 153–55. http://dx.doi.org/10.1007/s00601-009-0044-5.

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32

Jiang, Hongkai, Yong Xia, and Xiaodong Wang. "Rolling bearing fault detection using an adaptive lifting multiwavelet packet with a ${{\rm 1}\frac{{\rm 1}}{{\rm 2}}}$ dimension spectrum." Measurement Science and Technology 24, no. 12 (November 12, 2013): 125002. http://dx.doi.org/10.1088/0957-0233/24/12/125002.

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33

Torre, D., F. Speranza, A. Pugliese, L. Perversi, P. Marone, and G. Ferrario. "Effects of Recombinant Murine (rm) Interleukin-12 and rm Interferon- in Mice Infected with Bordetella pertussis." Journal of Infectious Diseases 174, no. 4 (October 1, 1996): 786–89. http://dx.doi.org/10.1093/infdis/174.4.786.

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34

Ispoglou, Theocharis, Roderick F. G. J. King, Remco C. J. Polman, and Cathy Zanker. "Daily L-Leucine Supplementation in Novice Trainees During a 12-Week Weight Training Program." International Journal of Sports Physiology and Performance 6, no. 1 (March 2011): 38–50. http://dx.doi.org/10.1123/ijspp.6.1.38.

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Purpose:To investigate the effects of daily oral L-leucine ingestion on strength, bone mineral-free lean tissue mass (LTM) and fat mass (FM) of free living humans during a 12-wk resistance-training program.Methods:Twenty-six initially untrained men (n = 13 per group) ingested either 4 g/d of L-leucine (leucine group: age 28.5 ± 8.2 y, body mass index 24.9 ± 4.2 kg/m2) or a corresponding amount of lactose (placebo group: age 28.2 ± 7.3 y, body mass index 24.9 ± 4.2 kg/m2). All participants trained under supervision twice per week following a prescribed resistance training program using eight standard exercise machines. Testing took place at baseline and at the end of the supplementation period. Strength on each exercise was assessed by fve repetition maximum (5-RM), and body composition was assessed by dual energy X-ray absorptiometry (DXA).Results:The leucine group demonstrated significantly higher gains in total 5-RM strength (sum of 5-RM in eight exercises) and 5-RM strength in five out of the eight exercises (P < .05). The percentage total 5-RM strength gains were 40.8% (± 7.8) and 31.0% (± 4.6) for the leucine and placebo groups respectively. Significant differences did not exist between groups in either total percentage LTM gains or total percentage FM losses (LTM: 2.9% ± 2.5 vs 2.0% ± 2.1, FM: 1.6% ± 15.6 vs 1.1% ± 7.6).Conclusion:These results suggest that 4 g/d of L-leucine supplementation may be used as a nutritional supplement to enhance strength performance during a 12-week resistance training program of initially untrained male participants.

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Atsuyama, Kenji. "The connection between the symmetric space $E_7/{\rm SO}(12)\cdot {\rm SO}(3)$ and projective planes." Kodai Mathematical Journal 9, no. 3 (1986): 334–50. http://dx.doi.org/10.2996/kmj/1138037262.

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Tarei, Pradeep Kumar, Jitesh J. Thakkar, and Barnali Nag. "Benchmarking the relationship between supply chain risk mitigation strategies and practices: an integrated approach." Benchmarking: An International Journal 27, no. 5 (April 28, 2020): 1683–715. http://dx.doi.org/10.1108/bij-12-2019-0523.

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PurposeThe purpose of this paper is to explore the relationship between various risk management strategies and risk management practices in order to design and hence enact a suitable supply chain risk mitigation (RM) plan. Additionally, this study proposes a hierarchical framework to explain the mutual relationship between supply chain risk management (SCRM) practices and strategies by considering the underlying dimensions between them.Design/methodology/approachAn amalgamation of systematic literature analysis (SLA) and correspondence analysis (CA) has been performed to develop the conceptual framework. A real-life case of Indian petroleum supply chain has been considered to validate and explain the proposed model.FindingsThe results reveal three underlying dimensions, which associate the relationship between RM strategies. They are, risk adaptability of SC managers with a variance of 34.71%, followed by resource capability of the firm and the degree of sophistication of RM practices, with variances of 27.72 and 20.35%, respectively. Risk avoidance strategy comprises of practices such as supplier evaluation, technology adaption, flexible process and information security. On the other extreme, the risk sharing strategy includes revenue sharing, insurance, collaboration, public–private partnership and so on as essential RM practices.Research limitations/implicationsThe study not only focuses on the distinction between RM strategies and practices, which were used interchangeably in the prior literature, but also provides an association between the same by exploring the underlying dimensions. These underlying dimensions perform a crucial role while developing a risk management plan. This study explicitly focuses on the RM step of SCRM process. Pre and post risk mitigation phases of SCRM process, such as risk assessment and risk monitoring, are beyond the scope of the current research.Originality/valueThe paper develops a framework for mapping various RM strategies with their corresponding practices by considering the Indian petroleum supply chain as a viable case study. Various theoretical and business implications are derived in the context of the developing country.

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Vandenbrouck, S., K. Madjour, D. Theron, Yajie Dong, Yat Li, C. M. Lieber, and C. Gaquiere. "12 GHz $F_{\rm MAX}$GaN/AlN/AlGaN Nanowire MISFET." IEEE Electron Device Letters 30, no. 4 (April 2009): 322–24. http://dx.doi.org/10.1109/led.2009.2014791.

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WEHRFRITZ, B. A. F. "Finitary and Artinian-finitary groups." Mathematical Proceedings of the Cambridge Philosophical Society 143, no. 2 (September 2007): 291–305. http://dx.doi.org/10.1017/s0305004107000485.

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AbstractLet M be a module over the ring R. The finitary automorphism group of M over R is and the Artinian-finitary automorphism group of M over R is We continue our study begun in [9] and [12] of the relationship between these two in some ways similar, but actually quite different types of automorphism group. Our study here involves the generalized finitary group $\{{\rm g} \in {\rm Aut}_{\rm R}{\rm M}{:}\,{\rm M}({\rm g} - 1)$ embeds into some finitely generated R-module which does not fit our earlier pattern of generalized finitary groups as described in [8].

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Fera, F., A. Armentano, P. Bartone, G. Ginolfi, C. Ceccotti, and K. Pardatscher. "Il ruolo della tomografia RM e dell'Angio-RM nello studio degli aneurismi cerebrali." Rivista di Neuroradiologia 10, no. 2_suppl (October 1997): 145–48. http://dx.doi.org/10.1177/19714009970100s259.

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To evaluate the reliability of magnetic resonance angiography for detecting intracranial aneurysms a prospective study was performed in 21 consecutive patients affected by SAH and in 13 patients in whom aneurysms were suspected on standard SE RM. In the SAH cohort 8 of 21 clearly showed an aneurysm, 3 of 21 were doubtfull. In the 13 patients without SAH, aneurysms were confirmed in 12. Due to flow artefacts in the small aneurysms a deceptive pseudoloop pattern was often observed.

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40

Ranjan, Prabhat, Tanmoy Chakraborty, and Ajay Kumar. "Density functional study of structures, stabilities and electronic properties of AgAunλ(λ=0,±1;n=1-12){\rm{AgAu}}_n^\lambda \left( {\lambda = 0, \pm 1;n = 1 - 12} \right) clusters: comparison with pure gold clusters." Materials Science-Poland 38, no. 1 (March 1, 2020): 97–107. http://dx.doi.org/10.2478/msp-2020-0014.

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AbstractGeometrical structures, relative stabilities and electronic properties of neutral, cationic and anionic pure gold {\rm{A}}u_{n + 1}^\lambda and Ag-doped bimetallic {\rm{AgAu}}_n^\lambda \left( {\lambda = 0, \pm 1;n = 1 - 12} \right) clusters have been systematically investigated by using density functional theory methodology. The optimized structures show that planar to three-dimensional structural transition occurs at n = 5 for cationic clusters. Due to strong relativistic effect of Au clusters, the ground state configurations of neutral and anionic bimetallic clusters favor planar geometry till n = 12. Silver atoms tend to occupy the most highly coordinated position and form the maximum number of bonds with Au atoms. The computed HOMO-LUMO energy gaps, fragmentation energies and second-order difference of energies show interesting odd-even oscillation behavior. The result indicates that AgAu5, {\rm{AgAu}}_2^ + and {\rm{AgAu}}_2^ - are the most stable clusters in this molecular system. The DFT based descriptors of bimetallic clusters are also discussed and compared with pure gold clusters. The high value of correlation coefficient between HOMO-LUMO energy gaps and DFT based descriptors supports our analysis. A good agreement between experimental and theoretical data has been obtained in this study.

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Ma, Hongliang, Mingguo Sun, Shenlong Zha, Qiang Liu, Zhensong Cao, Yinbo Huang, Zhu Zhu, and Ruizhong Rao. "Temperature dependence of line parameters of ${}^{12}\rm{C}{}^{16}\rm{O}_{2}$ near $2.004\,{\rm{\mu }}m$ studied by tunable diode laser spectroscopy." Chinese Physics B 27, no. 2 (February 2018): 023301. http://dx.doi.org/10.1088/1674-1056/27/2/023301.

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42

Calette, A. R., Aldo Rodríguez-Puebla, Vladimir Avila-Reese, and Claudia del P. Lagos. "The galaxy H i–(sub)halo connection and the H i spatial clustering of local galaxies." Monthly Notices of the Royal Astronomical Society 506, no. 1 (June 26, 2021): 1507–25. http://dx.doi.org/10.1093/mnras/stab1788.

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ABSTRACT We extend the local stellar galaxy–(sub)halo connection to the atomic hydrogen (H i) component by seeding semi-empirically galaxies into a large N-body dark matter (DM) simulation. The main input to construct the mock galaxy catalogue are: our constrained stellar mass-to-(sub)halo circular velocity (M*–VDM) relation, assuming a scatter independent of any galaxy property, and the empirical $M_{\rm H\, \small {I}}$ conditional probability distributions given M* for central and satellite galaxies. We find that the $\langle \log \mbox{$M_{\rm H\, \small {I}}$}\rangle -\log \mbox{$M_{\rm DM}$}$ relation is not a monotonic increasing function. It increases with mass up to $\mbox{$M_{\rm DM}$}\sim 10^{12}$ M⊙, attaining a maximum of $\langle \log (\mbox{$M_{\rm H\, \small {I}}$}/\mbox{M$_{\odot }$})\rangle \sim 9.2$, and at higher (sub)halo masses, $\langle \log (\mbox{$M_{\rm H\, \small {I}}$})\rangle$ decreases slightly with MDM. The scatter around it is also large and mass dependent. The bivariate $M_{\rm H\, \small {I}}$ and MDM distribution is broad and bimodal, specially at $\mbox{$M_{\rm DM}$}\gtrsim 10^{12}$ M⊙, which is inherited from the input $M_{\rm H\, \small {I}}$ conditional distributions. We also report the total (central+satellites) H i gas mass within haloes, $M^{\rm tot}_{\rm H\, \small {I}}$, as a function of MDM. The mean $\mbox{$M^{\rm tot}_{\rm H\, \small {I}}$}$–$\mbox{$M_{\rm DM}$}$ relation is an increasing monotonic function. The galaxy spatial clustering increases weakly as the $M_{\rm H\, \small {I}}$ threshold increases. Our H i mock galaxies cluster more in comparison to the blind H i ALFALFA (Arecibo Fast Legacy ALFA) survey but we show that it is mainly due to the selection effects. We discuss the implications of our results in the light of predictions from semi-analytical models and hydrodynamics simulations of galaxy evolution.

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Kolesnichenko, I. I., V. A. Namiot, and L. M. Balashova. "Express Screening of Tear Fluid for Evaluation of the Concentration of Lanomax Using Multisensory Stripping Voltammetry and Multivariate Statistics." EPJ Web of Conferences 224 (2019): 03002. http://dx.doi.org/10.1051/epjconf/201922403002.

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The drug concentrations monitoring is very important for finding the right dosage. The developed method is based on the recognition of multidimensional images, which are produced by multisensory electrochemical systems that provide reliable information on objects being tested, using multidimensional statistics. The measurements were carried out using a planar solid-state electrode. The test solution was a 0.05 M KCl solution, which contained the $ {\rm{Z}}{{\rm{n}}_2}^ + ,{\rm{C}}{{\rm{d}}_2}^ + ,{\rm{P}}{{\rm{b}}_2}^ + ,{\rm{C}}{{\rm{o}}_2}^ + $ and $ {\rm{H}}{{\rm{g}}_2}^ + $ metal cations in the concentration of 5 • 10−5 M. The efficiency of this method in determining lanosterol with accounting for changes in its concentration with over time has been demonstrated. In order to determine concentrations of Lanomax in tear fluid, a procedure for multisensory stripping voltammetry has been developed and tested. It has been shown that the effect of lacrimal fluid on metal dissolution currents in the test system lasts 12 hours after the Lanomax instillation.

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Chang, S. J., K. H. Lee, P. C. Chang, Y. C. Wang, C. L. Yu, C. H. Kuo, and S. L. Wu. "GaN-Based Schottky Barrier Photodetectors With a 12-Pair Mg$_{\rm x}$N$_{\rm y}$–GaN Buffer Layer." IEEE Journal of Quantum Electronics 44, no. 10 (October 2008): 916–21. http://dx.doi.org/10.1109/jqe.2008.2000916.

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QIN, XIAO-FANG, HAI-SHUN WU, and HAIJUN JIAO. "STRUCTURE AND STABILITY OF HYDROGEN POOR CLOSO-${\rm B}_{n}{\rm H}_{n-x}^{-/0/+}$ (n = 5 - 12)." Journal of Theoretical and Computational Chemistry 07, no. 04 (August 2008): 531–39. http://dx.doi.org/10.1142/s0219633608003940.

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Structures and stabilities of hydrogen poor closo-[Formula: see text], closo- B n H n-2, and closo-[Formula: see text] (n = 5 - 12) have been investigated at the B3LYP/6-311+G** density functional level of theory. It is found that [Formula: see text], B 5 H 3, [Formula: see text], and [Formula: see text] have open instead of the expected closo structures, and the other isomers have the same structural pattern as closo-[Formula: see text]. Energetic analysis identifies closo-[Formula: see text] (n = 7, 9), closo- B n H n-2 (n = 7, 11), and closo-[Formula: see text] (n = 6, 8, 10) as the most stable clusters. The CO affinities of the most stable closo- B n H n-1 CO -, closo- B n H n-2( CO )2, and closo-[Formula: see text] (n = 5 - 12) have been computed.

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Piana, Olmo, Pratika Dayal, Marta Volonteri, and Tirthankar Roy Choudhury. "The mass assembly of high-redshift black holes." Monthly Notices of the Royal Astronomical Society 500, no. 2 (October 29, 2020): 2146–58. http://dx.doi.org/10.1093/mnras/staa3363.

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ABSTRACT We use the Delphi semi-analytic model to study the mass assembly and properties of high-redshift (z > 4) black holes over a wide mass range, $10^3 \lt M_{\rm bh}/{\rm \rm M_\odot }\lt 10^{10}$. Our black hole growth implementation includes a critical halo mass ($M_{\mathrm{ h}}^{\mathrm{ crit}}$) below which the black hole is starved and above which it is allowed to grow either at the Eddington limit or proportionally to the gas content of the galaxy. As a consequence, after an initial growth phase dominated by black hole mergers down to z ∼ 7 (9), supermassive black holes in z = 4 halo masses of $M_\mathrm{ h}|_{z=4} \sim 10^{11.75} \, (10^{13.4}) \, {\rm \rm M_\odot }$ mainly grow by gas accretion from the interstellar medium. In particular, we find that (i) while most of the accretion occurs in the major branch for $M_\mathrm{ h}|_{z=4} \sim 10^{11\!-\!12} \, {\rm \rm M_\odot }$ haloes, accretion in secondary branches plays a significant role in assembling the black hole mass in higher mass haloes ($M_\mathrm{ h}|_{z=4} \gtrsim 10^{12} \, {\rm \rm M_\odot }$); (ii) while the Eddington ratio increases with decreasing redshift for low-mass ($M_{\mathrm{ bh}} \lt 10^5 \, {\rm \rm M_\odot }$) black holes, it shows the opposite trend for larger masses. In addition, since the accretion rate depends on the gas mass present in the host halo, the duty cycle of the Eddington-limited accretion phase – which can last up to ≈650 Myr – is crucially linked to the joint assembly history of the black hole and its host halo.

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Faigenbaum, Avery D., Laurie Milliken, Lucas Moulton, and Wayne L. Westcott. "Early Muscular Fitness Adaptations in Children in Response to Two Different Resistance Training Regimens." Pediatric Exercise Science 17, no. 3 (August 2005): 237–48. http://dx.doi.org/10.1123/pes.17.3.237.

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The purpose of this study was to compare early muscular fitness adaptations in children in response to low repetition maximum (LRM) and high repetition maximum (HRM) resistance training. Twenty-three girls and 20 boys between the ages of 8.0 and 12.3 years (mean age 10.6 ± 1.3 years) volunteered to participate in this study. Children performed one set of 6 to 10 RM (n = 12) or one set of 15 to 20 RM (n = 19) on child-size exercise machines twice weekly over 8 weeks. Children in the control group (n = 12) did not resistance train. Maximum strength (1 RM) on the chest press, local muscular endurance (15 RM) on the leg press, long jump, vertical jump, and v-sit flexibility were assessed at baseline and posttraining. The LRM and HRM groups made significantly greater gains in 1-RM strength (21% and 23%, respectively) as compared with the control group (1%). Only the HRM group made significantly greater gains in 15-RM local muscular endurance (42%) and flexibility (15%) than that recorded in the control group (4% and 5%, respectively). If children perform one set per exercise as part of an introductory resistance training program, these findings favor the prescription of a higher RM training range.

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Stern, Jonathan, Drummond Fielding, Claude-André Faucher-Giguère, and Eliot Quataert. "The maximum accretion rate of hot gas in dark matter haloes." Monthly Notices of the Royal Astronomical Society 492, no. 4 (January 28, 2020): 6042–58. http://dx.doi.org/10.1093/mnras/staa198.

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ABSTRACT We revisit the question of ‘hot mode’ versus ‘cold mode’ accretion on to galaxies using steady-state cooling flow solutions and idealized 3D hydrodynamic simulations. We demonstrate that for the hot accretion mode to exist, the cooling time is required to be longer than the free-fall time near the radius where the gas is rotationally supported, Rcirc, i.e. the existence of the hot mode depends on physical conditions at the galaxy scale rather than on physical conditions at the halo scale. When allowing for the depletion of the halo baryon fraction relative to the cosmic mean, the longer cooling times imply that a virialized gaseous halo may form in halo masses below the threshold of $\sim 10^{12}\, {\rm M_{\odot }}$ derived for baryon-complete haloes. We show that for any halo mass there is a maximum accretion rate for which the gas is virialized throughout the halo and can accrete via the hot mode of ${\dot{M}}_{\rm crit}\approx 0.7(v_{\rm c}/100\, \rm km\ s^{-1})^{5.4}(R_{\rm circ}/10\, {\rm kpc})(Z/\, {\rm Z_{\odot }})^{-0.9}\, {\rm M_{\odot }}\, {\rm yr}^{-1}$, where Z and vc are the metallicity and circular velocity measured at Rcirc. For accretion rates $\gtrsim {\dot{M}}_{\rm crit}$ the volume-filling gas phase can in principle be ‘transonic’ – virialized in the outer halo but cool and free-falling near the galaxy. We compare ${\dot{M}}_{\rm crit}$ to the average star formation rate (SFR) in haloes at 0 < z < 10 implied by the stellar-mass–halo-mass relation. For a plausible metallicity evolution with redshift, we find that ${\rm SFR}\lesssim {\dot{M}}_{\rm crit}$ at most masses and redshifts, suggesting that the SFR of galaxies could be primarily sustained by the hot mode in halo masses well below the classic threshold of $\sim 10^{12}\, {\rm M_{\odot }}$.

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Richings, Alexander J., Claude-André Faucher-Giguère, and Jonathan Stern. "Unravelling the physics of multiphase AGN winds through emission line tracers." Monthly Notices of the Royal Astronomical Society 503, no. 2 (February 27, 2021): 1568–85. http://dx.doi.org/10.1093/mnras/stab556.

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ABSTRACT Observations of emission lines in active galactic nuclei (AGNs) often find fast (∼1000 km s−1) outflows extending to kiloparsec scales, seen in ionized, neutral atomic and molecular gas. In this work we present radiative transfer calculations of emission lines in hydrodynamic simulations of AGN outflows driven by a hot wind bubble, including non-equilibrium chemistry, to explore how these lines trace the physical properties of the multiphase outflow. We find that the hot bubble compresses the line-emitting gas, resulting in higher pressures than in the ambient interstellar medium or that would be produced by the AGN radiation pressure. This implies that observed emission line ratios such as [O iv]$_{25 \, \rm {\mu m}}$ / [Ne ii]$_{12 \, \rm {\mu m}}$, [Ne v]$_{14 \, \rm {\mu m}}$ / [Ne ii]$_{12 \, \rm {\mu m}}$, and [N iii]$_{57 \, \rm {\mu m}}$ / [N ii]$_{122 \, \rm {\mu m}}$ constrain the presence of the bubble and hence the outflow driving mechanism. However, the line-emitting gas is under-pressurized compared to the hot bubble itself, and much of the line emission arises from gas that is out of pressure, thermal and/or chemical equilibrium. Our results thus suggest that assuming equilibrium conditions, as commonly done in AGN line emission models, is not justified if a hot wind bubble is present. We also find that ≳50 per cent of the mass outflow rate, momentum flux, and kinetic energy flux of the outflow are traced by lines such as [N ii]$_{122 \, \rm {\mu m}}$ and [Ne iii]$_{15 \, \rm {\mu m}}$ (produced in the 10$^{4} \, \rm {K}$ phase) and [C ii]$_{158 \, \rm {\mu m}}$ (produced in the transition from 10$^{4} \, \rm {K}$ to 100 K).

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Kaduk, J. A., P. J. Cahill, and L. N. Venkateshwaran. "Crystal structures of a solvated and unsolvated sulfone cyclic oligomer." Journal of Applied Crystallography 32, no. 1 (February 1, 1999): 15–20. http://dx.doi.org/10.1107/s0021889898006189.

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The structure of the DMSO (dimethyl sulfoxide) solvate of the macrocyclic [2+2] dimer, 17,17,37,37-tetramethyl-2,12,22,32-tetraoxa-7,27-dithianonacyclo[36.2.2.2^{3,6}.-2^{8,11}.2^{13,16} .2^{18,21} .2^{23,26} .2^{28,31} .2^{33,36} ]hexapentaconta-3,5,8,-10,13,15,18,20,23,25,28,30,33,35,38,40,41,43,45,47,49,51,53,55-tetracosaene 7,7,27,27-tetraoxide, formed from 4,\!4'-dichlorodiphenyl sulfone and bisphenol-A has been determined by single-crystal techniques and the structure of the unsolvated dimer refined using X-ray powder diffraction data. The molecular conformations are similar and phenyl–phenyl stacking interactions are apparently important in determining the molecular conformation in the solid state. {\rm C_{54}H_{44}O_8S_2} .{\rm C_2H_6OS} (1)cyclo-[p\hbox{-}{\rm C_6H_4)SO_2(}p\hbox{-}{\rm C_6H_4)O(}p{\rm \hbox{-}C_6H_4){\rm C(CH_3)_2(}p{\rm \hbox{-} {\rm C_6H_4)O]_2}.{\rm C_2H_6OS}: molecular weight 963.2, monoclinic, P2_1/c,a=9.702 (2), b=18.623 (3), c=13.676 (2) Å, \beta =91.18 (1)^\circ , V=2470.5 (7) Å^3,Z=2 .{\rm C_{54}H_{44}O_8S_2} (2),cyclo-[(p{\rm \hbox{-} C_6H_4)SO_2(}p{\rm \hbox{-} {\rm C_6H_4)O(}p{\rm \hbox{-} C_6H_4)C(CH_3)_2(}p{\rm \hbox{-} {\rm C_6H_4)O]_2} : molecular weight 885.06, monoclinic, P2_1/c , a=9.5703 (15), b=18.7582 (18), c=13.3945 (12) Å, \beta =92.684 (11)^\circ , V=2402.0 (5) Å^3,Z=2 .

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