Search

Your search keyword '"Sullivan C."' showing total 3,442 results
Start Over Author "Sullivan C."
3,442 results on '"Sullivan C."'

4. BISOU: a balloon project to measure the CMB spectral distortions

Author

Maffei, B., Abitbol, M. H., Aghanim, N., Aumont, J., Battistelli, E., Chluba, J., Coulon, X., De Bernardis, P., Douspis, M., Grain, J., Gervasoni, S., Hill, J. C., Kogut, A., Masi, S., Matsumura, T., Sullivan, C. O, Pagano, L., Pisano, G., Remazeilles, M., Ritacco, A., Rotti, A., Sauvage, V., Savini, G., Stever, S. L., Tartari, A., Thiele, L., and Trappe, N.

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

The BISOU (Balloon Interferometer for Spectral Observations of the Universe) project aims to study the viability and prospects of a balloon-borne spectrometer, pathfinder of a future space mission dedicated to the measurements of the CMB spectral distortions. We present here a preliminary concept based on previous space mission proposals, together with some sensitivity calculation results for the observation goals, showing that a 5-sigma measurement of the y-distortions is achievable., Comment: 12 pages. To be published on the proceedings of the 16th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories (MG16) - 5-9 July 2021. Online Conference, Italy. http://www.icra.it/mg/mg16/

Published
2021

5. QUBIC IV: Performance of TES Bolometers and Readout Electronics

Author

Piat, M., Stankowiak, G., Battistelli, E. S., de Bernardis, P., Alessandro, G. D, De Petris, M., Grandsire, L., Hamilton, J. -Ch., Hoang, T. D., Marnieros, S., Masi, S., Mennella, A., Mousset, L., Sullivan, C. O, Prele, D., Tartari, A., Thermeau, J. -P., Torchinsky, S. A., Voisin, F., Zannoni, M., Ade, P., Alberro, J. G., Almela, A., Amico, G., Arnaldi, L. H., Auguste, D., Aumont, J., Azzoni, S., Banfi, S., Belier, B., Bau, A., Bennett, D., Berge, L., Bernard, J. -Ph., Bersanelli, M., Bigot-Sazy, M. -A., Bonaparte, J., Bonis, J., Bunn, E., Burke, D., Buzi, D., Cavaliere, F., Chanial, P., Chapron, C., Charlassier, R., Cerutti, A. C. Cobos, Columbro, F., Coppolecchia, A., De Gasperis, G., De Leo, M., Dheilly, S., Duca, C., Dumoulin, L., Etchegoyen, A., Fasciszewski, A., Ferreyro, L. P., Fracchia, D., Franceschet, C., Lerena, M. M. Gamboa, Ganga, K. M., Garcia, B., Redondo, M. E. Garcia, Gaspard, M., Gayer, D., Gervasi, M., Giard, M., Gilles, V., Giraud-Heraud, Y., Berisson, M. Gomez, Gonzalez, M., Gradziel, M., Hampel, M. R., Harari, D., Henrot-Versille, S., Incardona, F., Jules, E., Kaplan, J., Kristukat, C., Lamagna, L., Loucatos, S., Louis, T., Maffei, B., Marty, W., Mattei, A., May, A., McCulloch, M., Mele, L., Melo, D., Montier, L., Mundo, L. M., Murphy, J. A., Murphy, J. D., Nati, F., Olivieri, E., Oriol, C., Paiella, A., Pajot, F., Passerini, A., Pastoriza, H., Pelosi, A., Perbost, C., Perciballi, M., Pezzotta, F., Piacentini, F., Piccirillo, L., Pisano, G., Platino, M., Polenta, G., Puddu, R., Rambaud, D., Rasztocky, E., Ringegni, P., Romero, G. E., Salum, J. M., Schillaci, A., Scoccola, C. G., Scully, S., Spinelli, S., Stolpovskiy, M., Supanitsky, A. D., Timbie, P., Tomasi, M., Tucker, C., Tucker, G., Vigano, D., Vittorio, N., Wicek, F., Wright, M., and Zullo, A.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

A prototype version of the Q & U bolometric interferometer for cosmology (QUBIC) underwent a campaign of testing in the laboratory at Astroparticle Physics and Cosmology laboratory in Paris (APC). The detection chain is currently made of 256 NbSi transition edge sensors (TES) cooled to 320 mK. The readout system is a 128:1 time domain multiplexing scheme based on 128 SQUIDs cooled at 1 K that are controlled and amplified by an SiGe application specific integrated circuit at 40 K. We report the performance of this readout chain and the characterization of the TES. The readout system has been functionally tested and characterized in the lab and in QUBIC. The low noise amplifier demonstrated a white noise level of 0.3 nV.Hz^-0.5. Characterizations of the QUBIC detectors and readout electronics includes the measurement of I-V curves, time constant and the noise equivalent power. The QUBIC TES bolometer array has approximately 80% detectors within operational parameters. It demonstrated a thermal decoupling compatible with a phonon noise of about 5.10^-17 W.Hz^-0.5 at 410 mK critical temperature. While still limited by microphonics from the pulse tubes and noise aliasing from readout system, the instrument noise equivalent power is about 2.10^-16 W.Hz^-0.5, enough for the demonstration of bolometric interferometry., Comment: Accepted for publication in JCAP

Published
2021
Full Text
View/download PDF

6. Reexamination of $^{6}$Li scattering as a Probe to Investigate the Isoscalar Giant Resonances in Nuclei

Author

Zamora, J. C., Sullivan, C., Zegers, R. G. T., Aoi, N., Batail, L., Bazin, D., Carpenter, M., Carroll, J. J., Deloncle, I., Fang, Y. D., Fujita, H., Garg, U., Gey, G., Guess, C. J., Harakeh, M. N., Hoang, T. H., Hudson, E., Ichige, N., Ideguchi, E., Inoue, A., Isaak, J., Iwamoto, C., Kacir, C., Kobayashi, N., Koike, T., Raju, M. Kumar, Lipschutz, S., Liu, M., von Neumann-Cosel, P., Noji, S., Ong, H. J., Péru, S., Pereira, J., Schmitt, J., Tamii, A., Titus, R., Werner, V., Yamamoto, Y., Zhou, X., and Zhu, S.

Subjects
Nuclear Experiment, Nuclear Theory
Abstract

Inelastic ${}^{6}$Li scattering at 100 MeV/u on ${}^{12}$C and ${}^{93}$Nb have been measured with the high-resolution magnetic spectrometer Grand Raiden. The magnetic-rigidity settings of the spectrometer covered excitation energies from 10 to 40 MeV and scattering angles in the range $0^\circ < \theta_{\text{lab.}}< 2^\circ$. The isoscalar giant monopole resonance was selectively excited in the present data. Measurements free of instrumental background and the very favorable resonance-to-continuum ratio of ${}^{6}$Li scattering allowed for precise determination of the $E0$ strengths in ${}^{12}$C and ${}^{93}$Nb. It was found that the monopole strength in ${}^{12}$C exhausts $52 \pm 3^\text{(stat.)} \pm 8 ^\text{(sys.)}$\% of the energy-weighted sum rule (EWSR), which is considerably higher than results from previous $\alpha$-scattering experiments. The monopole strength in ${}^{93}$Nb exhausts $92 \pm 4^\text{(stat.)} \pm 10 ^\text{(sys.)}$\% of the EWSR, and it is consistent with measurements of nuclei with mass number of $A\approx90$. Such comparison indicates that the isoscalar giant monopole resonance distributions in these nuclei are very similar, and no influence due to nuclear structure was observed., Comment: 6 Figures

Published
2020
Full Text
View/download PDF

7. Constraints for stellar electron-capture rates on $^{86}$Kr via the $^{86}$Kr($t$,$^{3}$He$+\gamma$)$^{86}$Br reaction and the implications for core-collapse supernovae

Author

Titus, R., Ney, E. M., Zegers, R. G. T., Bazin, D., Belarge, J., Bender, P. C., Brown, B. A., Campbell, C. M., Elman, B., Engel, J., Gade, A., Gao, B., Kwan, E., Lipschutz, S., Longfellow, B., Lunderberg, E., Mijatovic, T., Noji, S., Pereira, J., Schmitt, J., Sullivan, C., Weisshaar, D., and Zamora, J. C.

Subjects
Nuclear Experiment, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, Nuclear Theory
Abstract

In the late stages of stellar core-collapse, prior to core bounce, electron captures on medium-heavy nuclei drive deleptonization and simulations require the use of accurate reaction rates. Nuclei with neutron number near $N=50$, just above atomic number $Z=28$, play an important role, but rates used in astrophysical simulations rely primarily on a relatively simple single-state approximation. In order to improve the accuracy of astrophysical simulations, experimental data are needed to test the electron-capture rates and to guide the development of better theoretical models. This work presents the results of the $^{86}$Kr($t$,$^{3}$He+$\gamma$) experiment at the NSCL, from which an upper limit for the Gamow-Teller strength up to an excitation energy in $^{86}$Br of 5 MeV is extracted. The derived upper limit for the electron-capture rate on $^{86}$Kr indicates that the rate estimated through the single-state approximation is too high and that rates based on Gamow-Teller strengths estimated in shell-model and QRPA calculations are more accurate. The QRPA calculations tested in this manner were used for estimating the electron capture rates for 78 isotopes near $N=50$ and above $Z=28$. The impact of using these new electron-capture rates in simulations of supernovae instead of the rates based on the single-state approximation is investigated, indicating a significant reduction in the deleptonization that affects multi-messenger signals, such as the emission of neutrinos and gravitational waves., Comment: 15 pages, 10 figures

Published
2019
Full Text
View/download PDF

8. Single-particle shell strengths near the doubly magic nucleus $^{56}$Ni and the $^{56}$Ni(p,$\gamma$)$^{57}$Cu reaction rate in explosive astrophysical burning

Author

Kahl, D., Woods, P. J., Poxon-Pearson, T., Nunes, F. M., Brown, B. A., Schatz, H., Baumann, T., Bazin, D., Belarge, J. A., Bender, P. C., Elman, B., Estrade, A., Gade, A., Kankainen, A., Lederer-Woods, C., Lipschutz, S., Longfellow, B., Lonsdale, S. -J., Lunderberg, E., Montes, F., Ong, W. J., Perdikakis, G., Pereira, J., Sullivan, C., Taverner, R., Weisshaar, D., and Zegers, R.

Subjects
Nuclear Experiment, Astrophysics - Solar and Stellar Astrophysics, Nuclear Theory
Abstract

Angle-integrated cross-section measurements of the $^{56}$Ni(d,n) and (d,p) stripping reactions have been performed to determine the single-particle strengths of low-lying excited states in the mirror nuclei pair $^{57}$Cu-$^{57}$Ni situated adjacent to the doubly magic nucleus $^{56}$Ni. The reactions were studied in inverse kinematics utilizing a beam of radioactive $^{56}$Ni ions in conjunction with the GRETINA $\gamma$-array. Spectroscopic factors are compared with new shell-model calculations using a full $pf$ model space with the GPFX1A Hamiltonian for the isospin-conserving strong interaction plus Coulomb and charge-dependent Hamiltonians. These results were used to set new constraints on the $^{56}$Ni(p,$\gamma$)$^{57}$Cu reaction rate for explosive burning conditions in x-ray bursts, where $^{56}$Ni represents a key waiting point in the astrophysical rp-process., Comment: Final version accepted and published. 5 pages, 2 figures

Published
2019
Full Text
View/download PDF

9. Constraining the Neutron Star Compactness: Extraction of the $^{23}$Al($p,\gamma$) Reaction Rate for the $rp$-Process

Author

Wolf, C., Langer, C., Montes, F., Pereira, J., Ong, W. -J., Poxon-Pearson, T., Ahn, S., Ayoub, S., Baumann, T., Bazin, D., Bender, P. C., Brown, B. A., Browne, J., Crawford, H., Cyburt, R. H., Deleeuw, E., Elman, B., Fiebiger, S., Gade, A., Gastis, P., Lipschutz, S., Longfellow, B., Meisel, Z., Nunes, F. M., Perdikakis, G., Reifarth, R., Richter, W. A., Schatz, H., Schmidt, K., Schmitt, J., Sullivan, C., Titus, R., Weisshaar, D., Woods, P. J., Zamora, J. C., and Zegers, R. G. T.

Subjects
Nuclear Experiment, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics, Nuclear Theory
Abstract

The $^{23}$Al($p,\gamma$)$^{24}$Si reaction is among the most important reactions driving the energy generation in Type-I X-ray bursts. However, the present reaction-rate uncertainty limits constraints on neutron star properties that can be achieved with burst model-observation comparisons. Here, we present a novel technique for constraining this important reaction by combining the GRETINA array with the neutron detector LENDA coupled to the S800 spectrograph at the National Superconducting Cyclotron Laboratory. The $^{23}$Al($d,n$) reaction was used to populate the astrophysically important states in $^{24}$Si. This enables a measurement in complete kinematics for extracting all relevant inputs necessary to calculate the reaction rate. For the first time, a predicted close-lying doublet of a 2$_2^+$ and (4$_1^+$,0$_2^+$) state in $^{24}$Si was disentangled, finally resolving conflicting results from two previous measurements. Moreover, it was possible to extract spectroscopic factors using GRETINA and LENDA simultaneously. This new technique may be used to constrain other important reaction rates for various astrophysical scenarios.

Published
2019
Full Text
View/download PDF

10. Experimental Constraint on Stellar Electron-Capture Rates from the ${}^{88}\text{Sr}(t,{}^{3}\text{He}+\gamma){}^{88}\text{Rb}$ reaction at 115 MeV/u

Author

Zamora, J. C., Zegers, R. G. T., Austin, Sam M., Bazin, D., Brown, B. A., Bender, P. C., Crawford, H. L., Engel, J., Falduto, A., Gade, A., Gastis, P., Gao, B., Ginter, T., Guess, C. J., Lipschutz, S., Longfellow, B., Macchiavelli, A. O., Miki, K., Ney, E., Noji, S., Pereira, J., Schmitt, J., Sullivan, C., Titus, R., and Weisshaar, D.

Subjects
Nuclear Experiment, Astrophysics - Solar and Stellar Astrophysics
Abstract

The Gamow-Teller strength distribution from ${}^{88}$Sr was extracted from a $(t,{}^{3}\text{He}+\gamma)$ experiment at 115 MeV/$u$ to constrain estimates for the electron-capture rates on nuclei around $N=50$, between and including $^{78}$Ni and $^{88}$Sr, which are important for the late evolution of core-collapse supernovae. The observed strength below an excitation energy of 8 MeV was consistent with zero and below 10 MeV amounted to $0.1\pm0.05$. Except for a very-weak transition that could come from the 2.231-MeV $1^{+}$ state, no $\gamma$ lines that could be associated with the decay of known $1^{+}$ states were identified. The derived electron-capture rate from the measured strength distribution is more than an order of magnitude smaller than rates based on the single-state approximation presently used in astrophysical simulations for most nuclei near $N=50$. Rates based on shell-model and quasiparticle random-phase approximation calculations that account for Pauli blocking and core-polarization effects provide better estimates than the single-state approximation, although a relatively strong transition to the first $1^{+}$ state in $^{88}$Rb is not observed in the data. Pauli unblocking effects due to high stellar temperatures could partially counter the low electron-capture rates. The new data serves as a zero-temperature benchmark for constraining models used to estimate such effects.

Published
2019
Full Text
View/download PDF

11. Constraints for stellar electron-capture rates on Kr 86 via the Kr 86 (t, He 3 +γ) Br 86 reaction and the implications for core-collapse supernovae

Author

Titus, R, Ney, EM, Zegers, RGT, Bazin, D, Belarge, J, Bender, PC, Brown, BA, Campbell, CM, Elman, B, Engel, J, Gade, A, Gao, B, Kwan, E, Lipschutz, S, Longfellow, B, Lunderberg, E, Mijatović, T, Noji, S, Pereira, J, Schmitt, J, Sullivan, C, Weisshaar, D, and Zamora, JC

Subjects
nucl-ex, astro-ph.HE, astro-ph.SR, nucl-th
Abstract

Background: In the late stages of stellar core collapse just prior to core bounce, electron captures on medium-heavy nuclei drive deleptonization. Therefore, simulations require the use of accurate reaction rates. Nuclei with neutron number near N=50 above atomic number Z=28 play an important role. Rates presently used in astrophysical simulations rely primarily on a relatively simple single-state approximation. In order to improve the accuracy of the astrophysical simulations, experimental data are needed to test the electron-capture rates and to guide the development of better theoretical models and astrophysical simulations. Purpose: The purpose of the present work was to measure the Gamow-Teller transition strength from Kr86 to Br86, to derive the stellar electron-capture rates based on the extracted strengths, and to compare the derived rates with rates based on shell-model and quasiparticle random-phase approximation (QRPA) Gamow-Teller strengths calculations, as well as the single-state approximation. An additional purpose was to test the impact of using improved electron-capture rates on the late evolution of core-collapse supernovae. Method: The Gamow-Teller strengths from Kr86 were extracted from the Kr86(t,He3+γ) charge-exchange reaction at 115MeV/u. The electron-capture rates were calculated as a function of stellar density and temperature. Besides the case of Kr86, the electron-capture rates based on the QRPA calculations were calculated for 78 additional isotopes near N=50 above Z=28. The impact of using these rates instead of those based on the single-state approximation is studied in a spherically symmetrical simulation of core collapse just prior to bounce. Results: The derived electron-capture rates on Kr86 from the experimental Gamow-Teller strength distribution are much smaller than the rates estimated based on the single-state approximation. Rates based on Gamow-Teller strengths estimated in shell-model and QRPA calculations are more accurate. The core-collapse supernova simulation with electron-capture rates based on the QRPA calculations indicate a significant reduction in the deleptonization during the collapse phase. Conclusions: It is important to utilize microscopic theoretical models that are tested by experimental data to constrain and estimate Gamow-Teller strengths and derived electron-capture rates for nuclei near N=50 that are inputs for astrophysical simulations of core-collapse supernovae and their multimessenger signals, such as the emission of neutrinos and gravitational waves.

Published
2019

12. Constraints for stellar electron-capture rates on Kr86 via the Kr86(t,He3+γ)Br86 reaction and the implications for core-collapse supernovae

Author

Titus, R, Ney, EM, Zegers, RGT, Bazin, D, Belarge, J, Bender, PC, Brown, BA, Campbell, CM, Elman, B, Engel, J, Gade, A, Gao, B, Kwan, E, Lipschutz, S, Longfellow, B, Lunderberg, E, Mijatović, T, Noji, S, Pereira, J, Schmitt, J, Sullivan, C, Weisshaar, D, and Zamora, JC

Subjects
Nuclear and Plasma Physics, Synchrotrons and Accelerators, Physical Sciences, nucl-ex, astro-ph.HE, astro-ph.SR, nucl-th, Nuclear and plasma physics
Abstract

Background: In the late stages of stellar core collapse just prior to core bounce, electron captures on medium-heavy nuclei drive deleptonization. Therefore, simulations require the use of accurate reaction rates. Nuclei with neutron number near N=50 above atomic number Z=28 play an important role. Rates presently used in astrophysical simulations rely primarily on a relatively simple single-state approximation. In order to improve the accuracy of the astrophysical simulations, experimental data are needed to test the electron-capture rates and to guide the development of better theoretical models and astrophysical simulations. Purpose: The purpose of the present work was to measure the Gamow-Teller transition strength from Kr86 to Br86, to derive the stellar electron-capture rates based on the extracted strengths, and to compare the derived rates with rates based on shell-model and quasiparticle random-phase approximation (QRPA) Gamow-Teller strengths calculations, as well as the single-state approximation. An additional purpose was to test the impact of using improved electron-capture rates on the late evolution of core-collapse supernovae. Method: The Gamow-Teller strengths from Kr86 were extracted from the Kr86(t,He3+γ) charge-exchange reaction at 115MeV/u. The electron-capture rates were calculated as a function of stellar density and temperature. Besides the case of Kr86, the electron-capture rates based on the QRPA calculations were calculated for 78 additional isotopes near N=50 above Z=28. The impact of using these rates instead of those based on the single-state approximation is studied in a spherically symmetrical simulation of core collapse just prior to bounce. Results: The derived electron-capture rates on Kr86 from the experimental Gamow-Teller strength distribution are much smaller than the rates estimated based on the single-state approximation. Rates based on Gamow-Teller strengths estimated in shell-model and QRPA calculations are more accurate. The core-collapse supernova simulation with electron-capture rates based on the QRPA calculations indicate a significant reduction in the deleptonization during the collapse phase. Conclusions: It is important to utilize microscopic theoretical models that are tested by experimental data to constrain and estimate Gamow-Teller strengths and derived electron-capture rates for nuclei near N=50 that are inputs for astrophysical simulations of core-collapse supernovae and their multimessenger signals, such as the emission of neutrinos and gravitational waves.

Published
2019

15. Equation of State Effects on Gravitational Waves from Rotating Core Collapse

Author

Richers, S., Ott, C. D., Abdikamalov, E., O'Connor, E., and Sullivan, C.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Gravitational waves (GWs) generated by axisymmetric rotating collapse, bounce, and early postbounce phases of a galactic core-collapse supernova will be detectable by current-generation gravitational wave observatories. Since these GWs are emitted from the quadrupole-deformed nuclear-density core, they may encode information on the uncertain nuclear equation of state (EOS). We examine the effects of the nuclear EOS on GWs from rotating core collapse and carry out 1824 axisymmetric general-relativistic hydrodynamic simulations that cover a parameter space of 98 different rotation profiles and 18 different EOS. We show that the bounce GW signal is largely independent of the EOS and sensitive primarily to the ratio of rotational to gravitational energy, and at high rotation rates, to the degree of differential rotation. The GW frequency of postbounce core oscillations shows stronger EOS dependence that can be parameterized by the core's EOS-dependent dynamical frequency $\sqrt{G\bar{\rho}_c}$. We find that the ratio of the peak frequency to the dynamical frequency follows a universal trend that is obeyed by all EOS and rotation profiles and that indicates that the nature of the core oscillations changes when the rotation rate exceeds the dynamical frequency. We find that differences in the treatments of low-density nonuniform nuclear matter, of the transition from nonuniform to uniform nuclear matter, and in the description of nuclear matter up to around twice saturation density can mildly affect the GW signal. We find that approximations and uncertainties in electron capture rates can lead to variations in the GW signal that are of comparable magnitude to those due to different nuclear EOS. This emphasizes the need for reliable nuclear electron capture rates and for self-consistent multi-dimensional neutrino radiation-hydrodynamic simulations of rotating core collapse., Comment: Accepted to Phys. Rev. D., 29 pages, 18 figures. Key simulation results and gravitational waveforms are available at https://stellarcollapse.org/Richers_2017_RRCCSN_EOS

Published
2017
Full Text
View/download PDF

17. Sensitivity of stellar electron-capture rates to parent neutron number: A case study on a continuous chain of twenty Vanadium isotopes

Author

Hitt, G. W., Gupta, S., Zegers, R. G. T., Titus, R., Sullivan, C., Brown, B. A., Cole, A. L., and Shams, S.

Subjects
Nuclear Experiment, Astrophysics - Solar and Stellar Astrophysics, Nuclear Theory
Abstract

Gamow-Teller (GT) strength distributions (B(GT)) in electron-capture (EC) daughters stemming from the parent ground state are computed with the shell-model in the full pf-shell space, with quasi-particle random-phase approximation (QRPA) in the formalism of Krumlinde and M\"oller and with an Approximate Method (AM) for assigning an effective B(GT). These are compared to data available from decay and charge-exchange (CE) experiments across titanium isotopes in the pf-shell from A=43 to A=62, the largest set available for any chain of isotopes in the pf-shell. The present study is the first to examine B(GT) and the associated EC rates across a particular chain of isotopes with the purpose of examining rate sensitivities as neutron number increases. EC rates are also computed for a wide variety of stellar electron densities and temperatures providing concise estimates of the relative size of rate sensitivities for particular astrophysical scenarios. This work underscores the astrophysical motivation for CE experiments in inverse kinematics for nuclei away from stability at the luminosities of future Radioactive Ion Beam Facilities., Comment: 12 pages, 9 figures, submitted to Physical Review C

Published
2016

18. Observation of the Isovector Giant Monopole Resonance via the Si28(Be10,B*10[1.74 MeV]) Reaction at 100 AMeV

Author

Scott, M, Zegers, RGT, Almus, R, Austin, Sam M, Bazin, D, Brown, BA, Campbell, C, Gade, A, Bowry, M, Galès, S, Garg, U, Harakeh, MN, Kwan, E, Langer, C, Loelius, C, Lipschutz, S, Litvinova, E, Lunderberg, E, Morse, C, Noji, S, Perdikakis, G, Redpath, T, Robin, C, Sakai, H, Sasamoto, Y, Sasano, M, Sullivan, C, Tostevin, JA, Uesaka, T, and Weisshaar, D

Subjects
Mathematical Sciences, Physical Sciences, Engineering, General Physics
Abstract

The (^{10}Be,^{10}B^{*}[1.74  MeV]) charge-exchange reaction at 100  AMeV is presented as a new probe for isolating the isovector (ΔT=1) nonspin-transfer (ΔS=0) response of nuclei, with ^{28}Si being the first nucleus studied. By using a secondary ^{10}Be beam produced by fast fragmentation of ^{18}O nuclei at the NSCL Coupled Cyclotron Facility, applying the dispersion-matching technique with the S800 magnetic spectrometer to determine the excitation energy in ^{28}Al, and performing high-resolution γ-ray tracking with the Gamma-Ray Energy Tracking In-beam Nuclear Array (GRETINA) to identify the 1022-keV γ ray associated with the decay from the 1.74-MeV T=1 isobaric analog state in ^{10}B, a ΔS=0 excitation-energy spectrum in ^{28}Al was extracted. Monopole and dipole contributions were determined through a multipole-decomposition analysis, and the isovector giant dipole resonance and isovector giant monopole resonance (IVGMR) were identified. The results show that this probe is a powerful tool for studying the elusive IVGMR, which is of interest for performing stringent tests of modern density functional theories at high excitation energies and for constraining the bulk properties of nuclei and nuclear matter. The extracted distributions were compared with theoretical calculations based on the normal-modes formalism and the proton-neutron relativistic time-blocking approximation. Calculated cross sections based on these strengths underestimate the data by about a factor of 2, which likely indicates deficiencies in the reaction calculations based on the distorted wave Born approximation.

Published
2017

19. Observation of the Isovector Giant Monopole Resonance via the ^{28}Si(^{10}Be,^{10}B^{*}[1.74  MeV]) Reaction at 100  AMeV.

Author

Scott, M, Zegers, RGT, Almus, R, Austin, Sam M, Bazin, D, Brown, BA, Campbell, C, Gade, A, Bowry, M, Galès, S, Garg, U, Harakeh, MN, Kwan, E, Langer, C, Loelius, C, Lipschutz, S, Litvinova, E, Lunderberg, E, Morse, C, Noji, S, Perdikakis, G, Redpath, T, Robin, C, Sakai, H, Sasamoto, Y, Sasano, M, Sullivan, C, Tostevin, JA, Uesaka, T, and Weisshaar, D

Subjects
General Physics, Physical Sciences
Abstract

The (^{10}Be,^{10}B^{*}[1.74  MeV]) charge-exchange reaction at 100  AMeV is presented as a new probe for isolating the isovector (ΔT=1) nonspin-transfer (ΔS=0) response of nuclei, with ^{28}Si being the first nucleus studied. By using a secondary ^{10}Be beam produced by fast fragmentation of ^{18}O nuclei at the NSCL Coupled Cyclotron Facility, applying the dispersion-matching technique with the S800 magnetic spectrometer to determine the excitation energy in ^{28}Al, and performing high-resolution γ-ray tracking with the Gamma-Ray Energy Tracking In-beam Nuclear Array (GRETINA) to identify the 1022-keV γ ray associated with the decay from the 1.74-MeV T=1 isobaric analog state in ^{10}B, a ΔS=0 excitation-energy spectrum in ^{28}Al was extracted. Monopole and dipole contributions were determined through a multipole-decomposition analysis, and the isovector giant dipole resonance and isovector giant monopole resonance (IVGMR) were identified. The results show that this probe is a powerful tool for studying the elusive IVGMR, which is of interest for performing stringent tests of modern density functional theories at high excitation energies and for constraining the bulk properties of nuclei and nuclear matter. The extracted distributions were compared with theoretical calculations based on the normal-modes formalism and the proton-neutron relativistic time-blocking approximation. Calculated cross sections based on these strengths underestimate the data by about a factor of 2, which likely indicates deficiencies in the reaction calculations based on the distorted wave Born approximation.

Published
2017

20. The performance of the γ-ray tracking array GRETINA for γ-ray spectroscopy with fast beams of rare isotopes

Author

Weisshaar, D, Bazin, D, Bender, PC, Campbell, CM, Recchia, F, Bader, V, Baugher, T, Belarge, J, Carpenter, MP, Crawford, HL, Cromaz, M, Elman, B, Fallon, P, Forney, A, Gade, A, Harker, J, Kobayashi, N, Langer, C, Lauritsen, T, Lee, IY, Lemasson, A, Longfellow, B, Lunderberg, E, Macchiavelli, AO, Miki, K, Momiyama, S, Noji, S, Radford, DC, Scott, M, Sethi, J, Stroberg, SR, Sullivan, C, Titus, R, Wiens, A, Williams, S, Wimmer, K, and Zhu, S

Subjects
Nuclear and Plasma Physics, Synchrotrons and Accelerators, Physical Sciences, gamma-ray spectroscopy, Rare-isotope beams, GRETINA, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences, Nuclear & Particles Physics, Nuclear and plasma physics
Abstract

The γ-ray tracking array GRETINA was coupled to the S800 magnetic spectrometer for spectroscopy with fast beams of rare isotopes at the National Superconducting Cyclotron Laboratory on the campus of Michigan State University. We describe the technical details of this powerful setup and report on GRETINA's performance achieved with source and in-beam measurements. The γ-ray multiplicity encountered in experiments with fast beams is usually low, allowing for a simplified and efficient treatment of the data in the γ-ray analysis in terms of Doppler reconstruction and spectral quality. The results reported in this work were obtained from GRETINA consisting of 8 detector modules hosting four high-purity germanium crystals each. Currently, GRETINA consists of 10 detector modules.

Published
2017

21. Digital Data Acquisition For the Low Energy Neutron Detector Array (LENDA)

Author

Lipschutz, S., Zegers, R. G. T., Hill, J., Liddick, S. N., Noji, S., Prokop, C. J., Scott, M., Solt, M., Sullivan, C., and Tompkins, J.

Subjects
Physics - Instrumentation and Detectors, Nuclear Experiment
Abstract

A digital data acquisition system (DDAS) has been implemented for the Low Energy Neutron Detector Array (LENDA). LENDA is an array of 24 BC-408 plastic-scintillator bars designed to measure low-energy neutrons with kinetic energies in the range of 100 keV to 10 MeV from (p,n)-type charge-exchange reactions. Compared to the previous data acquisition (DAQ) system for LENDA, DDAS offers the possibility to lower the neutron detection threshold, increase the overall neutron-detection efficiency, decrease the dead time of the system, and allow for easy expansion of the array. The system utilized in this work was XIA's Digital Gamma Finder Pixie-16 250 MHz digitizers. A detector-limited timing resolution of 400 ps was achieved for a single LENDA bar. Using DDAS, the neutron detection threshold of the system was reduced compared to the previous analog system, now reaching below 100 keV. The new DAQ system was successfully used in a recent charge-exchange experiment using the $^{16}$C(p,n) reaction at the National Superconducting Cyclotron Laboratory (NSCL)., Comment: Typo fixed in Abstract

Published
2016
Full Text
View/download PDF

22. Population of 13Be in a Nucleon Exchange Reaction

Author

Marks, B. R., DeYoung, P. A., Smith, J. K., Baumann, T., Brown, J., Frank, N., Hinnefeld, J., Hoffman, M., Jones, M. D., Kohley, Z., Kuchera, A. N., Luther, B., Spyrou, A., Stephenson, S., Sullivan, C., Thoennessen, M., Viscariello, N., and Williams, S. J.

Subjects
Nuclear Experiment
Abstract

The neutron-unbound nucleus 13Be was populated with a nucleon-exchange reaction from a 71 MeV/u secondary 13B beam. The decay energy spectrum was reconstructed using invariant mass spectroscopy based on 12Be fragments in coincidence with neutrons. The data could be described with an s-wave resonance at E = 0.73(9) MeV with a width of Gamma = 1.98(34) MeV and a d-wave resonance at E = 2.56(13) MeV with a width of Gamma = 2.29(73) MeV. The observed spectral shape is consistent with previous one-proton removal reaction measurements from 14B., Comment: Published in Phys. Rev. C

Published
2015
Full Text
View/download PDF

24. You Better Be Glad I Love My Job!

Author

Mitchell, J. Keith, Sullivan, C. Michelle, Cole, Keith, and Harris, Ken

Subjects
DEVIANT behavior, ORGANIZATIONAL citizenship behavior, DEPENDENCY (Psychology), DEPENDENT variables, SAMPLE size (Statistics)
Abstract

Purpose - This paper investigates the effect of job satisfaction as it moderates the relationship between intent to turnover and role overload when deviant behavior is the dependent variable. Design/methodology/approach - A survey was used with a sample size of 171. Findings- Results show that despite prior research to the contrary, role overload is negatively associated with deviant behavior. Also, we confirmed that job satisfaction buffers role overload and intent to turnover. Practical implications - The findings offer important insights into the power of job satisfaction. When the employees are content with their role, they are willing to deal with conditions that are less than ideal. Originality - This study extends our understanding of the effect of job satisfaction in a negative environment. It also demonstrates the need to revisit the relationship between role overload and deviant behavior. [ABSTRACT FROM AUTHOR]

Published
2024
Full Text
View/download PDF

26. COVID-19 vaccines and adverse events of special interest: A multinational Global Vaccine Data Network (GVDN) cohort study of 99 million vaccinated individuals

Author

Faksova, K, Walsh, D, Jiang, Y, Griffin, J, Phillips, A, Gentile, A, Kwong, JC, Macartney, K, Naus, M, Grange, Z, Escolano, S, Sepulveda, G, Shetty, A, Pillsbury, A, Sullivan, C, Naveed, Z, Janjua, NZ, Giglio, N, Perala, J, Nasreen, S, Gidding, H, Hovi, P, Vo, T, Cui, F, Deng, L, Cullen, L, Artama, M, Lu, H, Clothier, HJ, Batty, K, Paynter, J, Petousis-Harris, H, Buttery, J, Black, S, Hviid, A, Faksova, K, Walsh, D, Jiang, Y, Griffin, J, Phillips, A, Gentile, A, Kwong, JC, Macartney, K, Naus, M, Grange, Z, Escolano, S, Sepulveda, G, Shetty, A, Pillsbury, A, Sullivan, C, Naveed, Z, Janjua, NZ, Giglio, N, Perala, J, Nasreen, S, Gidding, H, Hovi, P, Vo, T, Cui, F, Deng, L, Cullen, L, Artama, M, Lu, H, Clothier, HJ, Batty, K, Paynter, J, Petousis-Harris, H, Buttery, J, Black, S, and Hviid, A

Abstract

BACKGROUND: The Global COVID Vaccine Safety (GCoVS) Project, established in 2021 under the multinational Global Vaccine Data Network™ (GVDN®), facilitates comprehensive assessment of vaccine safety. This study aimed to evaluate the risk of adverse events of special interest (AESI) following COVID-19 vaccination from 10 sites across eight countries. METHODS: Using a common protocol, this observational cohort study compared observed with expected rates of 13 selected AESI across neurological, haematological, and cardiac outcomes. Expected rates were obtained by participating sites using pre-COVID-19 vaccination healthcare data stratified by age and sex. Observed rates were reported from the same healthcare datasets since COVID-19 vaccination program rollout. AESI occurring up to 42 days following vaccination with mRNA (BNT162b2 and mRNA-1273) and adenovirus-vector (ChAdOx1) vaccines were included in the primary analysis. Risks were assessed using observed versus expected (OE) ratios with 95 % confidence intervals. Prioritised potential safety signals were those with lower bound of the 95 % confidence interval (LBCI) greater than 1.5. RESULTS: Participants included 99,068,901 vaccinated individuals. In total, 183,559,462 doses of BNT162b2, 36,178,442 doses of mRNA-1273, and 23,093,399 doses of ChAdOx1 were administered across participating sites in the study period. Risk periods following homologous vaccination schedules contributed 23,168,335 person-years of follow-up. OE ratios with LBCI > 1.5 were observed for Guillain-Barré syndrome (2.49, 95 % CI: 2.15, 2.87) and cerebral venous sinus thrombosis (3.23, 95 % CI: 2.51, 4.09) following the first dose of ChAdOx1 vaccine. Acute disseminated encephalomyelitis showed an OE ratio of 3.78 (95 % CI: 1.52, 7.78) following the first dose of mRNA-1273 vaccine. The OE ratios for myocarditis and pericarditis following BNT162b2, mRNA-1273, and ChAdOx1 were significantly increased with LBCIs > 1.5. CONCLUSION: This multi-country a

Published
2024

27. It Is in Our DNA: Bringing Electronic Health Records and Genomic Data Together for Precision Medicine.

Author

Robertson, AJ, Mallett, AJ, Stark, Z, Sullivan, C, Robertson, AJ, Mallett, AJ, Stark, Z, and Sullivan, C

Abstract

Health care is at a turning point. We are shifting from protocolized medicine to precision medicine, and digital health systems are facilitating this shift. By providing clinicians with detailed information for each patient and analytic support for decision-making at the point of care, digital health technologies are enabling a new era of precision medicine. Genomic data also provide clinicians with information that can improve the accuracy and timeliness of diagnosis, optimize prescribing, and target risk reduction strategies, all of which are key elements for precision medicine. However, genomic data are predominantly seen as diagnostic information and are not routinely integrated into the clinical workflows of electronic medical records. The use of genomic data holds significant potential for precision medicine; however, as genomic data are fundamentally different from the information collected during routine practice, special considerations are needed to use this information in a digital health setting. This paper outlines the potential of genomic data integration with electronic records, and how these data can enable precision medicine.

Published
2024

28. COVID-19 vaccines and adverse events of special interest:A multinational Global Vaccine Data Network (GVDN) cohort study of 99 million vaccinated individuals

Author

Faksova, K., Walsh, D., Jiang, Y., Griffin, J., Phillips, A., Gentile, A., Kwong, J. C., Macartney, K., Naus, M., Grange, Z., Escolano, S., Sepulveda, G., Shetty, A., Pillsbury, A., Sullivan, C., Naveed, Z., Janjua, N. Z., Giglio, N., Perälä, J., Nasreen, S., Gidding, H., Hovi, P., Vo, T., Cui, F., Deng, L., Cullen, L., Artama, M., Weintraub, E., Lu, H., Clothier, H. J., Batty, K., Paynter, J., Petousis-Harris, H., Buttery, J., Black, S., Hviid, A., Faksova, K., Walsh, D., Jiang, Y., Griffin, J., Phillips, A., Gentile, A., Kwong, J. C., Macartney, K., Naus, M., Grange, Z., Escolano, S., Sepulveda, G., Shetty, A., Pillsbury, A., Sullivan, C., Naveed, Z., Janjua, N. Z., Giglio, N., Perälä, J., Nasreen, S., Gidding, H., Hovi, P., Vo, T., Cui, F., Deng, L., Cullen, L., Artama, M., Weintraub, E., Lu, H., Clothier, H. J., Batty, K., Paynter, J., Petousis-Harris, H., Buttery, J., Black, S., and Hviid, A.

Abstract

Background: The Global COVID Vaccine Safety (GCoVS) Project, established in 2021 under the multinational Global Vaccine Data Network™ (GVDN®), facilitates comprehensive assessment of vaccine safety. This study aimed to evaluate the risk of adverse events of special interest (AESI) following COVID-19 vaccination from 10 sites across eight countries. Methods: Using a common protocol, this observational cohort study compared observed with expected rates of 13 selected AESI across neurological, haematological, and cardiac outcomes. Expected rates were obtained by participating sites using pre-COVID-19 vaccination healthcare data stratified by age and sex. Observed rates were reported from the same healthcare datasets since COVID-19 vaccination program rollout. AESI occurring up to 42 days following vaccination with mRNA (BNT162b2 and mRNA-1273) and adenovirus-vector (ChAdOx1) vaccines were included in the primary analysis. Risks were assessed using observed versus expected (OE) ratios with 95 % confidence intervals. Prioritised potential safety signals were those with lower bound of the 95 % confidence interval (LBCI) greater than 1.5. Results: Participants included 99,068,901 vaccinated individuals. In total, 183,559,462 doses of BNT162b2, 36,178,442 doses of mRNA-1273, and 23,093,399 doses of ChAdOx1 were administered across participating sites in the study period. Risk periods following homologous vaccination schedules contributed 23,168,335 person-years of follow-up. OE ratios with LBCI > 1.5 were observed for Guillain-Barré syndrome (2.49, 95 % CI: 2.15, 2.87) and cerebral venous sinus thrombosis (3.23, 95 % CI: 2.51, 4.09) following the first dose of ChAdOx1 vaccine. Acute disseminated encephalomyelitis showed an OE ratio of 3.78 (95 % CI: 1.52, 7.78) following the first dose of mRNA-1273 vaccine. The OE ratios for myocarditis and pericarditis following BNT162b2, mRNA-1273, and ChAdOx1 were significantly increased with LBCIs > 1.5. Conclusion: This multi

Published
2024

29. Astrophysical weak-interaction rates for selected $A=20$ and $A=24$ nuclei

Author

Martínez-Pinedo, G., Lam, Y. H., Langanke, K., Zegers, R. G. T., and Sullivan, C.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Nuclear Experiment, Nuclear Theory
Abstract

We have evaluated the electron capture rates on $^{20}$Ne, $^{20}$F, $^{24}$Mg, $^{24}$Na and the $\beta$ decay rates for $^{20}$F and $^{24}$Na at temperature and density conditions relevant for the late-evolution stages of stars with $M=8$-12 M$_\odot$. The rates are based on recent experimental data and large-scale shell model calculations. We show that the electron capture rates on $^{20}$Ne, $^{24}$Mg and the $^{20}$F, $^{24}$Na $\beta$-decay rates are based on data in this astrophysical range, except for the capture rate on $^{20}$Ne, which we predict to have a dominating contribution from the second-forbidden transition between the $^{20}$Ne and $^{20}$F ground states in the density range $\log \rho Y_e (\mathrm{g~cm}^{-3}) = 9.3$-9.6. The dominance of a few individual transitions allows us to present the various rates by analytical expressions at the relevant astrophysical conditions. We also derive the screening corrections to the rates., Comment: 21 pages, 12 figures

Published
2014
Full Text
View/download PDF

31. The QUaD Galactic Plane Survey 1: Maps And Analysis of Diffuse Emission

Author

Culverhouse, T., Ade, P., Bock, J., Bowden, M., Brown, M. L., Cahill, G., Castro, P. G., Church, S., Friedman, R., Ganga, K., Gear, W. K., Gupta, S., Hinderks, J., Kovac, J., Lange, A. E., Leitch, E., Melhuish, S. J., Memari, Y., Murphy, J. A., Orlando, A., Schwarz, R., Sullivan, C. O', Piccirillo, L., Pryke, C., Rajguru, N., Rusholme, B., Taylor, A. N., Thompson, K. L., Turner, A. H., Wu, E. Y. S., and Zemcov, M.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We present a survey of ~800 square degrees of the galactic plane observed with the QUaD telescope. The primary product of the survey are maps of Stokes I, Q and U parameters at 100 and 150 GHz, with spatial resolution 5 and 3.5 arcminutes respectively. Two regions are covered, spanning approximately 245-295 and 315-5 degrees in galactic longitude l, and -4

Published
2010
Full Text
View/download PDF

32. Small Angular Scale Measurements of the CMB Temperature Power Spectrum from QUaD

Author

QUaD collaboration, Friedman, R. B., Ade, P., Bock, J., Bowden, M., Brown, M. L., Cahill, G., Castro, P. G., Church, S., Culverhouse, T., Ganga, K., Gear, W. K., Gupta, S., Hinderks, J., Kovac, J., Lange, A. E., Leitch, E., Melhuish, S. J., Memari, Y., Murphy, J. A., Orlando, A., Sullivan, C. O', Piccirillo, L., Pryke, C., Rajguru, N., Rusholme, B., Schwarz, R., Taylor, A. N., Thompson, K. L., Turner, A. H., Wu, E. Y. S., and Zemcov, M.

Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract

We present measurements of the cosmic microwave background (CMB) radiation temperature anisotropy in the multipole range 2000

Published
2009
Full Text
View/download PDF

34. Deletion 16p13.11 uncovers NDE1 mutations on the non-deleted homolog and extends the spectrum of severe microcephaly to include fetal brain disruption

Author

Sherr, Elliott, Paciorkowski, AR, Keppler-Noreuil, K, Robinson, L, Sullivan, C, Sajan, S, Christian, SL, Bukshpun, P, Gabriel, SB, Gleeson, JG, and Sherr, EH

Abstract

Deletions of 16p13.11 have been associated with a variety of phenotypes, and have also been found in normal individuals. We report on two unrelated patients with severe microcephaly, agenesis of the corpus callosum, scalp rugae, and a fetal brain disruptio

Published
2013

39. Time-Resolved Optical Observations of PSR 1509-58

Author

Shearer, A., Sullivan, C. M. M. O', Golden, A., Garcia, P. V. R., Redfern, M., Danks, A., and Cullum, M.

Subjects
Astrophysics
Abstract

Using time resolved 2-dimensional aperture photometry we have established that the optical candidate for PSR 1509-58 does not pulse. Our pulsed upper limits (m_V = 24.3 and m_B = 25.7) put severe constraints on this being the optical counterpart. Furthermore the colours of the candidate star are consistent with a main sequence star at a distance of 2-4 kpc. The probability of a chance coincidence with a normal star and the difficulty of explaining the lack of pulsed emission leads us to conclude that this object is an intermediate field star., Comment: 4 pages, 2 figures

Published
1998

41. The performance of the γ-ray tracking array GRETINA for γ-ray spectroscopy with fast beams of rare isotopes

Author

Weisshaar, D., Bazin, D., Bender, P.C., Campbell, C.M., Recchia, F., Bader, V., Baugher, T., Belarge, J., Carpenter, M.P., Crawford, H.L., Cromaz, M., Elman, B., Fallon, P., Forney, A., Gade, A., Harker, J., Kobayashi, N., Langer, C., Lauritsen, T., Lee, I.Y., Lemasson, A., Longfellow, B., Lunderberg, E., Macchiavelli, A.O., Miki, K., Momiyama, S., Noji, S., Radford, D.C., Scott, M., Sethi, J., Stroberg, S.R., Sullivan, C., Titus, R., Wiens, A., Williams, S., Wimmer, K., and Zhu, S.

Published
2017
Full Text
View/download PDF

46. High- K three-quasiparticle isomers in the proton-rich nucleus Nd129

Author

Petrache, C. M., primary, Uusitalo, J., additional, Briscoe, A. D., additional, Sullivan, C. M., additional, Joss, D. T., additional, Tann, H., additional, Aktas, Ö., additional, Alayed, B., additional, Al-Aqeel, M. A. M., additional, Astier, A., additional, Badran, H., additional, Cederwall, B., additional, Delafosse, C., additional, Ertoprak, A., additional, Favier, Z., additional, Forsberg, U., additional, Gins, W., additional, Grahn, T., additional, Greenlees, P. T., additional, He, X. T., additional, Heery, J., additional, Hilton, J., additional, Kalantan, S., additional, Li, R., additional, Jodidar, P. M., additional, Julin, R., additional, Juutinen, S., additional, Leino, M., additional, Lewis, M. C., additional, Li, J. G., additional, Li, Z. P., additional, Luoma, M., additional, Lv, B. F., additional, McCarter, A., additional, Nathaniel, S., additional, Ojala, J., additional, Page, R. D., additional, Pakarinen, J., additional, Papadakis, P., additional, Parr, E., additional, Partanen, J., additional, Paul, E. S., additional, Rahkila, P., additional, Ruotsalainen, P., additional, Sandzelius, M., additional, Sarén, J., additional, Smallcombe, J., additional, Sorri, J., additional, Szwec, S., additional, Wang, L. J., additional, Wang, Y., additional, Waring, L., additional, Xu, F. R., additional, Zhang, J., additional, Zhang, Z. H., additional, Zheng, K. K., additional, and Zimba, G., additional

Published
2023
Full Text
View/download PDF

50. Global multi-stakeholder endorsement of the MAFLD definition

Author

Mendez-Sanchez, N, Bugianesi, E, Gish, R, Lammert, F, Tilg, H, Nguyen, M, Sarin, S, Fabrellas, N, Zelber-Sagi, S, Fan, J, Shiha, G, Targher, G, Zheng, M, Chan, W, Vinker, S, Kawaguchi, T, Castera, L, Yilmaz, Y, Korenjak, M, Spearman, C, Ungan, M, Palmer, M, El-Shabrawi, M, Gruss, H, Dufour, J, Dhawan, A, Wedemeyer, H, George, J, Valenti, L, Fouad, Y, Romero-Gomez, M, Eslam, M, Abate, M, Abbas, B, Abbassy, A, Abd El Ghany, W, Abd Elkhalek, A, Abd ElMajeed, E, Abdalgaber, M, Abdallah, M, Abdallah, N, Abdelaleem, S, Abdelghani, Y, Abdelghany, W, Abdelhalim, S, Abdelhamid, W, Abdelhamid, N, Abdelkader, N, Abdelkreem, E, Abdelmohsen, A, Abdelrahman, A, Abd-elsalam, S, Abdeltawab, D, Abduh, A, Abdulhakam, N, Abdulla, M, Abedpoor, N, Abenavoli, L, Aberg, F, Ablack, O, Abo elftouh, M, Abo-Amer, Y, Aboubkr, A, Aboud, A, Abouelnaga, A, Aboufarrag, G, Aboutaleb, A, Abundis, L, Adali, G, Adames, E, Adams, L, Adda, D, Adel, N, Adel Sayed, M, Afaa, T, Afredj, N, Aghayeva, G, Aghemo, A, Aguilar-Salinas, C, Ahlenstiel, G, Ahmady, W, Ahmed, W, Ahmed, A, Ahmed, S, Ahmed, H, Ahmed, R, Aigner, E, Akarsu, M, Akroush, M, Akyuz, U, Al Mahtab, M, Al Qadiri, T, Al Rawahi, Y, AL rubaee, R, Al Saffar, M, Alam, S, Al-Ani, Z, Albillos, A, Alboraie, M, Al-Busafi, S, Al-Emam, M, Alharthi, J, Ali, K, Ali, B, Ali, M, Ali, R, Alisi, A, AL-Khafaji, A, Alkhatry, M, Aller, R, Almansoury, Y, Al-Naamani, K, Alnakeeb, A, Alonso, A, Alqahtani, S, Alrabadi, L, Alswat, K, Altaher, M, Altamimi, T, Altamirano, J, Alvares-da-Silva, M, Aly, E, Alzahaby, A, Alzamzamy, A, Amano, K, Amer, M, Amin, M, Amin, S, Amir, A, Ampuero, J, Anas, N, Andreone, P, Andriamandimby, S, Anees, M, Angela, P, Antonios, M, Arafat, W, Araya, J, Armendariz-Borunda, J, Armstrong, M, Ashktorab, H, Aspichueta, P, Assal, F, Atef, M, Attia, D, Atwa, H, Awad, R, Awad, M, Awny, S, Awolowo, O, Awuku, Y, Ayada, I, Aye, T, Ayman, S, Ayman, H, Ayoub, H, Azmy, H, Babaran, R, Badreldin, O, Badry, A, Bahcecioglu, I, Bahour, A, Bai, J, Balaban, Y, Balasubramanyam, M, Bamakhrama, K, Banales, J, Bangaru, B, Bao, J, Barahona, J, Barakat, S, Barbalho, S, Barbra, B, Barranco, B, Barrera, F, Baumann, U, Bazeed, S, Bech, E, Benayad, A, Benesic, A, Bernstein, D, Bessone, F, Birney, S, Bisseye, C, Blake, M, Bobat, B, Bonfrate, L, Bordin, D, Bosques-Padilla, F, Boursier, J, Boushab, B, Bowen, D, Bravo, P, Brennan, P, Bright, B, Broekaert, I, Buque, X, Burgos-Santamaria, D, Burman, J, Busetto, L, Byrne, C, Cabral-Prodigalidad, P, Cabrera-Alvarez, G, Cai, W, Cainelli, F, Caliskan, A, Canbay, A, Cano-Contreras, A, Cao, H, Cao, Z, Carrion, A, Carubbi, F, Casanovas, T, Castellanos Fernandez, M, Chai, J, Chan, S, Charatcharoenwitthaya, P, Chavez-Tapia, N, Chayama, K, Chen, J, Chen, L, Chen, Z, Chen, H, Chen, S, Chen, Q, Chen, Y, Chen, G, Chen, E, Chen, F, Chen, P, Cheng, R, Cheng, W, Chieh, J, Chokr, I, Cholongitas, E, Choudhury, A, Chowdhury, A, Chukwudike, E, Ciardullo, S, Clayton, M, Clement, K, Cloa, M, Coccia, C, Collazos, C, Colombo, M, Cosar, A, Cotrim, H, Couillerot, J, Coulibaly, A, Crespo, G, Crespo, J, Cruells, M, Cua, I, Dabbous, H, Dalekos, G, D'Alia, P, Dan, L, Dao, V, Darwish, M, Datz, C, Davalos-Moscol, M, Dawoud, H, de Careaga, B, de Knegt, R, de Ledinghen, V, de Silva, J, Debzi, N, Decraecker, M, Del Pozo, E, Delgado, T, Delgado-Blanco, M, Dembinski, L, Depina, A, Derbala, M, Desalegn, H, Desbois-Mouthon, C, Desoky, M, Dev, A, Di Ciaula, A, Diago, M, Diallo, I, Diaz, L, Dirchwolf, M, Dongiovanni, P, Dorofeyev, A, Dou, X, Douglas, M, Doulberis, M, Dovia, C, Doyle, A, Dragojevic, I, Drenth, J, Duan, X, Dulskas, A, Dumitrascu, D, Duncan, O, Dusabejambo, V, Dwawhi, R, Eiketsu, S, El Amrousy, D, El Deeb, A, El Deriny, G, El Din, H, El Kamshishy, S, El Kassas, M, El Raziky, M, Elagamy, O, Elakel, W, Elalfy, D, Elaraby, H, Elawady, H, Elbadawy, R, Eldash, H, Eldefrawy, M, Elecharri, C, Elfaramawy, A, Elfatih, M, Elfiky, M, Elgamsy, M, Elgendy, M, El-Guindi, M, Elhussieny, N, Eliwa, A, Elkabbany, Z, El-Khayat, H, El-Koofy, N, Elmetwalli, A, Elrabat, A, El-Raey, F, Elrashdy, F, Elsahhar, M, Elsaid, E, Elsayed, S, Elsayed, H, Elsayed, A, El-Serafy, M, Elsharkawy, A, Elsheemy, R, Elshemy, E, Elsherbini, S, Eltoukhy, N, Elwakil, R, Emad, O, Emad, S, Embabi, M, Ergenc, I, Ermolova, T, Esmat, G, Esmat, D, Estupinan, E, Ettair, S, Eugen, T, Ezz-Eldin, M, Falcon, L, Fan, Y, Fandari, S, Farag, M, Farahat, T, Fares, E, Fares, M, Fassio, E, Fathy, H, Fathy, D, Fathy, W, Fayed, S, Feng, D, Feng, G, Fernandez-Bermejo, M, Ferreira, C, Ferrer, J, Forbes, A, Fouad, R, Fouad, H, Frisch, T, Fujii, H, Fukunaga, S, Fukunishi, S, Fulya, H, Furuhashi, M, Gaber, Y, Galang, A, Gallardo, J, Galloso, R, Gamal, M, Gamal, R, Gamal, H, Gan, J, Ganbold, A, Gao, X, Garas, G, Garba, T, Garcia-Cortes, M, Garcia-Monzon, C, Garcia-Samaniego, J, Gastaldelli, A, Gatica, M, Gatley, E, Gegeshidze, T, Geng, B, Ghazinyan, H, Ghoneem, S, Giacomelli, L, Giannelli, G, Giannini, E, Giefer, M, Gines, P, Girala, M, Giraudi, P, Goh, G, Gomaa, A, Gong, B, Gonzales, D, Gonzalez, H, Gonzalez-Huezo, M, Graupera, I, Grgurevic, I, Gronbaek, H, Gu, X, Guan, L, Gueye, I, Guingane, A, Gul, O, Gul, C, Guo, Q, Gupta, P, Gurakar, A, Gutierrez, J, Habib, G, Hafez, A, Hagman, E, Halawa, E, Hamdy, O, Hamed, A, Hamed, D, Hamid, S, Hamoudi, W, Han, Y, Haridy, J, Haridy, H, Harris, D, Hart, M, Hasan, F, Hashim, A, Hassan, I, Hassan, A, Hassan, E, Hassan, M, Hassanin, F, Hassnine, A, Haukeland, J, Hawal, A, He, J, He, Q, He, Y, He, F, Hegazy, M, Hegazy, A, Henegil, O, Hernandez, N, Hernandez-Guerra, M, Higuera-de-la-Tijera, F, Hindy, I, Hirota, K, Ho, L, Hodge, A, Hosny, M, Hou, X, Huang, J, Huang, Y, Huang, Z, Huang, A, Huang, X, Hui-ping, S, Hunyady, B, Hussein, M, Hussein, O, Hussien, S, Ibanez-Samaniego, L, Ibdah, J, Ibrahim, L, Ibrahim, M, Ibrahim, I, Icaza-Chavez, M, Idelbi, S, Idilman, R, Ikeda, M, Indolfi, G, Invernizzi, F, Irshad, I, Isa, H, Iskandar, N, Ismaiel, A, Ismail, M, Ismail, Z, Ismail, F, Iwamoto, H, Jack, K, Jacob, R, Jafarov, F, Jafri, W, Jahshan, H, Jalal, P, Jancoriene, L, Janicko, M, Jayasena, H, Jefferies, M, Jha, V, Ji, F, Ji, Y, Jia, J, Jiang, C, Jiang, N, Jiang, Z, Jin, X, Jin, Y, Jing, X, Jingyu, Q, Jinjolava, M, Jong, F, Jucov, A, Julius, I, Kaddah, M, Kamada, Y, Kamal, A, Kamal, E, Kamel, A, Kao, J, Karin, M, Karlas, T, Kashwaa, M, Katsidzira, L, Kaya, E, Kayasseh, M, Keenan, B, Keklikkiran, C, Keml, W, Khalaf, D, Khalefa, R, Khamis, S, Khater, D, Khattab, H, Khavkin, A, Khlynova, O, Khmis, N, Kobyliak, N, Koffas, A, Koike, K, Kok, K, Koller, T, Komas, N, Korochanskaya, N, Koulla, Y, Koya, S, Kraft, C, Kraja, B, Krawczyk, M, Kuchay, M, Kulkarni, A, Kumar, A, Kumar, M, Lakoh, S, Lam, P, Lan, L, Lange, N, Lankarani, K, Lanthier, N, Lapshyna, K, Lashen, S, Laure, K, Lazebnik, L, Lebrec, D, Lee, S, Lee, W, Lee, Y, Leeming, D, Leite, N, Leon, R, Lesmana, C, Li, J, Li, Q, Li, Y, Li, L, Li, M, Liang, H, Lijuan, T, Lim, S, Lim, L, Lin, S, Lin, H, Lin, R, Lithy, R, Liu, Y, Liu, X, Liu, W, Liu, S, Liu, K, Liu, T, Lonardo, A, Lopez, M, Lopez-Benages, E, Lopez-Jaramillo, P, Lu, H, Lu, L, Lu, Y, Lubel, J, Lui, R, Lupasco, I, Luzina, E, Lv, X, Lynch, K, Ma, H, Machado, M, Maduka, N, Madzharova, K, Magdaong, R, Mahadeva, S, Mahfouz, A, Mahmood, N, Mahmoud, E, Mahrous, M, Maiwall, R, Majeed, A, Majumdar, A, Mak, L, Maklouf, M, Malekzadeh, R, Mandato, C, Mangia, A, Mann, J, Mansour, H, Mansouri, A, Mantovani, A, Mao, J, Maramag, F, Marchesini, G, Marcus, C, Marinho, R, Martinez-Chantar, M, Martins, A, Marwan, R, Mason, K, Masoud, G, Massoud, M, Matamoros, M, Mateos, R, Mawed, A, Mbanya, J, Mbendi, C, Mccolaugh, L, Mcleod, D, Medina, J, Megahed, A, Mehrez, M, Memon, I, Merat, S, Mercado, R, Mesbah, A, Meskini, T, Metwally, M, Metwaly, R, Miao, L, Micah, E, Miele, L, Milivojevic, V, Milovanovic, T, Mina, Y, Mishkovik, M, Mishriki, A, Mitchell, T, Mohamed, A, Mohamed, M, Mohamed, S, Mohammed, S, Mohammed, A, Mohan, V, Mohie, S, Mokhtar, A, Moniem, R, Montilla, M, Morales, J, Morata, M, Moreno-Planas, J, Morise, S, Mosaad, S, Moselhy, M, Mostafa, A, Mostafa, E, Mouane, N, Mousa, N, Moustafa, H, Msherif, A, Muller, K, Munoz, C, Munoz-Urribarri, A, Murillo, O, Mustapha, F, Muzurovic, E, Nabil, Y, Nafady, S, Nagamatsu, A, Nakajima, A, Nakano, D, Nan, Y, Nascimbeni, F, Naseef, M, Nashat, N, Natalia, T, Negro, F, Nersesov, A, Neuman, M, Ng'Wanasayi, M, Ni, Y, Nicoll, A, Niizeki, T, Nikolova, D, Ningning, W, Niriella, M, Nogoibaeva, K, Nordien, R, O Sullivan, C, O'Beirne, J, Obekpa, S, Ocama, P, Ochwoto, M, Ogolodom, M, Ojo, O, Okrostsvaridze, N, Oliveira, C, Omana, R, Omar, O, Omar, H, Omar, M, Omran, S, Omran, R, Osman, M, Owise, N, Owusu-Ansah, T, Padilla- Machaca, P, Palle, S, Pan, Z, Pan, X, Pan, Q, Papaefthymiou, A, Paquissi, F, Par, G, Parkash, A, Payawal, D, Peltekian, K, Peng, X, Peng, L, Peng, Y, Pengoria, R, Perez, M, Perez, J, Perez, N, Persico, M, Pessoa, M, Petta, S, Philip, M, Plaz Torres, M, Polavarapu, N, Poniachik, J, Portincasa, P, Pu, C, Purnak, T, Purwanto, E, Qi, X, Qian, Z, Qiang, Z, Qiao, Z, Qiao, L, Queiroz, A, Rabiee, A, Radwan, M, Rahetilahy, A, Ramadan, Y, Ramadan, D, Ramli, A, Ramm, G, Ran, A, Rankovic, I, Rao, H, Raouf, S, Ray, S, Reau, N, Refaat, A, Reiberger, T, Remes-Troche, J, Reyes, E, Richardson, B, Ridruejo, E, Riestra Jimenez, S, Rizk, I, Roberts, S, Roblero, J, Robles, J, Rockey, D, Rodriguez, M, Rodriguez Hernandez, H, Roman, E, Romeiro, F, Romeo, S, Rosales-Zabal, J, Roshdi, G, Rosso, N, Ruf, A, Ruiz, P, Runes, N, Ruzzenente, A, Ryan, M, Saad, A, Sabbagh, E, Sabbah, M, Saber, S, Sabrey, R, Sabry, R, Saeed, M, Said, D, Said, E, Sakr, M, Salah, Y, Salama, R, Salama, A, Saleh, H, Saleh, A, Salem, A, Salifou, A, Salih, A, Salman, A, Samouda, H, Sanai, F, Sanchez-Avila, J, Sanker, L, Sano, T, Sanz, M, Saparbu, T, Sawhney, R, Sayed, F, Sayed, S, Sayed, A, Sayed, M, Sebastiani, G, Secadas, L, Sediqi, K, Seif, S, Semida, N, Senates, E, Serban, E, Serfaty, L, Seto, W, Sghaier, I, Sha, M, Shabaan, H, Shalaby, L, Shaltout, I, Sharara, A, Sharma, V, Shawa, I, Shawkat, A, Shawky, N, Shehata, O, Sheils, S, Shewaye, A, Shi, G, Shi, J, Shimose, S, Shirono, T, Shou, L, Shrestha, A, Shui, G, Sievert, W, Sigurdardottir, S, Sira, M, Siradj, R, Sison, C, Smyth, L, Soliman, R, Sollano, J, Sombie, R, Sonderup, M, Sood, S, Soriano, G, Stedman, C, Stefanyuk, O, Stimac, D, Strasser, S, Strnad, P, Stuart, K, Su, W, Su, M, Sumida, Y, Sumie, S, Sun, D, Sun, J, Suzuki, H, Svegliati-Baroni, G, Swar, M, Taharboucht, S, Taher, Z, Takamura, S, Tan, L, Tan, S, Tanwandee, T, Tarek, S, Tatiana, G, Tavaglione, F, Tecson, G, Tee, H, Teschke, R, Tharwat, M, Thong, V, Thursz, M, Tine, T, Tiribelli, C, Tolmane, I, Tong, J, Tongo, M, Torkie, M, Torre, A, Torres, E, Trajkovska, M, Treeprasertsuk, S, Tsutsumi, T, Tu, T, Tur, J, Turan, D, Turcan, S, Turkina, S, Tutar, E, Tzeuton, C, Ugiagbe, R, Uygun, A, Vacca, M, Vajro, P, Van der Poorten, D, Van Kleef, L, Vashakidze, E, Velazquez, C, Velazquez, M, Vento, S, Verhoeven, V, Vespasiani-Gentilucci, U, Vethakkan, S, Vilaseca, J, Vitek, L, Volkanovska, A, Wallace, M, Wan, W, Wang, Y, Wang, X, Wang, C, Wang, M, Wangchuk, P, Weltman, M, White, M, Wiegand, J, Wifi, M, Wigg, A, Wilhelmi, M, William, R, Wittenburg, H, Wu, S, Wubeneh, A, Xia, H, Xiao, J, Xiao, X, Xiaofeng, W, Xiong, W, Xu, L, Xu, J, Xu, W, Xu, K, Xu, Y, Xu, S, Xu, M, Xu, A, Xu, C, Yan, H, Yang, J, Yang, R, Yang, Y, Yang, Q, Yang, N, Yao, J, Yara, J, Yaras, S, Yilmaz, N, Younes, R, Younes, H, Young, S, Youssef, F, Yu, Y, Yu, M, Yuan, J, Yue, Z, Yuen, M, Yun, W, Yurukova, N, Zakaria, S, Zaky, S, Zaldastanishvili, M, Zapata, R, Zare, N, Zerem, E, Zeriban, N, Zeshuai, X, Zhang, H, Zhang, X, Zhang, Y, Zhang, W, Zhang, Z, Zhao, J, Zhao, R, Zhao, H, Zheng, C, Zheng, Y, Zheng, R, Zheng, T, Zheng, K, Zhou, X, Zhou, Y, Zhou, H, Zhou, L, Zhu, L, Zhu, Y, Zhu, P, Ziada, E, Ziring, D, Ziyi, L, Zou, S, Zou, Z, Zou, H, Zuart Ruiz, R, Mendez-Sanchez N., Bugianesi E., Gish R. G., Lammert F., Tilg H., Nguyen M. H., Sarin S. K., Fabrellas N., Zelber-Sagi S., Fan J. -G., Shiha G., Targher G., Zheng M. -H., Chan W. -K., Vinker S., Kawaguchi T., Castera L., Yilmaz Y., Korenjak M., Spearman C. W., Ungan M., Palmer M., El-Shabrawi M., Gruss H. -J., Dufour J. -F., Dhawan A., Wedemeyer H., George J., Valenti L., Fouad Y., Romero-Gomez M., Eslam M., Abate M. L., Abbas B., Abbassy A. A., Abd El Ghany W., Abd Elkhalek A., Abd ElMajeed E., Abdalgaber M., AbdAllah M., Abdallah M., Abdallah N., Abdelaleem S., Abdelghani Y., Abdelghany W., Abdelhalim S. M., Abdelhamid W., Abdelhamid N., Abdelkader N. A., Abdelkreem E., Abdelmohsen A. M., Abdelrahman A. A., Abd-elsalam S. M., Abdeltawab D., Abduh A., Abdulhakam N., Abdulla M., Abedpoor N., Abenavoli L., Aberg F., Ablack O., Abo elftouh M., Abo-Amer Y. E. -E., Aboubkr A., Aboud A., Abouelnaga A. M., Aboufarrag G. A., Aboutaleb A., Abundis L., Adali G., Adames E., Adams L., Adda D., Adel N., Adel Sayed M., Afaa T. J., Afredj N., Aghayeva G., Aghemo A., Aguilar-Salinas C. A., Ahlenstiel G., Ahmady W., Ahmed W., Ahmed A., Ahmed S. N., Ahmed H. M., Ahmed R., Aigner E., Akarsu M., Akroush M., Akyuz U., Al Mahtab M., Al Qadiri T., Al Rawahi Y., AL rubaee R., Al Saffar M., Alam S., Al-Ani Z., Albillos A., Alboraie M., Al-Busafi S., Al-Emam M., Alharthi J., Ali K., Ali B. A., Ali M., Ali R. A. R., Alisi A., AL-Khafaji A. R., Alkhatry M., Aller R., Almansoury Y., Al-Naamani K., Alnakeeb A., Alonso A., Alqahtani S. A., Alrabadi L., Alswat K., Altaher M., Altamimi T., Altamirano J., Alvares-da-Silva M. R., Aly E. A. M., Alzahaby A., Alzamzamy A., Amano K., Amer M. A., Amin M. A., Amin S. A., Amir A. A., Ampuero J., Anas N., Andreone P., Andriamandimby S. F., Anees M., Angela P., Antonios M., Arafat W., Araya J. M., Armendariz-Borunda J., Armstrong M. J., Ashktorab H., Aspichueta P., Assal F., Atef M., Attia D., Atwa H., Awad R., Awad M. A. E., Awny S., Awolowo O., Awuku Y. A., Ayada I., Aye T. T., Ayman S., Ayman H., Ayoub H., Azmy H. M., Babaran R. P., Badreldin O., Badry A., Bahcecioglu I. H., Bahour A., Bai J., Balaban Y., Balasubramanyam M., Bamakhrama K., Banales J. M., Bangaru B., Bao J., Barahona J. S., Barakat S., Barbalho S. M., Barbra B., Barranco B., Barrera F., Baumann U., Bazeed S., Bech E., Benayad A., Benesic A., Bernstein D., Bessone F., Birney S., Bisseye C., Blake M., Bobat B., Bonfrate L., Bordin D. S., Bosques-Padilla F., Boursier J., Boushab B. M., Bowen D., Bravo P. M., Brennan P. N., Bright B., Broekaert I., Buque X., Burgos-Santamaria D., Burman J., Busetto L., Byrne C. D., Cabral-Prodigalidad P. A. I., Cabrera-Alvarez G., Cai W., Cainelli F., Caliskan A. R., Canbay A., Cano-Contreras A., Cao H. -X., Cao Z., Carrion A., Carubbi F., Casanovas T., Castellanos Fernandez M. I., Chai J., Chan S. P., Charatcharoenwitthaya P., Chavez-Tapia N., Chayama K., Chen J., Chen L., Chen Z. -W., Chen H., Chen S. -D., Chen Q., Chen Y., Chen G., Chen E. -Q., Chen F., Chen P. -J., Cheng R., Cheng W., Chieh J. T. W., Chokr I., Cholongitas E., Choudhury A., Chowdhury A., Chukwudike E. S., Ciardullo S., Clayton M., Clement K., Cloa M. M., Coccia C., Collazos C., Colombo M., Cosar A. M., Cotrim H. P., Couillerot J., Coulibaly A., Crespo G., Crespo J., Cruells M., Cua I. H. Y., Dabbous H. K., Dalekos G. N., D'Alia P., Dan L., Dao V. H., Darwish M., Datz C., Davalos-Moscol M. B., Dawoud H., de Careaga B. O., de Knegt R., de Ledinghen V., de Silva J., Debzi N., Decraecker M., Del Pozo E., Delgado T. C., Delgado-Blanco M., Dembinski L., Depina A., Derbala M., Desalegn H., Desbois-Mouthon C., Desoky M., Dev A., Di Ciaula A., Diago M., Diallo I., Diaz L. A., Dirchwolf M., Dongiovanni P., Dorofeyev A., Dou X., Douglas M. W., Doulberis M., Dovia C. K., Doyle A., Dragojevic I., Drenth J. P., Duan X., Dulskas A., Dumitrascu D. L., Duncan O., Dusabejambo V., Dwawhi R. S. N. A., Eiketsu S., El Amrousy D., El Deeb A., El Deriny G., El Din H. S., El Kamshishy S., El Kassas M., El Raziky M., Elagamy O. A., Elakel W., Elalfy D., Elaraby H., ElAwady H., Elbadawy R., Eldash H. H., Eldefrawy M. S., Elecharri C. L., Elfaramawy A., Elfatih M., Elfiky M., Elgamsy M., Elgendy M., El-Guindi M. A., Elhussieny N., Eliwa A. M., Elkabbany Z., El-Khayat H., El-Koofy N. M., Elmetwalli A., Elrabat A., El-Raey F., Elrashdy F., Elsahhar M., Elsaid E. M., Elsayed S., Elsayed H., Elsayed A., Elsayed A. M., El-Serafy M., Elsharkawy A. M., Elsheemy R. Y., Elshemy E. E., Elsherbini S., Eltoukhy N., Elwakil R., Emad O., Emad S., Embabi M., Ergenc I., Ermolova T., Esmat G., Esmat D. M., Estupinan E. C., Ettair S., Eugen T., Ezz-Eldin M., Falcon L. P. V., Fan Y. -C., Fandari S., Farag M., Farahat T. M., Fares E. M., Fares M., Fassio E., Fathy H., Fathy D., Fathy W., Fayed S., Feng D., Feng G., Fernandez-Bermejo M., Ferreira C. T., Ferrer J. D., Forbes A., Fouad R., Fouad H. M., Frisch T., Fujii H., Fukunaga S., Fukunishi S., Fulya H., Furuhashi M., Gaber Y., Galang A. J. G., Gallardo J. C., Galloso R., Gamal M., Gamal R., Gamal H., Gan J., Ganbold A., Gao X., Garas G., Garba T., Garcia-Cortes M., Garcia-Monzon C., Garcia-Samaniego J., Gastaldelli A., Gatica M., Gatley E., Gegeshidze T., Geng B., Ghazinyan H., Ghoneem S., Giacomelli L., Giannelli G., Giannini E. G., Giefer M., Gines P., Girala M., Giraudi P. J., Goh G. B. -B., Gomaa A. A., Gong B., Gonzales D. H. C., Gonzalez H. C., Gonzalez-Huezo M. S., Graupera I., Grgurevic I., Gronbaek H., Gu X., Guan L., Gueye I., Guingane A. N., Gul O. O., Gul C. B., Guo Q., Gupta P. P., Gurakar A., Gutierrez J. C. R., Habib G., Hafez A., Hagman E., Halawa E., Hamdy O., Hamed A. E., Hamed D. H., Hamid S., Hamoudi W., Han Y., Haridy J., Haridy H., Harris D. C. H. H., Hart M., Hasan F., Hashim A., Hassan I., Hassan A., Hassan E. A., Hassan A. A., Hassan M. S., Hassanin F., Hassnine A., Haukeland J. W., Hawal A. I. M., He J., He Q., He Y., He F. -P., Hegazy M., Hegazy A., Henegil O., Hernandez N., Hernandez-Guerra M., Higuera-de-la-Tijera F., Hindy I., Hirota K., Ho L. C., Hodge A., Hosny M., Hou X., Huang J. -F., Huang Y., Huang Z., Huang A., Huang X. -P., Hui-ping S., Hunyady B., Hussein M. A., Hussein O., Hussien S. M., Ibanez-Samaniego L., Ibdah J., Ibrahim L., Ibrahim M., Ibrahim I., Icaza-Chavez M. E., Idelbi S., Idilman R. I., Ikeda M., Indolfi G., Invernizzi F., Irshad I., Isa H. M. A., Iskandar N. J., Ismaiel A., Ismail M., Ismail Z., Ismail F., Iwamoto H., Jack K., Jacob R., Jafarov F., Jafri W., Jahshan H., Jalal P. K., Jancoriene L., Janicko M., Jayasena H., Jefferies M., Jha V., Ji F., Ji Y., Jia J., Jiang C., Jiang N., Jiang Z. -Z., Jin X., Jin Y., Jing X., Jingyu Q., Jinjolava M., Jong F. H. H., Jucov A., Julius I., Kaddah M., Kamada Y., kamal A., Kamal E. M., Kamel A. S., Kao J. -H., Karin M., Karlas T., Kashwaa M., Katsidzira L., Kaya E., Kayasseh M. A., Keenan B., Keklikkiran C., Keml W., Khalaf D. K., Khalefa R., Khamis S., Khater D., khattab H., Khavkin A., Khlynova O., Khmis N., Kobyliak N., Koffas A., Koike K., Kok K. Y. Y., Koller T., Komas N. P., Korochanskaya N. V., Koulla Y., Koya S., Kraft C., Kraja B., Krawczyk M., Kuchay M. S., Kulkarni A. V., Kumar A., Kumar M., Lakoh S., Lam P., Lan L., Lange N. F., Lankarani K. B., Lanthier N., Lapshyna K., Lashen S. A., Laure K. N. J., Lazebnik L., Lebrec D., Lee S. S., Lee W. S., Lee Y. Y., Leeming D. J., Leite N. C., Leon R., Lesmana C. R. A., Li J., Li Q., Li Y. -Y., Li Y., Li L., Li M., li Y., Liang H., Lijuan T., Lim S. G., Lim L. -L., Lin S., Lin H. -C., Lin R., Lithy R., Liu Y., Liu X., Liu W. -Y., Liu S., Liu K., Liu T., Lonardo A., Lopez M. B., Lopez-Benages E., Lopez-Jaramillo P., Lu H., Lu L. G., Lu Y., Lubel J., Lui R., Lupasco I., Luzina E., Lv X. -H., Lynch K., Ma H. -L., Machado M. V., Maduka N., Madzharova K., Magdaong R., Mahadeva S., Mahfouz A., Mahmood N. R. K. N., Mahmoud E., Mahrous M., Maiwall R., Majeed A., Majumdar A., Mak L., Maklouf M. M., Malekzadeh R., Mandato C., Mangia A., Mann J., Mansour H. H., Mansouri A., Mantovani A., Mao J. Q., Maramag F., Marchesini G., Marcus C., Marinho R. A. R. T., Martinez-Chantar M. L., Martins A. A. S., Marwan R., Mason K. F., Masoud G., Massoud M. N., Matamoros M. A., Mateos R. M., Mawed A., Mbanya J. C., Mbendi C., McColaugh L., McLeod D., Medina J. F. R., Megahed A., Mehrez M., Memon I., Merat S., Mercado R., Mesbah A., Meskini T., Metwally M., Metwaly R., Miao L., Micah E., Miele L., Milivojevic V., Milovanovic T., Mina Y. L., Mishkovik M., Mishriki A., Mitchell T., Mohamed A., Mohamed M., Mohamed S., Mohammed S., Mohammed A., Mohan V., Mohie S., Mokhtar A., Moniem R., Montilla M. S., Morales J. A. O., Morata M. M. S., Moreno-Planas J. M., Morise S., Mosaad S., Moselhy M., Mostafa A. M., Mostafa E., Mouane N., Mousa N., Moustafa H. M., Msherif A., Muller K., Munoz C., Munoz-Urribarri A. B., Murillo O. A., Mustapha F. I., Muzurovic E., Nabil Y., Nafady S., Nagamatsu A., Nakajima A., Nakano D., Nan Y., Nascimbeni F., Naseef M. S., Nashat N., Natalia T., Negro F., Nersesov A. V., Neuman M., Ng'wanasayi M., Ni Y., Nicoll A., Niizeki T., Nikolova D., Ningning W., Niriella M., Nogoibaeva K. A., Nordien R., O Sullivan C., O'Beirne J., Obekpa S., Ocama P., Ochwoto M., Ogolodom M. P., Ojo O., Okrostsvaridze N., Oliveira C. P., Omana R. C., Omar O. M., Omar H., Omar M., Omran S., Omran R., Osman M. M., Owise N., Owusu-Ansah T., Padilla- Machaca P. M., Palle S., Pan Z., Pan X. -Y., Pan Q., Papaefthymiou A., Paquissi F. C., Par G., Parkash A., Payawal D., Peltekian K. M., Peng X., Peng L., Peng Y., Pengoria R., Perez M., Perez J. L., Perez N. M., Persico M., Pessoa M. G., Petta S., Philip M., Plaz Torres M. C., Polavarapu N., Poniachik J., Portincasa P., Pu C., Purnak T., Purwanto E., Qi X., Qian Z., Qiang Z., Qiao Z., Qiao L., Queiroz A., Rabiee A., Radwan M., Rahetilahy A. M., Ramadan Y., Ramadan D., Ramli A. S., Ramm G. A., Ran A., Rankovic I., RAO H., Raouf S., Ray S., Reau N., Refaat A., Reiberger T., Remes-Troche J. M., Reyes E. C., Richardson B., Ridruejo E., Riestra Jimenez S., Rizk I., Roberts S., Roblero J. P., Robles J. A. P., Rockey D., Rodriguez M., Rodriguez Hernandez H., Roman E., Romeiro F. G., Romeo S., Rosales-Zabal J. M., Roshdi G. R., Rosso N., Ruf A., Ruiz P. C., Runes N. R., Ruzzenente A., Ryan M., Saad A., Sabbagh E. B., Sabbah M., Saber S., Sabrey R., Sabry R., Saeed M. A., Said D., Said E. M., Sakr M. A., Salah Y., Salama R. M., Salama A., Saleh H., Saleh A., Salem A., Salem A. T., Salifou A., Salih A. F., Salman A., Samouda H., Sanai F., Sanchez-Avila J. F., Sanker L., Sano T., Sanz M., Saparbu T., Sawhney R., Sayed F., Sayed S. A., Sayed A. O., Sayed M., Sebastiani G., Secadas L., Sediqi K. Q., Seif S., Semida N., Senates E., Serban E. D., Serfaty L., Seto W. -K., Sghaier I., Sha M., Shabaan H. M., Shalaby L., Shaltout I., Sharara A. I., Sharma V., Shawa I. T., Shawkat A., Shawky N., Shehata O., Sheils S., Shewaye A. B., Shi G., Shi J., Shimose S., Shirono T., Shou L., Shrestha A., Shui G., Sievert W., Sigurdardottir S., Sira M. M., Siradj R., Sison C., Smyth L., Soliman R., Sollano J. D., Sombie R., Sonderup M., Sood S., Soriano G., Stedman C. A. M., Stefanyuk O., Stimac D., Strasser S., Strnad P., Stuart K., Su W., Su M., Sumida Y., Sumie S., Sun D. -Q., Sun J., Suzuki H., Svegliati-Baroni G., Swar M. O., TAHARBOUCHT S., Taher Z., Takamura S., Tan L., Tan S. -S., Tanwandee T., Tarek S., Tatiana G., Tavaglione F., Tecson G. Y., Tee H. -P., Teschke R., Tharwat M., Thong V. D., Thursz M., Tine T., Tiribelli C., Tolmane I., Tong J., Tongo M., Torkie M., Torre A., Torres E. A., Trajkovska M., Treeprasertsuk S., Tsutsumi T., Tu T., Tur J. A., Turan D., Turcan S., Turkina S., Tutar E., Tzeuton C., Ugiagbe R., Uygun A., Vacca M., Vajro P., Van der Poorten D., Van Kleef L. A., Vashakidze E., Velazquez C. M., Velazquez M. I., Vento S., Verhoeven V., Vespasiani-Gentilucci U., Vethakkan S. R., Vilaseca J., Vitek L., Volkanovska A., Wallace M., Wan W., Wang Y., Wang X., Wang C., Wang M., Wangchuk P., Weltman M., White M., Wiegand J., Wifi M. -N., Wigg A., Wilhelmi M., William R., Wittenburg H., Wu S., Wubeneh A. M., Xia H., Xiao J., Xiao X., Xiaofeng W., Xiong W., Xu L., Xu J., Xu W., Xu J. -H., Xu K., Xu Y., Xu S. -H., Xu M., Xu A., Xu C., Yan H., Yang J., Yang R. -X., Yang Y., Yang Q., Yang N., Yao J., Yara J., Yaras S., Yilmaz N., Younes R., younes H., Young S., Youssef F., Yu Y., Yu M. -L., Yuan J., Yue Z., Yuen M. -F., Yun W., Yurukova N., Zakaria S., Zaky S., Zaldastanishvili M., Zapata R., Zare N., Zerem E., Zeriban N., Zeshuai X., Zhang H., Zhang X., Zhang Y., Zhang W. -H., Zhang Y. -P., Zhang Z. -Q., Zhao J., Zhao R. -R., Zhao H., Zheng C., Zheng Y., Zheng R., Zheng T. -L., Zheng K., Zhou X. Q., Zhou Y., Zhou Y. -J., Zhou H., Zhou L., Zhu L. D., Zhu Y. F., Zhu Y., Zhu P. -W., Ziada E., Ziring D., Ziyi L., Zou S., Zou Z., Zou H., Zuart Ruiz R., Mendez-Sanchez, N, Bugianesi, E, Gish, R, Lammert, F, Tilg, H, Nguyen, M, Sarin, S, Fabrellas, N, Zelber-Sagi, S, Fan, J, Shiha, G, Targher, G, Zheng, M, Chan, W, Vinker, S, Kawaguchi, T, Castera, L, Yilmaz, Y, Korenjak, M, Spearman, C, Ungan, M, Palmer, M, El-Shabrawi, M, Gruss, H, Dufour, J, Dhawan, A, Wedemeyer, H, George, J, Valenti, L, Fouad, Y, Romero-Gomez, M, Eslam, M, Abate, M, Abbas, B, Abbassy, A, Abd El Ghany, W, Abd Elkhalek, A, Abd ElMajeed, E, Abdalgaber, M, Abdallah, M, Abdallah, N, Abdelaleem, S, Abdelghani, Y, Abdelghany, W, Abdelhalim, S, Abdelhamid, W, Abdelhamid, N, Abdelkader, N, Abdelkreem, E, Abdelmohsen, A, Abdelrahman, A, Abd-elsalam, S, Abdeltawab, D, Abduh, A, Abdulhakam, N, Abdulla, M, Abedpoor, N, Abenavoli, L, Aberg, F, Ablack, O, Abo elftouh, M, Abo-Amer, Y, Aboubkr, A, Aboud, A, Abouelnaga, A, Aboufarrag, G, Aboutaleb, A, Abundis, L, Adali, G, Adames, E, Adams, L, Adda, D, Adel, N, Adel Sayed, M, Afaa, T, Afredj, N, Aghayeva, G, Aghemo, A, Aguilar-Salinas, C, Ahlenstiel, G, Ahmady, W, Ahmed, W, Ahmed, A, Ahmed, S, Ahmed, H, Ahmed, R, Aigner, E, Akarsu, M, Akroush, M, Akyuz, U, Al Mahtab, M, Al Qadiri, T, Al Rawahi, Y, AL rubaee, R, Al Saffar, M, Alam, S, Al-Ani, Z, Albillos, A, Alboraie, M, Al-Busafi, S, Al-Emam, M, Alharthi, J, Ali, K, Ali, B, Ali, M, Ali, R, Alisi, A, AL-Khafaji, A, Alkhatry, M, Aller, R, Almansoury, Y, Al-Naamani, K, Alnakeeb, A, Alonso, A, Alqahtani, S, Alrabadi, L, Alswat, K, Altaher, M, Altamimi, T, Altamirano, J, Alvares-da-Silva, M, Aly, E, Alzahaby, A, Alzamzamy, A, Amano, K, Amer, M, Amin, M, Amin, S, Amir, A, Ampuero, J, Anas, N, Andreone, P, Andriamandimby, S, Anees, M, Angela, P, Antonios, M, Arafat, W, Araya, J, Armendariz-Borunda, J, Armstrong, M, Ashktorab, H, Aspichueta, P, Assal, F, Atef, M, Attia, D, Atwa, H, Awad, R, Awad, M, Awny, S, Awolowo, O, Awuku, Y, Ayada, I, Aye, T, Ayman, S, Ayman, H, Ayoub, H, Azmy, H, Babaran, R, Badreldin, O, Badry, A, Bahcecioglu, I, Bahour, A, Bai, J, Balaban, Y, Balasubramanyam, M, Bamakhrama, K, Banales, J, Bangaru, B, Bao, J, Barahona, J, Barakat, S, Barbalho, S, Barbra, B, Barranco, B, Barrera, F, Baumann, U, Bazeed, S, Bech, E, Benayad, A, Benesic, A, Bernstein, D, Bessone, F, Birney, S, Bisseye, C, Blake, M, Bobat, B, Bonfrate, L, Bordin, D, Bosques-Padilla, F, Boursier, J, Boushab, B, Bowen, D, Bravo, P, Brennan, P, Bright, B, Broekaert, I, Buque, X, Burgos-Santamaria, D, Burman, J, Busetto, L, Byrne, C, Cabral-Prodigalidad, P, Cabrera-Alvarez, G, Cai, W, Cainelli, F, Caliskan, A, Canbay, A, Cano-Contreras, A, Cao, H, Cao, Z, Carrion, A, Carubbi, F, Casanovas, T, Castellanos Fernandez, M, Chai, J, Chan, S, Charatcharoenwitthaya, P, Chavez-Tapia, N, Chayama, K, Chen, J, Chen, L, Chen, Z, Chen, H, Chen, S, Chen, Q, Chen, Y, Chen, G, Chen, E, Chen, F, Chen, P, Cheng, R, Cheng, W, Chieh, J, Chokr, I, Cholongitas, E, Choudhury, A, Chowdhury, A, Chukwudike, E, Ciardullo, S, Clayton, M, Clement, K, Cloa, M, Coccia, C, Collazos, C, Colombo, M, Cosar, A, Cotrim, H, Couillerot, J, Coulibaly, A, Crespo, G, Crespo, J, Cruells, M, Cua, I, Dabbous, H, Dalekos, G, D'Alia, P, Dan, L, Dao, V, Darwish, M, Datz, C, Davalos-Moscol, M, Dawoud, H, de Careaga, B, de Knegt, R, de Ledinghen, V, de Silva, J, Debzi, N, Decraecker, M, Del Pozo, E, Delgado, T, Delgado-Blanco, M, Dembinski, L, Depina, A, Derbala, M, Desalegn, H, Desbois-Mouthon, C, Desoky, M, Dev, A, Di Ciaula, A, Diago, M, Diallo, I, Diaz, L, Dirchwolf, M, Dongiovanni, P, Dorofeyev, A, Dou, X, Douglas, M, Doulberis, M, Dovia, C, Doyle, A, Dragojevic, I, Drenth, J, Duan, X, Dulskas, A, Dumitrascu, D, Duncan, O, Dusabejambo, V, Dwawhi, R, Eiketsu, S, El Amrousy, D, El Deeb, A, El Deriny, G, El Din, H, El Kamshishy, S, El Kassas, M, El Raziky, M, Elagamy, O, Elakel, W, Elalfy, D, Elaraby, H, Elawady, H, Elbadawy, R, Eldash, H, Eldefrawy, M, Elecharri, C, Elfaramawy, A, Elfatih, M, Elfiky, M, Elgamsy, M, Elgendy, M, El-Guindi, M, Elhussieny, N, Eliwa, A, Elkabbany, Z, El-Khayat, H, El-Koofy, N, Elmetwalli, A, Elrabat, A, El-Raey, F, Elrashdy, F, Elsahhar, M, Elsaid, E, Elsayed, S, Elsayed, H, Elsayed, A, El-Serafy, M, Elsharkawy, A, Elsheemy, R, Elshemy, E, Elsherbini, S, Eltoukhy, N, Elwakil, R, Emad, O, Emad, S, Embabi, M, Ergenc, I, Ermolova, T, Esmat, G, Esmat, D, Estupinan, E, Ettair, S, Eugen, T, Ezz-Eldin, M, Falcon, L, Fan, Y, Fandari, S, Farag, M, Farahat, T, Fares, E, Fares, M, Fassio, E, Fathy, H, Fathy, D, Fathy, W, Fayed, S, Feng, D, Feng, G, Fernandez-Bermejo, M, Ferreira, C, Ferrer, J, Forbes, A, Fouad, R, Fouad, H, Frisch, T, Fujii, H, Fukunaga, S, Fukunishi, S, Fulya, H, Furuhashi, M, Gaber, Y, Galang, A, Gallardo, J, Galloso, R, Gamal, M, Gamal, R, Gamal, H, Gan, J, Ganbold, A, Gao, X, Garas, G, Garba, T, Garcia-Cortes, M, Garcia-Monzon, C, Garcia-Samaniego, J, Gastaldelli, A, Gatica, M, Gatley, E, Gegeshidze, T, Geng, B, Ghazinyan, H, Ghoneem, S, Giacomelli, L, Giannelli, G, Giannini, E, Giefer, M, Gines, P, Girala, M, Giraudi, P, Goh, G, Gomaa, A, Gong, B, Gonzales, D, Gonzalez, H, Gonzalez-Huezo, M, Graupera, I, Grgurevic, I, Gronbaek, H, Gu, X, Guan, L, Gueye, I, Guingane, A, Gul, O, Gul, C, Guo, Q, Gupta, P, Gurakar, A, Gutierrez, J, Habib, G, Hafez, A, Hagman, E, Halawa, E, Hamdy, O, Hamed, A, Hamed, D, Hamid, S, Hamoudi, W, Han, Y, Haridy, J, Haridy, H, Harris, D, Hart, M, Hasan, F, Hashim, A, Hassan, I, Hassan, A, Hassan, E, Hassan, M, Hassanin, F, Hassnine, A, Haukeland, J, Hawal, A, He, J, He, Q, He, Y, He, F, Hegazy, M, Hegazy, A, Henegil, O, Hernandez, N, Hernandez-Guerra, M, Higuera-de-la-Tijera, F, Hindy, I, Hirota, K, Ho, L, Hodge, A, Hosny, M, Hou, X, Huang, J, Huang, Y, Huang, Z, Huang, A, Huang, X, Hui-ping, S, Hunyady, B, Hussein, M, Hussein, O, Hussien, S, Ibanez-Samaniego, L, Ibdah, J, Ibrahim, L, Ibrahim, M, Ibrahim, I, Icaza-Chavez, M, Idelbi, S, Idilman, R, Ikeda, M, Indolfi, G, Invernizzi, F, Irshad, I, Isa, H, Iskandar, N, Ismaiel, A, Ismail, M, Ismail, Z, Ismail, F, Iwamoto, H, Jack, K, Jacob, R, Jafarov, F, Jafri, W, Jahshan, H, Jalal, P, Jancoriene, L, Janicko, M, Jayasena, H, Jefferies, M, Jha, V, Ji, F, Ji, Y, Jia, J, Jiang, C, Jiang, N, Jiang, Z, Jin, X, Jin, Y, Jing, X, Jingyu, Q, Jinjolava, M, Jong, F, Jucov, A, Julius, I, Kaddah, M, Kamada, Y, Kamal, A, Kamal, E, Kamel, A, Kao, J, Karin, M, Karlas, T, Kashwaa, M, Katsidzira, L, Kaya, E, Kayasseh, M, Keenan, B, Keklikkiran, C, Keml, W, Khalaf, D, Khalefa, R, Khamis, S, Khater, D, Khattab, H, Khavkin, A, Khlynova, O, Khmis, N, Kobyliak, N, Koffas, A, Koike, K, Kok, K, Koller, T, Komas, N, Korochanskaya, N, Koulla, Y, Koya, S, Kraft, C, Kraja, B, Krawczyk, M, Kuchay, M, Kulkarni, A, Kumar, A, Kumar, M, Lakoh, S, Lam, P, Lan, L, Lange, N, Lankarani, K, Lanthier, N, Lapshyna, K, Lashen, S, Laure, K, Lazebnik, L, Lebrec, D, Lee, S, Lee, W, Lee, Y, Leeming, D, Leite, N, Leon, R, Lesmana, C, Li, J, Li, Q, Li, Y, Li, L, Li, M, Liang, H, Lijuan, T, Lim, S, Lim, L, Lin, S, Lin, H, Lin, R, Lithy, R, Liu, Y, Liu, X, Liu, W, Liu, S, Liu, K, Liu, T, Lonardo, A, Lopez, M, Lopez-Benages, E, Lopez-Jaramillo, P, Lu, H, Lu, L, Lu, Y, Lubel, J, Lui, R, Lupasco, I, Luzina, E, Lv, X, Lynch, K, Ma, H, Machado, M, Maduka, N, Madzharova, K, Magdaong, R, Mahadeva, S, Mahfouz, A, Mahmood, N, Mahmoud, E, Mahrous, M, Maiwall, R, Majeed, A, Majumdar, A, Mak, L, Maklouf, M, Malekzadeh, R, Mandato, C, Mangia, A, Mann, J, Mansour, H, Mansouri, A, Mantovani, A, Mao, J, Maramag, F, Marchesini, G, Marcus, C, Marinho, R, Martinez-Chantar, M, Martins, A, Marwan, R, Mason, K, Masoud, G, Massoud, M, Matamoros, M, Mateos, R, Mawed, A, Mbanya, J, Mbendi, C, Mccolaugh, L, Mcleod, D, Medina, J, Megahed, A, Mehrez, M, Memon, I, Merat, S, Mercado, R, Mesbah, A, Meskini, T, Metwally, M, Metwaly, R, Miao, L, Micah, E, Miele, L, Milivojevic, V, Milovanovic, T, Mina, Y, Mishkovik, M, Mishriki, A, Mitchell, T, Mohamed, A, Mohamed, M, Mohamed, S, Mohammed, S, Mohammed, A, Mohan, V, Mohie, S, Mokhtar, A, Moniem, R, Montilla, M, Morales, J, Morata, M, Moreno-Planas, J, Morise, S, Mosaad, S, Moselhy, M, Mostafa, A, Mostafa, E, Mouane, N, Mousa, N, Moustafa, H, Msherif, A, Muller, K, Munoz, C, Munoz-Urribarri, A, Murillo, O, Mustapha, F, Muzurovic, E, Nabil, Y, Nafady, S, Nagamatsu, A, Nakajima, A, Nakano, D, Nan, Y, Nascimbeni, F, Naseef, M, Nashat, N, Natalia, T, Negro, F, Nersesov, A, Neuman, M, Ng'Wanasayi, M, Ni, Y, Nicoll, A, Niizeki, T, Nikolova, D, Ningning, W, Niriella, M, Nogoibaeva, K, Nordien, R, O Sullivan, C, O'Beirne, J, Obekpa, S, Ocama, P, Ochwoto, M, Ogolodom, M, Ojo, O, Okrostsvaridze, N, Oliveira, C, Omana, R, Omar, O, Omar, H, Omar, M, Omran, S, Omran, R, Osman, M, Owise, N, Owusu-Ansah, T, Padilla- Machaca, P, Palle, S, Pan, Z, Pan, X, Pan, Q, Papaefthymiou, A, Paquissi, F, Par, G, Parkash, A, Payawal, D, Peltekian, K, Peng, X, Peng, L, Peng, Y, Pengoria, R, Perez, M, Perez, J, Perez, N, Persico, M, Pessoa, M, Petta, S, Philip, M, Plaz Torres, M, Polavarapu, N, Poniachik, J, Portincasa, P, Pu, C, Purnak, T, Purwanto, E, Qi, X, Qian, Z, Qiang, Z, Qiao, Z, Qiao, L, Queiroz, A, Rabiee, A, Radwan, M, Rahetilahy, A, Ramadan, Y, Ramadan, D, Ramli, A, Ramm, G, Ran, A, Rankovic, I, Rao, H, Raouf, S, Ray, S, Reau, N, Refaat, A, Reiberger, T, Remes-Troche, J, Reyes, E, Richardson, B, Ridruejo, E, Riestra Jimenez, S, Rizk, I, Roberts, S, Roblero, J, Robles, J, Rockey, D, Rodriguez, M, Rodriguez Hernandez, H, Roman, E, Romeiro, F, Romeo, S, Rosales-Zabal, J, Roshdi, G, Rosso, N, Ruf, A, Ruiz, P, Runes, N, Ruzzenente, A, Ryan, M, Saad, A, Sabbagh, E, Sabbah, M, Saber, S, Sabrey, R, Sabry, R, Saeed, M, Said, D, Said, E, Sakr, M, Salah, Y, Salama, R, Salama, A, Saleh, H, Saleh, A, Salem, A, Salifou, A, Salih, A, Salman, A, Samouda, H, Sanai, F, Sanchez-Avila, J, Sanker, L, Sano, T, Sanz, M, Saparbu, T, Sawhney, R, Sayed, F, Sayed, S, Sayed, A, Sayed, M, Sebastiani, G, Secadas, L, Sediqi, K, Seif, S, Semida, N, Senates, E, Serban, E, Serfaty, L, Seto, W, Sghaier, I, Sha, M, Shabaan, H, Shalaby, L, Shaltout, I, Sharara, A, Sharma, V, Shawa, I, Shawkat, A, Shawky, N, Shehata, O, Sheils, S, Shewaye, A, Shi, G, Shi, J, Shimose, S, Shirono, T, Shou, L, Shrestha, A, Shui, G, Sievert, W, Sigurdardottir, S, Sira, M, Siradj, R, Sison, C, Smyth, L, Soliman, R, Sollano, J, Sombie, R, Sonderup, M, Sood, S, Soriano, G, Stedman, C, Stefanyuk, O, Stimac, D, Strasser, S, Strnad, P, Stuart, K, Su, W, Su, M, Sumida, Y, Sumie, S, Sun, D, Sun, J, Suzuki, H, Svegliati-Baroni, G, Swar, M, Taharboucht, S, Taher, Z, Takamura, S, Tan, L, Tan, S, Tanwandee, T, Tarek, S, Tatiana, G, Tavaglione, F, Tecson, G, Tee, H, Teschke, R, Tharwat, M, Thong, V, Thursz, M, Tine, T, Tiribelli, C, Tolmane, I, Tong, J, Tongo, M, Torkie, M, Torre, A, Torres, E, Trajkovska, M, Treeprasertsuk, S, Tsutsumi, T, Tu, T, Tur, J, Turan, D, Turcan, S, Turkina, S, Tutar, E, Tzeuton, C, Ugiagbe, R, Uygun, A, Vacca, M, Vajro, P, Van der Poorten, D, Van Kleef, L, Vashakidze, E, Velazquez, C, Velazquez, M, Vento, S, Verhoeven, V, Vespasiani-Gentilucci, U, Vethakkan, S, Vilaseca, J, Vitek, L, Volkanovska, A, Wallace, M, Wan, W, Wang, Y, Wang, X, Wang, C, Wang, M, Wangchuk, P, Weltman, M, White, M, Wiegand, J, Wifi, M, Wigg, A, Wilhelmi, M, William, R, Wittenburg, H, Wu, S, Wubeneh, A, Xia, H, Xiao, J, Xiao, X, Xiaofeng, W, Xiong, W, Xu, L, Xu, J, Xu, W, Xu, K, Xu, Y, Xu, S, Xu, M, Xu, A, Xu, C, Yan, H, Yang, J, Yang, R, Yang, Y, Yang, Q, Yang, N, Yao, J, Yara, J, Yaras, S, Yilmaz, N, Younes, R, Younes, H, Young, S, Youssef, F, Yu, Y, Yu, M, Yuan, J, Yue, Z, Yuen, M, Yun, W, Yurukova, N, Zakaria, S, Zaky, S, Zaldastanishvili, M, Zapata, R, Zare, N, Zerem, E, Zeriban, N, Zeshuai, X, Zhang, H, Zhang, X, Zhang, Y, Zhang, W, Zhang, Z, Zhao, J, Zhao, R, Zhao, H, Zheng, C, Zheng, Y, Zheng, R, Zheng, T, Zheng, K, Zhou, X, Zhou, Y, Zhou, H, Zhou, L, Zhu, L, Zhu, Y, Zhu, P, Ziada, E, Ziring, D, Ziyi, L, Zou, S, Zou, Z, Zou, H, Zuart Ruiz, R, Mendez-Sanchez N., Bugianesi E., Gish R. G., Lammert F., Tilg H., Nguyen M. H., Sarin S. K., Fabrellas N., Zelber-Sagi S., Fan J. -G., Shiha G., Targher G., Zheng M. -H., Chan W. -K., Vinker S., Kawaguchi T., Castera L., Yilmaz Y., Korenjak M., Spearman C. W., Ungan M., Palmer M., El-Shabrawi M., Gruss H. -J., Dufour J. -F., Dhawan A., Wedemeyer H., George J., Valenti L., Fouad Y., Romero-Gomez M., Eslam M., Abate M. L., Abbas B., Abbassy A. A., Abd El Ghany W., Abd Elkhalek A., Abd ElMajeed E., Abdalgaber M., AbdAllah M., Abdallah M., Abdallah N., Abdelaleem S., Abdelghani Y., Abdelghany W., Abdelhalim S. M., Abdelhamid W., Abdelhamid N., Abdelkader N. A., Abdelkreem E., Abdelmohsen A. M., Abdelrahman A. A., Abd-elsalam S. M., Abdeltawab D., Abduh A., Abdulhakam N., Abdulla M., Abedpoor N., Abenavoli L., Aberg F., Ablack O., Abo elftouh M., Abo-Amer Y. E. -E., Aboubkr A., Aboud A., Abouelnaga A. M., Aboufarrag G. A., Aboutaleb A., Abundis L., Adali G., Adames E., Adams L., Adda D., Adel N., Adel Sayed M., Afaa T. J., Afredj N., Aghayeva G., Aghemo A., Aguilar-Salinas C. A., Ahlenstiel G., Ahmady W., Ahmed W., Ahmed A., Ahmed S. N., Ahmed H. M., Ahmed R., Aigner E., Akarsu M., Akroush M., Akyuz U., Al Mahtab M., Al Qadiri T., Al Rawahi Y., AL rubaee R., Al Saffar M., Alam S., Al-Ani Z., Albillos A., Alboraie M., Al-Busafi S., Al-Emam M., Alharthi J., Ali K., Ali B. A., Ali M., Ali R. A. R., Alisi A., AL-Khafaji A. R., Alkhatry M., Aller R., Almansoury Y., Al-Naamani K., Alnakeeb A., Alonso A., Alqahtani S. A., Alrabadi L., Alswat K., Altaher M., Altamimi T., Altamirano J., Alvares-da-Silva M. R., Aly E. A. M., Alzahaby A., Alzamzamy A., Amano K., Amer M. A., Amin M. A., Amin S. A., Amir A. A., Ampuero J., Anas N., Andreone P., Andriamandimby S. F., Anees M., Angela P., Antonios M., Arafat W., Araya J. M., Armendariz-Borunda J., Armstrong M. J., Ashktorab H., Aspichueta P., Assal F., Atef M., Attia D., Atwa H., Awad R., Awad M. A. E., Awny S., Awolowo O., Awuku Y. A., Ayada I., Aye T. T., Ayman S., Ayman H., Ayoub H., Azmy H. M., Babaran R. P., Badreldin O., Badry A., Bahcecioglu I. H., Bahour A., Bai J., Balaban Y., Balasubramanyam M., Bamakhrama K., Banales J. M., Bangaru B., Bao J., Barahona J. S., Barakat S., Barbalho S. M., Barbra B., Barranco B., Barrera F., Baumann U., Bazeed S., Bech E., Benayad A., Benesic A., Bernstein D., Bessone F., Birney S., Bisseye C., Blake M., Bobat B., Bonfrate L., Bordin D. S., Bosques-Padilla F., Boursier J., Boushab B. M., Bowen D., Bravo P. M., Brennan P. N., Bright B., Broekaert I., Buque X., Burgos-Santamaria D., Burman J., Busetto L., Byrne C. D., Cabral-Prodigalidad P. A. I., Cabrera-Alvarez G., Cai W., Cainelli F., Caliskan A. R., Canbay A., Cano-Contreras A., Cao H. -X., Cao Z., Carrion A., Carubbi F., Casanovas T., Castellanos Fernandez M. I., Chai J., Chan S. P., Charatcharoenwitthaya P., Chavez-Tapia N., Chayama K., Chen J., Chen L., Chen Z. -W., Chen H., Chen S. -D., Chen Q., Chen Y., Chen G., Chen E. -Q., Chen F., Chen P. -J., Cheng R., Cheng W., Chieh J. T. W., Chokr I., Cholongitas E., Choudhury A., Chowdhury A., Chukwudike E. S., Ciardullo S., Clayton M., Clement K., Cloa M. M., Coccia C., Collazos C., Colombo M., Cosar A. M., Cotrim H. P., Couillerot J., Coulibaly A., Crespo G., Crespo J., Cruells M., Cua I. H. Y., Dabbous H. K., Dalekos G. N., D'Alia P., Dan L., Dao V. H., Darwish M., Datz C., Davalos-Moscol M. B., Dawoud H., de Careaga B. O., de Knegt R., de Ledinghen V., de Silva J., Debzi N., Decraecker M., Del Pozo E., Delgado T. C., Delgado-Blanco M., Dembinski L., Depina A., Derbala M., Desalegn H., Desbois-Mouthon C., Desoky M., Dev A., Di Ciaula A., Diago M., Diallo I., Diaz L. A., Dirchwolf M., Dongiovanni P., Dorofeyev A., Dou X., Douglas M. W., Doulberis M., Dovia C. K., Doyle A., Dragojevic I., Drenth J. P., Duan X., Dulskas A., Dumitrascu D. L., Duncan O., Dusabejambo V., Dwawhi R. S. N. A., Eiketsu S., El Amrousy D., El Deeb A., El Deriny G., El Din H. S., El Kamshishy S., El Kassas M., El Raziky M., Elagamy O. A., Elakel W., Elalfy D., Elaraby H., ElAwady H., Elbadawy R., Eldash H. H., Eldefrawy M. S., Elecharri C. L., Elfaramawy A., Elfatih M., Elfiky M., Elgamsy M., Elgendy M., El-Guindi M. A., Elhussieny N., Eliwa A. M., Elkabbany Z., El-Khayat H., El-Koofy N. M., Elmetwalli A., Elrabat A., El-Raey F., Elrashdy F., Elsahhar M., Elsaid E. M., Elsayed S., Elsayed H., Elsayed A., Elsayed A. M., El-Serafy M., Elsharkawy A. M., Elsheemy R. Y., Elshemy E. E., Elsherbini S., Eltoukhy N., Elwakil R., Emad O., Emad S., Embabi M., Ergenc I., Ermolova T., Esmat G., Esmat D. M., Estupinan E. C., Ettair S., Eugen T., Ezz-Eldin M., Falcon L. P. V., Fan Y. -C., Fandari S., Farag M., Farahat T. M., Fares E. M., Fares M., Fassio E., Fathy H., Fathy D., Fathy W., Fayed S., Feng D., Feng G., Fernandez-Bermejo M., Ferreira C. T., Ferrer J. D., Forbes A., Fouad R., Fouad H. M., Frisch T., Fujii H., Fukunaga S., Fukunishi S., Fulya H., Furuhashi M., Gaber Y., Galang A. J. G., Gallardo J. C., Galloso R., Gamal M., Gamal R., Gamal H., Gan J., Ganbold A., Gao X., Garas G., Garba T., Garcia-Cortes M., Garcia-Monzon C., Garcia-Samaniego J., Gastaldelli A., Gatica M., Gatley E., Gegeshidze T., Geng B., Ghazinyan H., Ghoneem S., Giacomelli L., Giannelli G., Giannini E. G., Giefer M., Gines P., Girala M., Giraudi P. J., Goh G. B. -B., Gomaa A. A., Gong B., Gonzales D. H. C., Gonzalez H. C., Gonzalez-Huezo M. S., Graupera I., Grgurevic I., Gronbaek H., Gu X., Guan L., Gueye I., Guingane A. N., Gul O. O., Gul C. B., Guo Q., Gupta P. P., Gurakar A., Gutierrez J. C. R., Habib G., Hafez A., Hagman E., Halawa E., Hamdy O., Hamed A. E., Hamed D. H., Hamid S., Hamoudi W., Han Y., Haridy J., Haridy H., Harris D. C. H. H., Hart M., Hasan F., Hashim A., Hassan I., Hassan A., Hassan E. A., Hassan A. A., Hassan M. S., Hassanin F., Hassnine A., Haukeland J. W., Hawal A. I. M., He J., He Q., He Y., He F. -P., Hegazy M., Hegazy A., Henegil O., Hernandez N., Hernandez-Guerra M., Higuera-de-la-Tijera F., Hindy I., Hirota K., Ho L. C., Hodge A., Hosny M., Hou X., Huang J. -F., Huang Y., Huang Z., Huang A., Huang X. -P., Hui-ping S., Hunyady B., Hussein M. A., Hussein O., Hussien S. M., Ibanez-Samaniego L., Ibdah J., Ibrahim L., Ibrahim M., Ibrahim I., Icaza-Chavez M. E., Idelbi S., Idilman R. I., Ikeda M., Indolfi G., Invernizzi F., Irshad I., Isa H. M. A., Iskandar N. J., Ismaiel A., Ismail M., Ismail Z., Ismail F., Iwamoto H., Jack K., Jacob R., Jafarov F., Jafri W., Jahshan H., Jalal P. K., Jancoriene L., Janicko M., Jayasena H., Jefferies M., Jha V., Ji F., Ji Y., Jia J., Jiang C., Jiang N., Jiang Z. -Z., Jin X., Jin Y., Jing X., Jingyu Q., Jinjolava M., Jong F. H. H., Jucov A., Julius I., Kaddah M., Kamada Y., kamal A., Kamal E. M., Kamel A. S., Kao J. -H., Karin M., Karlas T., Kashwaa M., Katsidzira L., Kaya E., Kayasseh M. A., Keenan B., Keklikkiran C., Keml W., Khalaf D. K., Khalefa R., Khamis S., Khater D., khattab H., Khavkin A., Khlynova O., Khmis N., Kobyliak N., Koffas A., Koike K., Kok K. Y. Y., Koller T., Komas N. P., Korochanskaya N. V., Koulla Y., Koya S., Kraft C., Kraja B., Krawczyk M., Kuchay M. S., Kulkarni A. V., Kumar A., Kumar M., Lakoh S., Lam P., Lan L., Lange N. F., Lankarani K. B., Lanthier N., Lapshyna K., Lashen S. A., Laure K. N. J., Lazebnik L., Lebrec D., Lee S. S., Lee W. S., Lee Y. Y., Leeming D. J., Leite N. C., Leon R., Lesmana C. R. A., Li J., Li Q., Li Y. -Y., Li Y., Li L., Li M., li Y., Liang H., Lijuan T., Lim S. G., Lim L. -L., Lin S., Lin H. -C., Lin R., Lithy R., Liu Y., Liu X., Liu W. -Y., Liu S., Liu K., Liu T., Lonardo A., Lopez M. B., Lopez-Benages E., Lopez-Jaramillo P., Lu H., Lu L. G., Lu Y., Lubel J., Lui R., Lupasco I., Luzina E., Lv X. -H., Lynch K., Ma H. -L., Machado M. V., Maduka N., Madzharova K., Magdaong R., Mahadeva S., Mahfouz A., Mahmood N. R. K. N., Mahmoud E., Mahrous M., Maiwall R., Majeed A., Majumdar A., Mak L., Maklouf M. M., Malekzadeh R., Mandato C., Mangia A., Mann J., Mansour H. H., Mansouri A., Mantovani A., Mao J. Q., Maramag F., Marchesini G., Marcus C., Marinho R. A. R. T., Martinez-Chantar M. L., Martins A. A. S., Marwan R., Mason K. F., Masoud G., Massoud M. N., Matamoros M. A., Mateos R. M., Mawed A., Mbanya J. C., Mbendi C., McColaugh L., McLeod D., Medina J. F. R., Megahed A., Mehrez M., Memon I., Merat S., Mercado R., Mesbah A., Meskini T., Metwally M., Metwaly R., Miao L., Micah E., Miele L., Milivojevic V., Milovanovic T., Mina Y. L., Mishkovik M., Mishriki A., Mitchell T., Mohamed A., Mohamed M., Mohamed S., Mohammed S., Mohammed A., Mohan V., Mohie S., Mokhtar A., Moniem R., Montilla M. S., Morales J. A. O., Morata M. M. S., Moreno-Planas J. M., Morise S., Mosaad S., Moselhy M., Mostafa A. M., Mostafa E., Mouane N., Mousa N., Moustafa H. M., Msherif A., Muller K., Munoz C., Munoz-Urribarri A. B., Murillo O. A., Mustapha F. I., Muzurovic E., Nabil Y., Nafady S., Nagamatsu A., Nakajima A., Nakano D., Nan Y., Nascimbeni F., Naseef M. S., Nashat N., Natalia T., Negro F., Nersesov A. V., Neuman M., Ng'wanasayi M., Ni Y., Nicoll A., Niizeki T., Nikolova D., Ningning W., Niriella M., Nogoibaeva K. A., Nordien R., O Sullivan C., O'Beirne J., Obekpa S., Ocama P., Ochwoto M., Ogolodom M. P., Ojo O., Okrostsvaridze N., Oliveira C. P., Omana R. C., Omar O. M., Omar H., Omar M., Omran S., Omran R., Osman M. M., Owise N., Owusu-Ansah T., Padilla- Machaca P. M., Palle S., Pan Z., Pan X. -Y., Pan Q., Papaefthymiou A., Paquissi F. C., Par G., Parkash A., Payawal D., Peltekian K. M., Peng X., Peng L., Peng Y., Pengoria R., Perez M., Perez J. L., Perez N. M., Persico M., Pessoa M. G., Petta S., Philip M., Plaz Torres M. C., Polavarapu N., Poniachik J., Portincasa P., Pu C., Purnak T., Purwanto E., Qi X., Qian Z., Qiang Z., Qiao Z., Qiao L., Queiroz A., Rabiee A., Radwan M., Rahetilahy A. M., Ramadan Y., Ramadan D., Ramli A. S., Ramm G. A., Ran A., Rankovic I., RAO H., Raouf S., Ray S., Reau N., Refaat A., Reiberger T., Remes-Troche J. M., Reyes E. C., Richardson B., Ridruejo E., Riestra Jimenez S., Rizk I., Roberts S., Roblero J. P., Robles J. A. P., Rockey D., Rodriguez M., Rodriguez Hernandez H., Roman E., Romeiro F. G., Romeo S., Rosales-Zabal J. M., Roshdi G. R., Rosso N., Ruf A., Ruiz P. C., Runes N. R., Ruzzenente A., Ryan M., Saad A., Sabbagh E. B., Sabbah M., Saber S., Sabrey R., Sabry R., Saeed M. A., Said D., Said E. M., Sakr M. A., Salah Y., Salama R. M., Salama A., Saleh H., Saleh A., Salem A., Salem A. T., Salifou A., Salih A. F., Salman A., Samouda H., Sanai F., Sanchez-Avila J. F., Sanker L., Sano T., Sanz M., Saparbu T., Sawhney R., Sayed F., Sayed S. A., Sayed A. O., Sayed M., Sebastiani G., Secadas L., Sediqi K. Q., Seif S., Semida N., Senates E., Serban E. D., Serfaty L., Seto W. -K., Sghaier I., Sha M., Shabaan H. M., Shalaby L., Shaltout I., Sharara A. I., Sharma V., Shawa I. T., Shawkat A., Shawky N., Shehata O., Sheils S., Shewaye A. B., Shi G., Shi J., Shimose S., Shirono T., Shou L., Shrestha A., Shui G., Sievert W., Sigurdardottir S., Sira M. M., Siradj R., Sison C., Smyth L., Soliman R., Sollano J. D., Sombie R., Sonderup M., Sood S., Soriano G., Stedman C. A. M., Stefanyuk O., Stimac D., Strasser S., Strnad P., Stuart K., Su W., Su M., Sumida Y., Sumie S., Sun D. -Q., Sun J., Suzuki H., Svegliati-Baroni G., Swar M. O., TAHARBOUCHT S., Taher Z., Takamura S., Tan L., Tan S. -S., Tanwandee T., Tarek S., Tatiana G., Tavaglione F., Tecson G. Y., Tee H. -P., Teschke R., Tharwat M., Thong V. D., Thursz M., Tine T., Tiribelli C., Tolmane I., Tong J., Tongo M., Torkie M., Torre A., Torres E. A., Trajkovska M., Treeprasertsuk S., Tsutsumi T., Tu T., Tur J. A., Turan D., Turcan S., Turkina S., Tutar E., Tzeuton C., Ugiagbe R., Uygun A., Vacca M., Vajro P., Van der Poorten D., Van Kleef L. A., Vashakidze E., Velazquez C. M., Velazquez M. I., Vento S., Verhoeven V., Vespasiani-Gentilucci U., Vethakkan S. R., Vilaseca J., Vitek L., Volkanovska A., Wallace M., Wan W., Wang Y., Wang X., Wang C., Wang M., Wangchuk P., Weltman M., White M., Wiegand J., Wifi M. -N., Wigg A., Wilhelmi M., William R., Wittenburg H., Wu S., Wubeneh A. M., Xia H., Xiao J., Xiao X., Xiaofeng W., Xiong W., Xu L., Xu J., Xu W., Xu J. -H., Xu K., Xu Y., Xu S. -H., Xu M., Xu A., Xu C., Yan H., Yang J., Yang R. -X., Yang Y., Yang Q., Yang N., Yao J., Yara J., Yaras S., Yilmaz N., Younes R., younes H., Young S., Youssef F., Yu Y., Yu M. -L., Yuan J., Yue Z., Yuen M. -F., Yun W., Yurukova N., Zakaria S., Zaky S., Zaldastanishvili M., Zapata R., Zare N., Zerem E., Zeriban N., Zeshuai X., Zhang H., Zhang X., Zhang Y., Zhang W. -H., Zhang Y. -P., Zhang Z. -Q., Zhao J., Zhao R. -R., Zhao H., Zheng C., Zheng Y., Zheng R., Zheng T. -L., Zheng K., Zhou X. Q., Zhou Y., Zhou Y. -J., Zhou H., Zhou L., Zhu L. D., Zhu Y. F., Zhu Y., Zhu P. -W., Ziada E., Ziring D., Ziyi L., Zou S., Zou Z., Zou H., and Zuart Ruiz R.

Published
2022

Catalog

Books, media, physical & digital resources
See catalog results