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118 results on '"Fan, Q. W."'

1. Measurement of the $^{159}$Tb(n, $\gamma$) cross section at the CSNS Back-n facility

Author

Zhang, S., Li, G., Jiang, W., Wang, D. X., Ren, J., Li, E. T., Huang, M., Tang, J. Y., Ruan, X. C., Wang, H. W., Li, Z. H., Chen, Y. S., Liu, L. X., Li, X. X., Fan, Q. W., Fan, R. R., Hu, X. R., Wang, J. C., Li, X., Niu, 1D. D., Song, N., and Gu, M.

Subjects
Nuclear Experiment, Astrophysics - Solar and Stellar Astrophysics
Abstract

The stellar (n, $\gamma$) cross section data for the mass numbers around A $\approx$ 160 are of key importance to nucleosynthesis in the main component of the slow neutron capture process, which occur in the thermally pulsing asymptotic giant branch (TP--AGB). The new measurement of (n, $\gamma$) cross sections for $^{159}$Tb was performed using the C$_6$D$_6$ detector system at the back streaming white neutron beam line (Back-n) of the China spallation neutron source (CSNS) with neutron energies ranging from 1 eV to 1 MeV. Experimental resonance capture kernels were reported up to 1.2 keV neutron energy with this capture measurement. Maxwellian-averaged cross sections (MACS) were derived from the measured $^{159}$Tb (n, $\gamma$) cross sections at $kT$ = 5 $\sim$ 100 keV and are in good agreement with the recommended data of KADoNiS-v0.3 and JEFF-3.3, while KADoNiS-v1.0 and ENDF-VIII.0 significantly overestimate the present MACS up to 40$\%$ and 20$\%$, respectively. A sensitive test of the s-process nucleosynthesis was also performed with the stellar evolution code MESA. Significant changes in abundances around A $\approx$ 160 were observed between the ENDF/B-VIII.0 and present measured rate of $^{159}$Tb(n, $\gamma$)$^{160}$Tb in the MESA simulation., Comment: 13 pages, 7 figures

Published
2022
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2. Deep underground laboratory measurement of $^{13}$C($\alpha$,$n$)$^{16}$O in the Gamow windows of the $s$- and $i$-processes

Author

Gao, B., Jiao, T. Y., Li, Y. T., Chen, H., Lin, W. P., An, Z., Ru, L. H., Zhang, Z. C., Tang, X. D., Wang, X. Y., Zhang, N. T., Fang, X., Xie, D. H., Fan, Y. H., Ma, L., Zhang, X., Bai, F., Wang, P., Fan, Y. X., Liu, G., Huang, H. X., Wu, Q., Zhu, Y. B., Chai, J. L., Li, J. Q., Sun, L. T., Wang, S., Cai, J. W., Li, Y. Z., Su, J., Zhang, H., Li, Z. H., Li, Y. J., Li, E. T., Chen, C., Shen, Y. P., Lian, G., Guo, B., Li, X. Y., Zhang, L. Y., He, J. J., Sheng, Y. D., Chen, Y. J., Wang, L. H., Zhang, L., Cao, F. Q., Nan, W., Nan, W. K., Li, G. X., Song, N., Cui, B. Q., Chen, L. H., Ma, R. G., Yan, S. Q., Liao, J. H., Wang, Y. B., Zeng, S., Nan, D., Fan, Q. W., Qi, N. C., Sun, W. L., Guo, X. Y., Zhang, P., Chen, Y. H., Zhou, Y., Zhou, J. F., He, J. R., Shang, C. S., Li, M. C., Kubono, S., Liu, W. P., deBoer, R. J., Wiescher, M., and Pignatari, M.

Subjects
Nuclear Experiment
Abstract

The $^{13}$C($\alpha$,$n$)$^{16}$O reaction is the main neutron source for the slow-neutron-capture (s-) process in Asymptotic Giant Branch stars and for the intermediate (i-) process. Direct measurements at astrophysical energies in above-ground laboratories are hindered by the extremely small cross sections and vast cosmic-ray induced background. We performed the first consistent direct measurement in the range of $E_{\rm c.m.}=$0.24 MeV to 1.9 MeV using the accelerators at the China Jinping Underground Laboratory (CJPL) and Sichuan University. Our measurement covers almost the entire i-process Gamow window in which the large uncertainty of the previous experiments has been reduced from 60\% down to 15\%, eliminates the large systematic uncertainty in the extrapolation arising from the inconsistency of existing data sets, and provides a more reliable reaction rate for the studies of the s- and i-processes along with the first direct determination of the alpha strength for the near-threshold state.

Published
2022
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3. The $^{59}$Fe(n, {\gamma})$^{60}$Fe Cross Section from the Surrogate Ratio Method and Its Effect on the $^{60}$Fe Nucleosynthesis

Author

Yan, S. Q., Li, X. Y., Nishio, K., Lugaro, M., Li, Z. H., Makii, H., Pignatari, M., Wang, Y. B., Orlandi, R., Hirose, K., Tsukada, K., Mohr, P., Li, G. S., Wang, J. G., Gao, B. S., Han, Y. L., Guo, B., Li, Y. J., Shen, Y. P., Sato, T. K., Ito, Y., Suzaki, F., Su, J., Yang, Y. Y., Wang, J. S., Ma, J. B., Ma, P., Bai, Z., Xu, S. W., Ren, J., Fan, Q. W., Zeng, S., Han, Z. Y., Nan, W., Nan, W. K., Chen, C., Lian, G., Hu, Q., Duan, F. F., Jin, S. Y., Tang, X. D., and Liu, W. P.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

The long-lived $^{60}$Fe (with a half-life of 2.62 Myr) is a crucial diagnostic of active nucleosynthesis in the Milky Way galaxy and in supernovae near the solar system. The neutron-capture reaction $^{59}$Fe(n,$\gamma$)$^{60}$Fe on $^{59}$Fe (half-life = 44.5 days) is the key reaction for the production of $^{60}$Fe in massive stars. This reaction cross section has been previously constrained by the Coulomb dissociation experiment, which offered partial constraint on the $E$1 $\gamma$-ray strength function but a negligible constraint on the $M$1 and $E$2 components. In this work, for the first time, we use the surrogate ratio method to experimentally determine the $^{59}$Fe(n,$\gamma$)$^{60}$Fe cross sections in which all the components are included. We derived a Maxwellian-averaged cross section of 27.5 $\pm$ 3.5 mb at $kT$= 30 keV and 13.4 $\pm$ 1.7 mb at $kT$= 90 keV, roughly 10 - 20% higher than previous estimates. We analyzed the impact of our new reaction rates in nucleosynthesis models of massive stars and found that uncertainties in the production of $^{60}$Fe from the $^{59}$Fe(n,$\gamma$)$^{60}$Fe rate are at most of 25%. We conclude that stellar physics uncertainties now play a major role in the accurate evaluation of the stellar production of $^{60}$Fe., Comment: 9 pages with 6 figures

Published
2021
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4. Astrophysical $S_{E2}$ factor of the ${}^{12}\mathrm{C}(\alpha,\gamma){}^{16}\mathrm{O}$ reaction through the ${}^{12}\mathrm{C}({}^{11}\mathrm{B},{}^{7}\mathrm{Li}){}^{16}\mathrm{O}$ transfer reaction

Author

Shen, Y. P., Guo, B., Li, Z. H., Li, Y. J., Pang, D. Y., Adhikari, S., An, Z. D., Su, J., Yan, S. Q., Du, X. C., Fan, Q. W., Gan, L., Han, Z. Y., Li, D. H., Li, E. T., Lian, G., Liu, J. C., Ma, T. L., Pei, C. J., Su, Y., Wang, Y. B., Zhou, Y., and Liu, W. P.

Subjects
Nuclear Experiment
Abstract

The ${}^{12}\mathrm{C}(\alpha,\gamma){}^{16}\mathrm{O}$ reaction plays a key role in the evolution of stars with masses of $M >$ 0.55 $M_\odot$. The cross-section of the ${}^{12}\mathrm{C}(\alpha,\gamma){}^{16}\mathrm{O}$ reaction within the Gamow window ($E_\textrm{c.m.}$ = 300 keV, $T_\textrm9$ = 0.2) is extremely small (about $10^{-17}$ barn), which makes the direct measurement in a ground-based laboratory with existing techniques unfeasible. Up until now, the cross-sections at lower energies can only be extrapolated from the data at higher energies. However, two subthreshold resonances, located at $E_x$ = 7.117 MeV and $E_x$ = 6.917 MeV, make this extrapolation more complicated. In this work, the 6.917 MeV subthreshold resonance in the ${}^{12}\mathrm{C}(\alpha,\gamma){}^{16}\mathrm{O}$ reaction was investigated via the ${}^{12}\mathrm{C}({}^{11}\mathrm{B},{}^{7}\mathrm{Li}){}^{16}\mathrm{O}$ reaction. The experiment was performed using the Q3D magnetic spectrograph at the HI-13 tandem accelerator. We measured the angular distribution of the ${}^{12}\mathrm{C}({}^{11}\mathrm{B},{}^{7}\mathrm{Li}){}^{16}\mathrm{O}$ transfer reaction leading to the 6.917 MeV state. Based on the FRDWBA analysis, we derived the asymptotic normalization coefficient (ANC) of the 6.917 MeV level in $^{16}$O to be (1.10 $\pm$ 0.29) $\times 10^{10}$ fm$^{-1}$, with which the reduced $\alpha$ width was computed to be $18.0\pm4.7$ keV at the channel radius of 6.5 fm. Finally, we calculated the astrophysical $S_{E2}(300)$ factor of the ground-state transitions to be 46.2 $\pm$ 7.7 keV b. The result for the astrophysical $S_{E2}(300)$ factor confirms the values obtained in various direct and indirect measurements and presents an independent examination of the most important data in nuclear astrophysics., Comment: submitted to Physical Review C

Published
2018
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5. Proton widths of the low-lying 16F states from the 15N(7Li, 6Li)16N reaction

Author

Wu, Z. D., Guo, B., Li, Z. H., Li, Y. J., Su, J., Pang, D. Y., Yan, S. Q., Li, E. T., Bai, X. X., Du, X. C., Fan, Q. W., Gan, L., He, J. J., Jin, S. J., Jing, L., Li, L., Li, Z. C., Lian, G., Liu, J. C., Shen, Y. P., Wang, Y. B., Yu, X. Q., Zeng, S., Zhang, D. H., Zhang, L. Y., Zhang, W. J., and Liu, W. P.

Subjects
Nuclear Experiment
Abstract

All the 16F levels are unbound by proton emission. To date the four low-lying 16F levels below 1 MeV have been experimentally identified with well established spin-parity values and excitation energies with an accuracy of 4 - 6 keV. However, there are still considerable discrepancies for their level widths. The present work aims to explore these level widths through an independent method. The angular distributions of the 15N(7Li, 6Li)16N reaction leading to the first four states in 16N were measured using a high-precision Q3D magnetic spectrograph. The neutron spectroscopic factors and the asymptotic normalization coefficients for these states in 16N were then derived based on distorted wave Born approximation analysis. The proton widths of the four low-lying resonant states in 16F were obtained according to charge symmetry of strong interaction., Comment: 14 pages, 6 figures, 4 tables

Published
2014
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6. Spectroscopic factors for low-lying 16N levels and the astrophysical 15N(n,gamma)16N reaction rate

Author

Guo, B., Li, Z. H., Li, Y. J., Su, J., Pang, D. Y., Yan, S. Q., Wu, Z. D., Li, E. T., Bai, X. X., Du, X. C., Fan, Q. W., Gan, L., He, J. J., Jin, S. J., Jing, L., Li, L., Li, Z. C., Lian, G., Liu, J. C., Shen, Y. P., Wang, Y. B., Yu, X. Q., Zeng, S., Zhang, L. Y., Zhang, W. J., and Liu, W. P.

Subjects
Nuclear Experiment
Abstract

Fluorine is a key element for nucleosynthetic studies since it is extremely sensitive to the physical conditions within stars. The astrophysical site to produce fluorine is suggested to be asymptotic giant branch (AGB) stars. In these stars the 15N(n, g)16N reaction could affect the abundance of fluorine by competing with 15N(a, g)19F. The 15N(n, g)16N reaction rate depends directly on the neutron spectroscopic factors of the low-lying states in 16N. The angular distributions of the 15N(7Li, 6Li)16N reaction populating the ground state and the first three excited states in 16N are measured using a Q3D magnetic spectrograph and are used to derive the spectroscopic factors of these states based on distorted wave Born approximation (DWBA) analysis. The spectroscopic factors of these four states are extracted to be 0.96+-0.09, 0.69+-0.09, 0.84+-0.08 and 0.65+-0.08, respectively. Based on the new spectroscopic factors we derive the 15N(n,g)16N reaction rate. The accuracy and precision of the spectroscopic factors are enhanced due to the first application of high-precision magnetic spectrograph for resolving the closely-spaced 16N levels which can not be achieved in most recent measurement. The present result demonstrates that two levels corresponding to neutron transfers to the 2s1/2 orbit in 16N are not so good single-particle levels although 15N is a closed neutron-shell nucleus. This finding is contrary to the shell model expectation. The present work also provides an independent examination to shed some light on the existing discrepancies in the spectroscopic factors and the 15N(n, g)16N rate., Comment: 13 pages, 4 figures, 2 tables

Published
2013
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7. New determination of the 13C(a, n)16O reaction rate and its influence on the s-process nucleosynthesis in AGB stars

Author

Guo, B., Li, Z. H., Lugaro, M., Buntain, J., Pang, D. Y., Li, Y. J., Su, J., Yan, S. Q., Bai, X. X., Chen, Y. S., Fan, Q. W., Jin, S. J., Karakas, A. I., Li, E. T., Li, Z. C., Lian, G., Liu, J. C., Liu, X., Shi, J. R., Shu, N. C., Wang, B. X., Wang, Y. B., Zeng, S., and Liu, W. P.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Nuclear Experiment
Abstract

We present a new measurement of the $\alpha$-spectroscopic factor ($S_\alpha$) and the asymptotic normalization coefficient (ANC) for the 6.356 MeV 1/2$^+$ subthreshold state of $^{17}$O through the $^{13}$C($^{11}$B, $^{7}$Li)$^{17}$O transfer reaction and we determine the $\alpha$-width of this state. This is believed to have a strong effect on the rate of the $^{13}$C($\alpha$, $n$)$^{16}$O reaction, the main neutron source for {\it slow} neutron captures (the $s$-process) in asymptotic giant branch (AGB) stars. Based on the new width we derive the astrophysical S-factor and the stellar rate of the $^{13}$C($\alpha$, $n$)$^{16}$O reaction. At a temperature of 100 MK our rate is roughly two times larger than that by \citet{cau88} and two times smaller than that recommended by the NACRE compilation. We use the new rate and different rates available in the literature as input in simulations of AGB stars to study their influence on the abundances of selected $s$-process elements and isotopic ratios. There are no changes in the final results using the different rates for the $^{13}$C($\alpha$, $n$)$^{16}$O reaction when the $^{13}$C burns completely in radiative conditions. When the $^{13}$C burns in convective conditions, as in stars of initial mass lower than $\sim$2 $M_\sun$ and in post-AGB stars, some changes are to be expected, e.g., of up to 25% for Pb in our models. These variations will have to be carefully analyzed when more accurate stellar mixing models and more precise observational constraints are available.

Published
2012
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8. Asymptotic normalization coefficient from the 12C(7Li,6He)13N reaction and the astrophysical 12C(p,g)13N reaction rate

Author

Li, Z. H., Su, J., Guo, B., Li, Z. C., Bai, X. X., Liu, J. C., Li, Y. J., Yan, S. Q., Wang, B. X., Wang, Y. B., Lian, G., Zeng, S., Li, E. T., Fang, X., Liu, W. P., Chen, Y. S., Shu, N. C., and Fan, Q. W.

Subjects
Nuclear Experiment
Abstract

Angular distribution of the 12C(7Li,6He)13N reaction at E(7Li) = 44.0 MeV was measured at the HI-13 tandem accelerator of Beijing, China. Asymptotic normalization coefficient (ANC) of 13N = 12C + p was derived to be 1.64 $\pm$ 0.11 fm$^{-1/2}$ through distorted wave Born approximation (DWBA) analysis. The ANC was then used to deduce the astrophysical $S(E)$ factors and reaction rates for direct capture in 12C(p,g)13N at energies of astrophysical relevance., Comment: 13 pages, 4 figues, submitted to Nucl. Phys. A

Published
2009

9. Updated reaction rate of Mg25(p,γ)Al26 and its astrophysical implication

Author

Zhang, H., primary, Su, J., additional, Li, Z. H., additional, Li, Y. J., additional, Li, E. T., additional, Chen, C., additional, He, J. J., additional, Shen, Y. P., additional, Lian, G., additional, Guo, B., additional, Li, X. Y., additional, Zhang, L. Y., additional, Sheng, Y. D., additional, Chen, Y. J., additional, Wang, L. H., additional, Zhang, L., additional, Cao, F. Q., additional, Nan, W., additional, Nan, W. K., additional, Li, G. X., additional, Song, N., additional, Cui, B. Q., additional, Chen, L. H., additional, Ma, R. G., additional, Zhang, Z. C., additional, Jiao, T. Y., additional, Gao, B. S., additional, Tang, X. D., additional, Wu, Q., additional, Li, J. Q., additional, Sun, L. T., additional, Wang, S., additional, Yan, S. Q., additional, Liao, J. H., additional, Wang, Y. B., additional, Zeng, S., additional, Nan, D., additional, Fan, Q. W., additional, and Liu, W. P., additional

Published
2023
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10. Measurement of the Tb159(n,γ) cross section at the CSNS Back-n facility

Author

Zhang, S., primary, Li, G., additional, Jiang, W., additional, Wang, D. X., additional, Ren, J., additional, Huang, M., additional, Li, E. T., additional, Tang, J. Y., additional, Ruan, X. C., additional, Wang, H. W., additional, Li, Z. H., additional, Chen, Y. S., additional, Liu, L. X., additional, Li, X. X., additional, Fan, Q. W., additional, Fan, R. R., additional, Hu, X. R., additional, Wang, J. C., additional, Li, X., additional, Niu, D. D., additional, Song, N., additional, and Gu, M., additional

Published
2023
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11. Astrophysical N15(n,γ)N16 reaction rate from precision measurement of the N15(d,p)N16 angular distributions

Author

Li, X. Y., primary, Guo, B., additional, Li, Z. H., additional, Li, Y. J., additional, Su, J., additional, Pang, D. Y., additional, He, J. J., additional, Yan, S. Q., additional, Fan, Q. W., additional, Liu, J. C., additional, Gan, L., additional, Han, Z. Y., additional, Li, E. T., additional, Lian, G., additional, Shen, Y. P., additional, Wang, Y. B., additional, Zeng, S., additional, and Liu, W. P., additional

Published
2022
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12. Fast-timing lifetime measurements of the 33/2+ and 25/2- states in 189Hg: oblate excitations

Author

Zheng, Yun, primary, Li, Congbo, additional, Wu, Xiaoguang, additional, Ma, H L, additional, Zhu, L H, additional, Li, T X, additional, Huang, Z Y, additional, Chen, H, additional, He, C Y, additional, Fan, Q W, additional, Li, Guangsheng, additional, Chen, Q M, additional, Zhong, J, additional, Hu, S P, additional, Li, Hongwei, additional, Wang, Jing-Long, additional, Liu, J J, additional, Wu, Y H, additional, and Luo, P W, additional

Published
2022
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13. The 59Fe (n,γ) 60Fe Cross Section from the Surrogate Ratio Method and Its Effect on the 60Fe Nucleosynthesis

Author

Yan, S. Q., primary, Li, X. Y., additional, Nishio, K., additional, Lugaro, M., additional, Li, Z. H., additional, Makii, H., additional, Pignatari, M., additional, Wang, Y. B., additional, Orlandi, R., additional, Hirose, K., additional, Tsukada, K., additional, Mohr, P., additional, Li, G. S., additional, Wang, J. G., additional, Gao, B. S., additional, Han, Y. L., additional, Guo, B., additional, Li, Y. J., additional, Shen, Y. P., additional, Sato, T. K., additional, Ito, Y., additional, Suzaki, F., additional, Su, J., additional, Yang, Y. Y., additional, Wang, J. S., additional, Ma, J. B., additional, Ma, P., additional, Bai, Z., additional, Xu, S. W., additional, Ren, J., additional, Fan, Q. W., additional, Zeng, S., additional, Han, Z. Y., additional, Nan, W., additional, Nan, W. K., additional, Chen, C., additional, Lian, G., additional, Hu, Q., additional, Duan, F. F., additional, Jin, S. Y., additional, Tang, X. D., additional, and Liu, W. P., additional

Published
2021
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14. The $^{59}$Fe(n, ��)$^{60}$Fe Cross Section from the Surrogate Ratio Method and Its Effect on the $^{60}$Fe Nucleosynthesis

Author

Yan, S. Q., Li, X. Y., Nishio, K., Lugaro, M., Li, Z. H., Makii, H., Pignatari, M., Wang, Y. B., Orlandi, R., Hirose, K., Tsukada, K., Mohr, P., Li, G. S., Wang, J. G., Gao, B. S., Han, Y. L., Guo, B., Li, Y. J., Shen, Y. P., Sato, T. K., Ito, Y., Suzaki, F., Su, J., Yang, Y. Y., Wang, J. S., Ma, J. B., Ma, P., Bai, Z., Xu, S. W., Ren, J., Fan, Q. W., Zeng, S., Han, Z. Y., Nan, W., Nan, W. K., Chen, C., Lian, G., Hu, Q., Duan, F. F., Jin, S. Y., Tang, X. D., and Liu, W. P.

Subjects
Astrophysics of Galaxies (astro-ph.GA), FOS: Physical sciences
Abstract

The long-lived $^{60}$Fe (with a half-life of 2.62 Myr) is a crucial diagnostic of active nucleosynthesis in the Milky Way galaxy and in supernovae near the solar system. The neutron-capture reaction $^{59}$Fe(n,$��$)$^{60}$Fe on $^{59}$Fe (half-life = 44.5 days) is the key reaction for the production of $^{60}$Fe in massive stars. This reaction cross section has been previously constrained by the Coulomb dissociation experiment, which offered partial constraint on the $E$1 $��$-ray strength function but a negligible constraint on the $M$1 and $E$2 components. In this work, for the first time, we use the surrogate ratio method to experimentally determine the $^{59}$Fe(n,$��$)$^{60}$Fe cross sections in which all the components are included. We derived a Maxwellian-averaged cross section of 27.5 $\pm$ 3.5 mb at $kT$= 30 keV and 13.4 $\pm$ 1.7 mb at $kT$= 90 keV, roughly 10 - 20% higher than previous estimates. We analyzed the impact of our new reaction rates in nucleosynthesis models of massive stars and found that uncertainties in the production of $^{60}$Fe from the $^{59}$Fe(n,$��$)$^{60}$Fe rate are at most of 25%. We conclude that stellar physics uncertainties now play a major role in the accurate evaluation of the stellar production of $^{60}$Fe., 9 pages with 6 figures

Published
2021
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17. Fast-timing lifetime measurements of the 33/2 + and 25/2 âˆ' states in 189 Hg: oblate excitations.

Author

Zheng, Y, Li, C B, Wu, X G, Ma, H L, Zhu, L H, Li, T X, Huang, Z Y, Chen, H, He, C Y, Fan, Q W, Li, G S, Chen, Q M, Zhong, J, Hu, S P, Li, H W, Wang, J L, Liu, J J, Wu, Y H, and Luo, P W

Subjects
QUADRUPOLE moments, MERCURY isotopes, MERCURY, MEASUREMENT
Abstract

The lifetimes of the I Ď€ = 33/2+ and I Ď€ = 25/2âˆ' states with E x = 2674.6 keV and E x = 1917.3 keV, respectively, in 189Hg have been determined by using the fast-timing techniques with the HPGe and LaBr3:Ce array via the 175Lu(19F, 5 n)189Hg reaction at a beam energy of 100 MeV. The deduced B (E 2) strengths have been discussed in relation to the systematics of the previously reported B (E 2) strengths in the heavy mercury isotopes. The transition quadrupole moments Q t are derived from present experimental data. The Q t values together with the excitation energies of the (+, 0)(+, 1/2) and (+, 0)(âˆ', 1/2) bands are interpreted in terms of the Nilssonâ€"Strutinskyâ€"Bogoliubov model (CNSB) calculations suggesting oblate excitations in 189Hg. [ABSTRACT FROM AUTHOR]

Published
2022
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19. Constraining the External Capture to the O16 Ground State and the E2 S Factor of the C12(α,γ)O16 Reaction

Author

Shen, Y. P., primary, Guo, B., additional, deBoer, R. J., additional, Li, Z. H., additional, Li, Y. J., additional, Tang, X. D., additional, Pang, D. Y., additional, Adhikari, S., additional, Basu, C., additional, Su, J., additional, Yan, S. Q., additional, Fan, Q. W., additional, Liu, J. C., additional, Chen, C., additional, Han, Z. Y., additional, Li, X. Y., additional, Lian, G., additional, Ma, T. L., additional, Nan, W., additional, Nan, W. K., additional, Wang, Y. B., additional, Zeng, S., additional, Zhang, H., additional, and Liu, W. P., additional

Published
2020
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20. Astrophysical SE2 factor of the C12(α,γ)O16 reaction through the C12(B11,Li7)O16 transfer reaction

Author

Shen, Y. P., primary, Guo, B., additional, Li, Z. H., additional, Li, Y. J., additional, Pang, D. Y., additional, Adhikari, S., additional, An, Z. D., additional, Su, J., additional, Yan, S. Q., additional, Du, X. C., additional, Fan, Q. W., additional, Gan, L., additional, Han, Z. Y., additional, Li, D. H., additional, Li, E. T., additional, Li, X. Y., additional, Lian, G., additional, Liu, J. C., additional, Ma, T. L., additional, Pei, C. J., additional, Su, Y., additional, Wang, Y. B., additional, Zeng, S., additional, Zhou, Y., additional, and Liu, W. P., additional

Published
2019
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24. Radii of the bound states in 16 N from the asymptotic normalization coefficients

Author

Li, E. T., primary, Guo, B., additional, Li, Z. H., additional, Wang, Y. B., additional, Li, Y. J., additional, Wu, Z. D., additional, Su, J., additional, Pang, D. Y., additional, Bai, X. X., additional, Du, X. C., additional, Fan, Q. W., additional, Gan, L., additional, Han, Z. Y., additional, Hao, X., additional, Hu, S. P., additional, He, J. J., additional, Jing, L., additional, Jin, S. J., additional, Li, L., additional, Li, X. Y., additional, Li, Z. C., additional, Lian, G., additional, Liu, J. C., additional, Luo, Q., additional, Qiao, L. H., additional, Shen, Y. P., additional, Sun, H. B., additional, Yan, S. Q., additional, Yu, X. Q., additional, Zeng, S., additional, Zhang, D. H., additional, Zhang, L. Y., additional, Zhang, W. J., additional, Zhou, Y., additional, and Liu, W. P., additional

Published
2016
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25. Spectroscopic factors for low-lying 16N levels and the astrophysical 15N(n,gamma)16N reaction rate

Author

Guo, B., Li, Z. H., Li, Y. J., Su, J., Pang, D. Y., Yan, S. Q., Wu, Z. D., Li, E. T., Bai, X. X., Du, X. C., Fan, Q. W., Gan, L., He, J. J., Jin, S. J., Jing, L., Li, L., Li, Z. C., Lian, G., Liu, J. C., Shen, Y. P., Wang, Y. B., Yu, X. Q., Zeng, S., Zhang, L. Y., Zhang, W. J., and Liu, W. P.

Subjects
FOS: Physical sciences, Nuclear Experiment (nucl-ex), Nuclear Experiment
Abstract

Fluorine is a key element for nucleosynthetic studies since it is extremely sensitive to the physical conditions within stars. The astrophysical site to produce fluorine is suggested to be asymptotic giant branch (AGB) stars. In these stars the 15N(n, g)16N reaction could affect the abundance of fluorine by competing with 15N(a, g)19F. The 15N(n, g)16N reaction rate depends directly on the neutron spectroscopic factors of the low-lying states in 16N. The angular distributions of the 15N(7Li, 6Li)16N reaction populating the ground state and the first three excited states in 16N are measured using a Q3D magnetic spectrograph and are used to derive the spectroscopic factors of these states based on distorted wave Born approximation (DWBA) analysis. The spectroscopic factors of these four states are extracted to be 0.96+-0.09, 0.69+-0.09, 0.84+-0.08 and 0.65+-0.08, respectively. Based on the new spectroscopic factors we derive the 15N(n,g)16N reaction rate. The accuracy and precision of the spectroscopic factors are enhanced due to the first application of high-precision magnetic spectrograph for resolving the closely-spaced 16N levels which can not be achieved in most recent measurement. The present result demonstrates that two levels corresponding to neutron transfers to the 2s1/2 orbit in 16N are not so good single-particle levels although 15N is a closed neutron-shell nucleus. This finding is contrary to the shell model expectation. The present work also provides an independent examination to shed some light on the existing discrepancies in the spectroscopic factors and the 15N(n, g)16N rate., Comment: 13 pages, 4 figures, 2 tables

Published
2014
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27. Guidelines for the use and interpretation of assays for monitoring autophagy

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Klionsky, D.J. Abdalla, F.C. Abeliovich, H. Abraham, R.T. Acevedo-Arozena, A. Adeli, K. Agholme, L. Agnello, M. Agostinis, P. Aguirre-Ghiso, J.A. Ahn, H.J. Ait-Mohamed, O. Ait-Si-Ali, S. Akematsu, T. Akira, S. Al-Younes, H.M. Al-Zeer, M.A. Albert, M.L. Albin, R.L. Alegre-Abarrategui, J. Aleo, M.F. Alirezaei, M. Almasan, A. Almonte-Becerril, M. Amano, A. Amaravadi, R. Amarnath, S. Amer, A.O. Andrieu-Abadie, N. Anantharam, V. Ann, D.K. Anoopkumar-Dukie, S. Aoki, H. Apostolova, N. Arancia, G. Aris, J.P. Asanuma, K. Asare, N.Y.O. Ashida, H. Askanas, V. Askew, D.S. Auberger, P. Baba, M. Backues, S.K. Baehrecke, E.H. Bahr, B.A. Bai, X.-Y. Bailly, Y. Baiocchi, R. Baldini, G. Balduini, W. Ballabio, A. Bamber, B.A. Bampton, E.T.W. Bánhegyi, G. Bartholomew, C.R. Bassham, D.C. Bast Jr., R.C. Batoko, H. Bay, B.-H. Beau, I. Béchet, D.M. Begley, T.J. Behl, C. Behrends, C. Bekri, S. Bellaire, B. Bendall, L.J. Benetti, L. Berliocchi, L. Bernardi, H. Bernassola, F. Besteiro, S. Bhatia-Kissova, I. 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Wu, W.K.K. Wyttenbach, A. Xavier, R.J. Xi, Z. Xia, P. Xiao, G. Xie, Z. Xie, Z. Xu, D.-Z. Xu, J. Xu, L. Xu, X. Yamamoto, A. Yamamoto, A. Yamashina, S. Yamashita, M. Yan, X. Yanagida, M. Yang, D.-S. Yang, E. Yang, J.-M. Yang, S.Y. Yang, W. Yang, W.Y. Yang, Z. Yao, M.-C. Yao, T.-P. Yeganeh, B. Yen, W.-L. Yin, J.-J. Yin, X.-M. Yoo, O.-J. Yoon, G. Yoon, S.-Y. Yorimitsu, T. Yoshikawa, Y. Yoshimori, T. Yoshimoto, K. You, H.J. Youle, R.J. Younes, A. Yu, L. Yu, L. Yu, S.-W. Yu, W.H. Yuan, Z.-M. Yue, Z. Yun, C.-H. Yuzaki, M. Zabirnyk, O. Silva-Zacarin, E. David Zacks, E. Zacksenhaus, L. Zaffaroni, N. Zakeri, Z. Zeh III, H.J. Zeitlin, S.O. Zhang, H. Zhang, H.-L. Zhang, J. Zhang, J.-P. Zhang, L. Zhang, L. Zhang, M.-Y. Zhang, X.D. Zhao, M. Zhao, Y.-F. Zhao, Y. Zhao, Z.J. Zheng, X. Zhivotovsky, B. Zhong, Q. Zhou, C.-Z. Zhu, C. Zhu, W.-G. Zhu, X.-F. Zhu, X. Zhu, Y. Zoladek, T. Zong, W.-X. Zorzano, A. Zschocke, J. Zuckerbraun, B.

Abstract

In 2008 we published the first set of guidelines for standardizing research in autophagy. Since then, research on this topic has continued to accelerate, and many new scientists have entered the field. Our knowledge base and relevant new technologies have also been expanding. Accordingly, it is important to update these guidelines for monitoring autophagy in different organisms. Various reviews have described the range of assays that have been used for this purpose. Nevertheless, there continues to be confusion regarding acceptable methods to measure autophagy, especially in multicellular eukaryotes. A key point that needs to be emphasized is that there is a difference between measurements that monitor the numbers or volume of autophagic elements (e.g., autophagosomes or autolysosomes) at any stage of the autophagic process vs. those that measure flux through the autophagy pathway (i.e., the complete process); thus, a block in macroautophagy that results in autophagosome accumulation needs to be differentiated from stimuli that result in increased autophagic activity, defined as increased autophagy induction coupled with increased delivery to, and degradation within, lysosomes (in most higher eukaryotes and some protists such as Dictyostelium) or the vacuole (in plants and fungi). In other words, it is especially important that investigators new to the field understand that the appearance of more autophagosomes does not necessarily equate with more autophagy. In fact, in many cases, autophagosomes accumulate because of a block in trafficking to lysosomes without a concomitant change in autophagosome biogenesis, whereas an increase in autolysosomes may reflect a reduction in degradative activity. Here, we present a set of guidelines for the selection and interpretation of methods for use by investigators who aim to examine macroautophagy and related processes, as well as for reviewers who need to provide realistic and reasonable critiques of papers that are focused on these processes. These guidelines are not meant to be a formulaic set of rules, because the appropriate assays depend in part on the question being asked and the system being used. In addition, we emphasize that no individual assay is guaranteed to be the most appropriate one in every situation, and we strongly recommend the use of multiple assays to monitor autophagy. In these guidelines, we consider these various methods of assessing autophagy and what information can, or cannot, be obtained from them. Finally, by discussing the merits and limits of particular autophagy assays, we hope to encourage technical innovation in the field. © 2012 Landes Bioscience.

Published
2012

28. Proton spectroscopic factor of the12Cground state from the12C(11B,12C)11Belastic transfer reaction

Author

Li, E. T., primary, Li, Z. H., additional, Li, Y. J., additional, Guo, B., additional, Wang, Y. B., additional, Pang, D. Y., additional, Su, J., additional, Yan, S. Q., additional, Zeng, S., additional, Gan, L., additional, Li, Z. C., additional, Liu, J. C., additional, Bai, X. X., additional, Wu, Z. D., additional, Jin, S. J., additional, Zhang, L. Y., additional, Yu, X. Q., additional, Li, L., additional, Sun, H. B., additional, Lian, G., additional, Fan, Q. W., additional, and Liu, W. P., additional

Published
2014
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31. Astrophysical SE2 factor of the 12C(α, γ)16O reaction through the 12C(11B, 7Li)16O transfer reaction.

Author

Guo, B., Du, X. C., Li, Z. H., Li, Y. J., Pang, D. Y., Su, J., Yan, S. Q., Fan, Q. W., Gan, L., Han, Z. Y., Li, E. T., Li, X. Y., Lian, G., Liu, J. C., Pei, C. J., Qiao, L. H., Shen, Y. P., Su, Y., Wang, Y. B., and Zeng, S.

Subjects
CARBON isotopes, OXYGEN isotopes, ANGULAR distribution (Nuclear physics), POTENTIAL barrier, MAGNETIC spectrometer, NUCLEAR astrophysics, TANDEM accelerators
Abstract

The 12C(α, γ)16O reaction plays a key role in the evolution of stars with masses of M > 0.55 M⊙. At the Gamow peak (Ec.m. = 300 keV, T9 = 0.2), the cross section of the 12C(α, γ)16O reaction is so small (about 10-17 barn) that the direct measurement in ground laboratory is not feasible with the existing technology. Up to now, the cross sections at lower energies can only be extrapolated from the data at higher energies. However, two subthreshold resonances, locating at Ex = 7.117 MeV and Ex = 6.917 MeV, make this extrapolation more complicated. In this work the 6.917 MeV subthreshold resonance in the 12C(α, γ)16O reaction was investigated via the 12C(11B,7Li)16O reaction. The experiment was performed using the Q3D magnetic spectrograph at HI-13 tandem accelerator. We measured the angular distribution of the 12C(11B,7Li)16O transfer reaction leading to the 6.917 MeV state. Based on DWBA analysis, we derived the square of ANC of the 6.917 MeV level in 16O to be (2.45 ± 0.28) x1010 fm-1, with which the reduced-α width can be computed. Finally, we calculated the astrophysical SE2 factor of the 6.917 MeV resonance to be 67.6 ± 7.7 keV b. [ABSTRACT FROM AUTHOR]

Published
2016
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32. MTOR KINASE INHIBITORS AND APOPTOSIS IN GLIOBLASTOMA

Author

Weiss, W. A., primary, Wong, R., additional, Fan, Q.-W., additional, Ilkhanizadeh, S., additional, Lu, M., additional, Beyer, J., additional, Dube, N., additional, Forsayeth, J., additional, Kells, A., additional, Xu, T., additional, Bankiewicz, K., additional, Ducker, G., additional, Feldman, M., additional, and Shokat, K., additional

Published
2014
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33. Proton widths of the low-lying16Fstates from the15N(7Li,6Li)16Nreaction

Author

Wu, Z. D., primary, Guo, B., additional, Li, Z. H., additional, Li, Y. J., additional, Su, J., additional, Pang, D. Y., additional, Yan, S. Q., additional, Li, E. T., additional, Bai, X. X., additional, Du, X. C., additional, Fan, Q. W., additional, Gan, L., additional, He, J. J., additional, Jin, S. J., additional, Jing, L., additional, Li, L., additional, Li, Z. C., additional, Lian, G., additional, Liu, J. C., additional, Shen, Y. P., additional, Wang, Y. B., additional, Yu, X. Q., additional, Zeng, S., additional, Zhang, D. H., additional, Zhang, L. Y., additional, Zhang, W. J., additional, and Liu, W. P., additional

Published
2014
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34. Spectroscopic factors for low-lyingN16levels and the astrophysicalN15(n,γ)N16reaction rate

Author

Guo, B., primary, Li, Z. H., additional, Li, Y. J., additional, Su, J., additional, Pang, D. Y., additional, Yan, S. Q., additional, Wu, Z. D., additional, Li, E. T., additional, Bai, X. X., additional, Du, X. C., additional, Fan, Q. W., additional, Gan, L., additional, He, J. J., additional, Jin, S. J., additional, Jing, L., additional, Li, L., additional, Li, Z. C., additional, Lian, G., additional, Liu, J. C., additional, Shen, Y. P., additional, Wang, Y. B., additional, Yu, X. Q., additional, Zeng, S., additional, Zhang, L. Y., additional, Zhang, W. J., additional, and Liu, W. P., additional

Published
2014
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36. CELL BIOLOGY AND SIGNALING

Author

Agarwal, M., primary, Nitta, R., additional, Dovat, S., additional, Li, G., additional, Arita, H., additional, Narita, Y., additional, Fukushima, S., additional, Tateishi, K., additional, Matsushita, Y., additional, Yoshida, A., additional, Miyakita, Y., additional, Ohno, M., additional, Collins, V. P., additional, Kawahara, N., additional, Shibui, S., additional, Ichimura, K., additional, Kahn, S. A., additional, Gholamin, S., additional, Junier, M.-P., additional, Chneiweiss, H., additional, Weissman, I., additional, Mitra, S., additional, Cheshier, S., additional, Avril, T., additional, Hamlat, A., additional, Le Reste, P.-J., additional, Mosser, J., additional, Quillien, V., additional, Carrato, C., additional, Munoz-Marmol, A., additional, Serrano, L., additional, Pijuan, L., additional, Hostalot, C., additional, Villa, S. l., additional, Ariza, A., additional, Etxaniz, O., additional, Balana, C., additional, Benveniste, E. T., additional, Zheng, Y., additional, McFarland, B., additional, Drygin, D., additional, Bellis, S., additional, Bredel, M., additional, Lotsch, D., additional, Engelmaier, C., additional, Allerstorfer, S., additional, Grusch, M., additional, Pichler, J., additional, Weis, S., additional, Hainfellner, J., additional, Marosi, C., additional, Spiegl-Kreinecker, S., additional, Berger, W., additional, Bronisz, A., additional, Nowicki, M. O., additional, Wang, Y., additional, Ansari, K., additional, Chiocca, E. A., additional, Godlewski, J., additional, Brown, K., additional, Kwatra, M., additional, Bui, T., additional, Zhu, S., additional, Kozono, D., additional, Li, J., additional, Kushwaha, D., additional, Carter, B., additional, Chen, C., additional, Schulte, J., additional, Srikanth, M., additional, Das, S., additional, Zhang, J., additional, Lathia, J., additional, Yin, L., additional, Rich, J., additional, Olson, E., additional, Kessler, J., additional, Chenn, A., additional, Cherry, A., additional, Haas, B., additional, Lin, Y. H., additional, Ong, S.-E., additional, Stella, N., additional, Cifarelli, C. P., additional, Griffin, R. J., additional, Cong, D., additional, Zhu, W., additional, Shi, Y., additional, Clark, P., additional, Kuo, J., additional, Hu, S., additional, Sun, D., additional, Bookland, M., additional, Darbinian, N., additional, Dey, A., additional, Robitaille, M., additional, Remke, M., additional, Faury, D., additional, Maier, C., additional, Malhotra, A., additional, Jabado, N., additional, Taylor, M., additional, Angers, S., additional, Kenney, A., additional, Ren, X., additional, Zhou, H., additional, Schur, M., additional, Baweja, A., additional, Singh, M., additional, Erdreich-Epstein, A., additional, Fu, J., additional, Koul, D., additional, Yao, J., additional, Saito, N., additional, Zheng, S., additional, Verhaak, R., additional, Lu, Z., additional, Yung, W. K. A., additional, Gomez, G., additional, Volinia, S., additional, Croce, C., additional, Brennan, C., additional, Cavenee, W., additional, Furnari, F., additional, Lopez, S. G., additional, Qu, D., additional, Petritsch, C., additional, Gonzalez-Huarriz, M., additional, Aldave, G., additional, Ravi, D., additional, Rubio, A., additional, Diez-Valle, R., additional, Marigil, M., additional, Jauregi, P., additional, Vera, B., additional, Rocha, A. A. d. l., additional, Tejada-Solis, S., additional, Alonso, M. M., additional, Gopal, U., additional, Isaacs, J., additional, Gruber-Olipitz, M., additional, Dabral, S., additional, Ramkissoon, S., additional, Kung, A., additional, Pak, E., additional, Chung, J., additional, Theisen, M., additional, Sun, Y., additional, Monrose, V., additional, Franchetti, Y., additional, Shulman, D., additional, Redjal, N., additional, Tabak, B., additional, Beroukhim, R., additional, Zhao, J., additional, Buonamici, S., additional, Ligon, K., additional, Kelleher, J., additional, Segal, R., additional, Canton, D., additional, Diaz, P., additional, Scott, J., additional, Hara, K., additional, Kageji, T., additional, Mizobuchi, Y., additional, Kitazato, K., additional, Okazaki, T., additional, Fujihara, T., additional, Nakajima, K., additional, Mure, H., additional, Kuwayama, K., additional, Hara, T., additional, Nagahiro, S., additional, Hill, L., additional, Botfield, H., additional, Hossain-Ibrahim, K., additional, Logan, A., additional, Cruickshank, G., additional, Liu, Y., additional, Gilbert, M., additional, Kyprianou, N., additional, Rangnekar, V., additional, Horbinski, C., additional, Hu, Y., additional, Vo, C., additional, Li, Z., additional, Ke, C., additional, Ru, N., additional, Hess, K. R., additional, Linskey, M. E., additional, Zhou, Y.-a. H., additional, Hu, F., additional, Vinnakota, K., additional, Wolf, S., additional, Kettenmann, H., additional, Jackson, P. J., additional, Larson, J. D., additional, Beckmann, D. A., additional, Moriarity, B. S., additional, Largaespada, D. A., additional, Jalali, S., additional, Agnihotri, S., additional, Singh, S., additional, Burrell, K., additional, Croul, S., additional, Zadeh, G., additional, Kang, S.-H., additional, Yu, M. O., additional, Song, N.-H., additional, Park, K.-J., additional, Chi, S.-G., additional, Chung, Y.-G., additional, Kim, S. K., additional, Kim, J. W., additional, Kim, J. Y., additional, Kim, J. E., additional, Choi, S. H., additional, Kim, T. M., additional, Lee, S.-H., additional, Kim, S.-K., additional, Park, S.-H., additional, Kim, I. H., additional, Park, C.-K., additional, Jung, H.-W., additional, Koldobskiy, M., additional, Ahmed, I., additional, Ho, G., additional, Snowman, A., additional, Raabe, E., additional, Eberhart, C., additional, Snyder, S., additional, Gugel, I., additional, Bornemann, A., additional, Pantazis, G., additional, Mack, S., additional, Shih, D., additional, Sabha, N., additional, Tatagiba, M., additional, Krischek, B., additional, Schulte, A., additional, Liffers, K., additional, Kathagen, A., additional, Riethdorf, S., additional, Westphal, M., additional, Lamszus, K., additional, Lee, J. S., additional, Xiao, J., additional, Patel, P., additional, Schade, J., additional, Wang, J., additional, Deneen, B., additional, Song, H.-R., additional, Leiss, L., additional, Gjerde, C., additional, Saed, H., additional, Rahman, A., additional, Lellahi, M., additional, Enger, P. O., additional, Leung, R., additional, Gil, O., additional, Lei, L., additional, Canoll, P., additional, Sun, S., additional, Lee, D., additional, Ho, A. S. W., additional, Pu, J. K. S., additional, Zhang, X.-q., additional, Lee, N. P., additional, Dat, P. J. R., additional, Leung, G. K. K., additional, Loetsch, D., additional, Steiner, E., additional, Holzmann, K., additional, Pirker, C., additional, Hlavaty, J., additional, Petznek, H., additional, Hegedus, B., additional, Garay, T., additional, Mohr, T., additional, Sommergruber, W., additional, Lukiw, W. J., additional, Jones, B. M., additional, Zhao, Y., additional, Bhattacharjee, S., additional, Culicchia, F., additional, Magnus, N., additional, Garnier, D., additional, Meehan, B., additional, McGraw, S., additional, Hashemi, M., additional, Lee, T. H., additional, Milsom, C., additional, Gerges, N., additional, Trasler, J., additional, Pawlinski, R., additional, Mackman, N., additional, Rak, J., additional, Maherally, Z., additional, Thorne, A., additional, An, Q., additional, Barbu, E., additional, Fillmore, H., additional, Pilkington, G., additional, Tan, S. L., additional, Tan, S., additional, Choi, S., additional, Potts, C., additional, Ford, D. A., additional, Nahle, Z., additional, Kenney, A. M., additional, Matlaf, L., additional, Khan, S., additional, Zider, A., additional, Singer, E., additional, Cobbs, C., additional, Soroceanu, L., additional, McFarland, B. C., additional, Hong, S. W., additional, Rajbhandari, R., additional, Twitty, G. B., additional, Gray, G. K., additional, Yu, H., additional, Benveniste, E. N., additional, Nozell, S. E., additional, Minata, M., additional, Kim, S., additional, Mao, P., additional, Kaushal, J., additional, Nakano, I., additional, Mizowaki, T., additional, Sasayama, T., additional, Tanaka, K., additional, Mizukawa, K., additional, Nishihara, M., additional, Nakamizo, S., additional, Tanaka, H., additional, Kohta, M., additional, Hosoda, K., additional, Kohmura, E., additional, Moeckel, S., additional, Meyer, K., additional, Leukel, P., additional, Bogdahn, U., additional, Riehmenschneider, M. J., additional, Bosserhoff, A. K., additional, Spang, R., additional, Hau, P., additional, Mukasa, A., additional, Watanabe, A., additional, Ogiwara, H., additional, Aburatani, H., additional, Mukherjee, J., additional, Obha, S., additional, See, W., additional, Pieper, R., additional, Otsuka, R., additional, Kung, D., additional, Sinha, T., additional, Meares, G., additional, Nozell, S., additional, Ott, M., additional, Litzenburger, U., additional, Rauschenbach, K., additional, Bunse, L., additional, Pusch, S., additional, Ochs, K., additional, Sahm, F., additional, Opitz, C., additional, von Deimling, A., additional, Wick, W., additional, Platten, M., additional, Peruzzi, P., additional, Read, R., additional, Fenton, T., additional, Wykosky, J., additional, Vandenberg, S., additional, Babic, I., additional, Iwanami, A., additional, Yang, H., additional, Mischel, P., additional, Thomas, J., additional, Ronellenfitsch, M. W., additional, Thiepold, A. L., additional, Harter, P. N., additional, Mittelbronn, M., additional, Steinbach, J. P., additional, Rybakova, Y., additional, Kalen, A., additional, Sarsour, E., additional, Goswami, P., additional, Silber, J., additional, Harinath, G., additional, Aldaz, B., additional, Fabius, A. W. M., additional, Turcan, S., additional, Chan, T. A., additional, Huse, J. T., additional, Sonabend, A. M., additional, Bansal, M., additional, Guarnieri, P., additional, Soderquist, C., additional, Yun, J., additional, Kennedy, B., additional, Sisti, J., additional, Bruce, S., additional, Bruce, R., additional, Shakya, R., additional, Ludwig, T., additional, Rosenfeld, S., additional, Sims, P. A., additional, Bruce, J. N., additional, Califano, A., additional, Stockhausen, M.-T., additional, Kristoffersen, K., additional, Olsen, L. S., additional, Poulsen, H. S., additional, Stringer, B., additional, Day, B., additional, Barry, G., additional, Piper, M., additional, Jamieson, P., additional, Ensbey, K., additional, Bruce, Z., additional, Richards, L., additional, Boyd, A., additional, Sufit, A., additional, Burleson, T., additional, Le, J. P., additional, Keating, A. K., additional, Sundstrom, T., additional, Varughese, J. K., additional, Harter, P., additional, Prestegarden, L., additional, Petersen, K., additional, Azuaje, F., additional, Tepper, C., additional, Ingham, E., additional, Even, L., additional, Johnson, S., additional, Skaftnesmo, K. O., additional, Lund-Johansen, M., additional, Bjerkvig, R., additional, Ferrara, K., additional, Thorsen, F., additional, Takeshima, H., additional, Yamashita, S., additional, Yokogami, K., additional, Mizuguchi, S., additional, Nakamura, H., additional, Kuratsu, J., additional, Fukushima, T., additional, Morishita, K., additional, Tang, Y., additional, Vaka, D., additional, Chen, S., additional, Ponnuswami, A., additional, Cho, Y.-J., additional, Monje, M., additional, Nakamura, T., additional, Cahill, D., additional, Tiemann, K., additional, Hedman, H., additional, Niclou, S. P., additional, Timmer, M., additional, Tjiong, R., additional, Rohn, G., additional, Goldbrunner, R., additional, Stavrinou, P., additional, Perrech, M., additional, Tokita, M., additional, Mikheev, S., additional, Sellers, D., additional, Mikheev, A., additional, Kosai, Y., additional, Rostomily, R., additional, Tritschler, I., additional, Seystahl, K., additional, Schroeder, J. J., additional, Weller, M., additional, Wade, A., additional, Robinson, A. E., additional, Phillips, J. J., additional, Gong, Y., additional, Ma, Y., additional, Cheng, Z., additional, Thompson, R., additional, Fan, Q.-W., additional, Cheng, C., additional, Gustafson, W., additional, Charron, E., additional, Zipper, P., additional, Wong, R., additional, Chen, J., additional, Lau, J., additional, Knobbe-Thosen, C., additional, Jura, N., additional, Reifenberger, G., additional, Shokat, K., additional, Weiss, W., additional, Wu, S., additional, Hu, J., additional, Taylor, T., additional, Villa, G. R., additional, Mischel, P. S., additional, Gonias, S. L., additional, Yamashita, D., additional, Kondo, T., additional, Takahashi, H., additional, Inoue, A., additional, Kohno, S., additional, Harada, H., additional, Ohue, S., additional, Ohnishi, T., additional, Li, P., additional, Ng, J., additional, Yuelling, L., additional, Du, F., additional, Curran, T., additional, Yang, Z.-j., additional, Zhu, D., additional, Castellino, R. C., additional, Van Meir, E. G., additional, Begum, G., additional, Wang, Q., additional, Yang, S.-S., additional, Lin, S.-H., additional, and Kahle, K., additional

Published
2013
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37. Erratum to: New determination of the astrophysical 13 C( p, $ \gamma$ 14 N S(E) factors and reaction rates via the 13 C( 7 Li, 6 He) 14 N reaction

Author

Li, Y. J., primary, Li, Z. H., additional, Li, E. T., additional, Bai, X. X., additional, Su, J., additional, Guo, B., additional, Wang, B. X., additional, Yan, S. Q., additional, Zeng, S., additional, Li, Z. C., additional, Liu, J. C., additional, Liu, X., additional, Jin, S. J., additional, Wang, Y. B., additional, Zhang, L. Y., additional, Yu, X. Q., additional, Li, L., additional, Lian, G., additional, Fan, Q. W., additional, and Liu, W. P., additional

Published
2013
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38. Erratum: New determination of the proton spectroscopic factor in9Befrom the13C(9Be,8Li)14Nangular distribution [Phys. Rev. C87, 017601 (2013)]

Author

Li, Z. H., primary, Li, Y. J., additional, Su, J., additional, Guo, B., additional, Li, E. T., additional, Dong, K. J., additional, Bai, X. X., additional, Li, Z. C., additional, Liu, J. C., additional, Yan, S. Q., additional, Wang, Y. B., additional, Zeng, S., additional, Lian, G., additional, Wang, B. X., additional, Jin, S. J., additional, Liu, X., additional, Zhang, W. J., additional, Huang, W. Z., additional, Fan, Q. W., additional, Gan, L., additional, Wu, Z. D., additional, and Liu, W. P., additional

Published
2013
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39. New determination of the proton spectroscopic factor in9Be from the13C(9Be,8Li)14N angular distribution

Author

Li, Z. H., primary, Li, Y. J., additional, Su, J., additional, Guo, B., additional, Li, E. T., additional, Dong, K. J., additional, Bai, X. X., additional, Li, Z. C., additional, Liu, J. C., additional, Yan, S. Q., additional, Wang, Y. B., additional, Zeng, S., additional, Lian, G., additional, Wang, B. X., additional, Jin, S. J., additional, Liu, X., additional, Zhang, W. J., additional, Huang, W. Z., additional, Fan, Q. W., additional, Gan, L., additional, Wu, Z. D., additional, and Liu, W. P., additional

Published
2013
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41. NEW DETERMINATION OF THE13C(α,n)16O REACTION RATE AND ITS INFLUENCE ON THEs-PROCESS NUCLEOSYNTHESIS IN AGB STARS

Author

Guo, B., primary, Li, Z. H., additional, Lugaro, M., additional, Buntain, J., additional, Pang, D. Y., additional, Li, Y. J., additional, Su, J., additional, Yan, S. Q., additional, Bai, X. X., additional, Chen, Y. S., additional, Fan, Q. W., additional, Jin, S. J., additional, Karakas, A. I., additional, Li, E. T., additional, Li, Z. C., additional, Lian, G., additional, Liu, J. C., additional, Liu, X., additional, Shi, J. R., additional, Shu, N. C., additional, Wang, B. X., additional, Wang, Y. B., additional, Zeng, S., additional, and Liu, W. P., additional

Published
2012
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43. Pre-clinical Experimental Therapeutics and Pharmacology

Author

Jensen, R. L., primary, Gilliespie, D., additional, Ajewung, N., additional, Faure, R., additional, Kamnasaran, D., additional, Poirier, D., additional, Tamura, K., additional, Wakimoto, H., additional, Rabkin, S. D., additional, Martuza, R. L., additional, Shah, K., additional, Hashizume, R., additional, Aoki, Y., additional, Serwer, L. P., additional, Drummond, D., additional, Noble, C., additional, Park, J., additional, Bankiewicz, K., additional, James, D. C., additional, Gupta, N., additional, Agerholm-Larsen, B., additional, Iversen, H. K., additional, Jensen, K. S., additional, Moller, J., additional, Ibsen, P., additional, Mahmood, F., additional, Gehl, J., additional, Corem, E., additional, Ram, Z., additional, Daniels, D., additional, Last, D., additional, Shneor, R., additional, Salomon, S., additional, Perlstein, B., additional, Margel, S., additional, Mardor, Y., additional, Charest, G., additional, Fortin, D., additional, Mathieu, D., additional, Sanche, L., additional, Paquette, B., additional, Li, H.-F., additional, Hariono, S., additional, Dasgupta, T., additional, Kim, J.-S., additional, Haas-Kogan, D., additional, Weiss, W. A., additional, James, C. D., additional, Waldman, T., additional, Nicolaides, T., additional, Ozawa, T., additional, Rao, S., additional, Sun, H., additional, Ng, C., additional, De La Torre, J., additional, Santos, R., additional, Prados, M., additional, Butowski, N., additional, Michaud, K., additional, Solomon, D. A., additional, Prados, M. D., additional, Pandya, H., additional, Gibo, D., additional, Debinski, W., additional, Vinchon-Petit, S., additional, Jarnet, D., additional, Jadaud, E., additional, Feuvret, L., additional, Garcion, E., additional, Menei, P., additional, Chen, R., additional, Yu, J.-C., additional, Liu, C., additional, Jaffer, Z. M., additional, Chabala, J. C., additional, Winssinger, N., additional, Rubenstein, A. E., additional, Emdad, L., additional, Kothari, H., additional, Qadeer, Z., additional, Binello, E., additional, Germano, I., additional, Hirschberg, H., additional, Baek, S.-K., additional, Kwon, Y. J., additional, Sun, C. H., additional, Li, S. C., additional, Madsen, S., additional, Liu, T., additional, Wang, S.-W., additional, Gibo, D. M., additional, Fan, Q.-W., additional, Cheng, C., additional, Hackett, C., additional, Feldman, M., additional, Houseman, B. T., additional, Oakes, S. A., additional, Debnath, J., additional, Shokat, K. M., additional, Sai, K., additional, Chen, F., additional, Qiu, Z., additional, Mou, Y., additional, Zhang, X., additional, Yang, Q., additional, Chen, Z., additional, Patel, T. R., additional, Zhou, J., additional, Piepmeier, J. M., additional, Saltzman, W. M., additional, Banerjee, S., additional, Kaul, A., additional, Gianino, S. M., additional, Christians, U., additional, Gutmann, D. H., additional, Wu, J., additional, Shen, R., additional, Puduvalli, V., additional, Koul, D., additional, Alfred Yung, W. K., additional, Yun, J., additional, Sonabend, A., additional, Stuart, M., additional, Yanagihara, T., additional, Dashnaw, S., additional, Brown, T., additional, McCormick, P., additional, Romanov, A., additional, Sebastian, M., additional, Canoll, P., additional, Bruce, J. N., additional, Piao, L., additional, Joshi, K., additional, Lee, R. J., additional, Nakano, I., additional, Madsen, S. J., additional, Chou, C. C., additional, Blickenstaff, J. W., additional, Sun, C.-H., additional, Zhou, Y.-H., additional, Tome, C. M. L., additional, Wykosky, J., additional, Palma, E., additional, Nduom, E., additional, Machaidze, R., additional, Kaluzova, M., additional, Wang, Y., additional, Nie, S., additional, Hadjipanayis, C., additional, Saito, R., additional, Nakamura, T., additional, Sonoda, Y., additional, Kumabe, T., additional, Tominaga, T., additional, Lun, X., additional, Zemp, F., additional, Zhou, H., additional, Stechishin, O., additional, Kelly, J. J., additional, Weiss, S., additional, Hamilton, M. G., additional, Cairncross, G., additional, Rabinovich, B. A., additional, Bell, J., additional, McFadden, G., additional, Senger, D. L., additional, Forsyth, P. A., additional, Kang, P., additional, Jane, E. P., additional, Premkumar, D. R., additional, Pollack, I. F., additional, Yoo, J. Y., additional, Haseley, A., additional, Bratasz, A., additional, Powell, K., additional, Chiocca, E. A., additional, Kaur, B., additional, Johns, T. G., additional, Ferruzzi, P., additional, Mennillo, F., additional, De Rosa, A., additional, Rossi, M., additional, Giordano, C., additional, Magrini, R., additional, Benedetti, G., additional, Pericot, G. l., additional, Magnoni, L., additional, Mori, E., additional, Thomas, R., additional, Tunici, P., additional, Bakker, A., additional, Pradarelli, J., additional, Kaka, A., additional, Alvarez-Breckenridge, C., additional, Pan, Q., additional, Teknos, T., additional, Cen, L., additional, Ostrem, J. L., additional, Schroeder, M. A., additional, Mladek, A. C., additional, Fink, S. R., additional, Jenkins, R. B., additional, Sarkaria, J. N., additional, Madhankumar, A. B., additional, Slagle-Webb, B., additional, Park, A., additional, Pang, M., additional, Klinger, M., additional, Harbaugh, K. S., additional, Sheehan, J. M., additional, Connor, J. R., additional, Chen, T. C., additional, Wang, W., additional, Hofman, F. M., additional, Drummond, D. C., additional, Noble, C. O., additional, Park, J. W., additional, Zhou, Y., additional, Marks, J. D., additional, Alonso, M. M., additional, Gomez-Manzano, C., additional, Cortes-Santiago, N., additional, Roche, F. P., additional, Fueyo, J., additional, Johannessen, T.-C. A., additional, Grudic, A., additional, Tysnes, B. B., additional, Nigro, J., additional, Bjerkvig, R., additional, Joshi, A. D., additional, Parsons, W., additional, Velculescu, V. E., additional, Riggins, G. J., additional, Bindra, R. S., additional, Jasin, M., additional, Powell, S. N., additional, Fu, J., additional, Shen, R.-J., additional, Colman, H., additional, Lang, F. F., additional, Jensen, M. R., additional, Friedman, G. K., additional, Haas, M., additional, Cassady, K. A., additional, Gillespie, G. Y., additional, Nguyen, V., additional, Murphy, L. T., additional, Beauchamp, A. S., additional, Hollingsworth, C. K., additional, Mintz, A., additional, Garg, S., additional, Kridel, S., additional, Conrad, C. A., additional, Madden, T., additional, Ji, Y., additional, Priebe, W., additional, Seleverstov, O., additional, Purow, B. W., additional, Grant, G. A., additional, Wilson, C., additional, Campbell, M., additional, Humphries, P., additional, Li, S., additional, Li, J., additional, Johnson, A., additional, Bigner, D., additional, Dewhirst, M., additional, Pokorny, J. L., additional, Kitange, G. J., additional, Carlson, B. L., additional, Suphangul, M., additional, Petro, B., additional, Mukhtar, L., additional, Baig, M. S., additional, Villano, J., additional, Mahmud, N., additional, Keir, S. T., additional, Reardon, D. A., additional, Watson, M., additional, Shore, G. C., additional, Bigner, D. D., additional, Friedman, H. S., additional, and Gururangan, S., additional

Published
2010
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49. Human N-Acetylglucosamine-6-O-Sulfotransferase Involved in the Biosynthesis of 6-Sulfo Sialyl Lewis X: Molecular Cloning, Chromosomal Mapping, and Expression in Various Organs and Tumor Cells

Author

Uchimura, K., primary, Muramatsu, H., additional, Kaname, T., additional, Ogawa, H., additional, Yamakawa, T., additional, Fan, Q.-W., additional, Mitsuoka, C., additional, Kannagi, R., additional, Habuchi, O., additional, Yokoyama, I., additional, Yamamura, K.-i., additional, Ozaki, T., additional, Nakagawara, A., additional, Kadomatsu, K., additional, and Muramatsu, T., additional

Published
1998
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