Zobrazeno 1 - 10
of 618
pro vyhledávání: '"MARCINKOWSKI, R."'
Autor:
Produit, N., Bao, T. W., Batsch, T., Bernasconi, T., Britvich, I., Cadoux, F., Cernuda, I., Chai, J. Y., Dong, Y. W., Gauvin, N., Hajdas, W., Kole, M., Kong, M. N., Kramert, R., Li, L., Liu, J. T., Liu, X., Marcinkowski, R., Orsi, S., Pohl, M., Rapin, D., Rybka, D., Rutczynska, A., Shi, H. L., Socha, P., Sun, J. C., Song, L. M., Szabelski, J., Traseira, I., Xiao, H. L., Wang, R. J., Wen, X., Wu, B. B., Zhang, L., Zhang, L. Y., Zhang, S. N., Zhang, Y. J., Zwolinska, A.
The POLAR detector is a space based Gamma Ray Burst (GRB) polarimeter with a wide field of view, which covers almost half the sky. The instrument uses Compton scattering of gamma rays on a plastic scintillator hodoscope to measure the polarization of
Externí odkaz:
http://arxiv.org/abs/1709.07191
Autor:
Kole, M., Li, Z. H., Produit, N., Tymieniecka, T., Zhang, J., Zwolinska, A., Bao, T. W., Bernasconi, T., Cadoux, F., Feng, M. Z., Gauvin, N., Hajdas, W., Kong, S. W., Li, H. C., Li, L., Liu, X., Marcinkowski, R., Orsi, S., Pohl, M., Rybka, D., Sun, J. C., Song, L. M., Szabelski, J., Wang, R. J., Wang, Y. H., Wen, X., Wu, B. B., Wu, X., Xiao, H. L., Zhang, L., Zhang, L. Y., Zhang, S. N., Zhang, X. F., Zhang, Y. J., Zhao, Y.
POLAR is a new satellite-born detector aiming to measure the polarization of an unprecedented number of Gamma-Ray Bursts in the 50-500 keV energy range. The instrument, launched on-board the Tiangong-2 Chinese Space lab on the 15th of September 2016,
Externí odkaz:
http://arxiv.org/abs/1708.00664
Autor:
Xiao, H. L., Hajdas, W., Socha, P., Marcinkowski, R., Wu, B. B., Bao, T. W., Chai, J. Y., Dong, Y. W., Kong, M. N., Li, L., Li, Z. H., Liu, J. T., Shi, H. L., Song, L. M., Sun, J. C., Wang, R. J., Wang, Y. H., Wen, X., Xiong, S. L., Zhang, J., Zhang, L. Y., Zhang, S. N., Zhang, X. F., Zhang, Y. J., Cadoux, F., Pohl, M., Wu, X., Batsch, T., Rybka, D., Rutczynska, A., Szabelski, J., Zwolinska, A., Gauvin, N., Produit, N., Bernasconi, T.
POLAR is space-borne detector designed for a precise measurement of gamma-ray polarization of the prompt emissions of Gamma-Ray Bursts in the energy range 50 keV - 500 keV. POLAR is a compact Compton polarimeter consisting of 40$\times$ 40 plastic sc
Externí odkaz:
http://arxiv.org/abs/1704.06173
Autor:
Zhang, X. F., Hajdas, W., Xiao, H. L., Wen, X., Wu, B. B., Bao, T. W., Batsch, T., Bernasconi, T., Cadoux, F., Cernuda, I., Chai, J. Y., Dong, Y. W., Gauvin, N., He, J. J., Kole, M., Kong, M. N., Lechanoine-Leluc, C., Li, L., Li, Z. H., Liu, J. T., Liu, X., Marcinkowski, R., Orsi, S., Pohl, M., Rapin, D., Rybka, D., Shi, H. L., Song, L. M., Sun, J. C., Szabelski, J., Wang, R. J., Wang, Y. H., Wu, X., Xiong, S. L., Xu, M., Zhang, L., Zhang, L. Y., Zhang, P., Zhang, S. N., Zhang, Y. J., Zwolinska, A.
As a space-borne detector POLAR is designed to conduct hard X-ray polarization measurements of gamma-ray bursts on the statistically significant sample of events and with an unprecedented accuracy. During its development phase a number of tests, cali
Externí odkaz:
http://arxiv.org/abs/1703.04210
Autor:
Kole, M., Bao, T. W., Batsch, T., Bernasconi, T., Cadoux, F., Chai, J. Y., Dong, Y. W., Gauvin, N., Hajdas, W., He, J. J., Kong, M. N., Kong, S. W., Lechanoine-Leluc, C., Li, L., Li, Z. H., Liu, J. T., Liu, X., Marcinkowski, R., Orsi, S., Pohl, M., Produit, N., Rapin, D., Rutczynska, A., Rybka, D., Shi, H. L., Song, L. M., Sun, J. C., Szabelski, J., Wang, R. J., Wang, Y. J., Wen, X., Wu, B. B., Wu, X., Xiao, H. L., Xiong, S. L., Xu, H. H., Xu, M., Zhang, J., Zhang, L., Zhang, L. Y., Zhang, S. N., Zhang, X. F., Zhang, Y. J., Zwolinska, A.
Publikováno v:
from IEEE NSS/MIC 2016 Conference Record
Gamma-ray polarimetry is a new powerful tool to study the processes responsible for the emission from astrophysical sources and the environments in which this emission takes place. Few successful polarimetric measurements have however been performed
Externí odkaz:
http://arxiv.org/abs/1612.04098
Autor:
Xiao, H. L., Hajdas, W., Bao, T. W., Batsch, T., Bernasconi, T., Cernuda, I., Chai, J. Y., Dong, Y. W., Gauvin, N., Kole, M., Kong, M. N., Kong, S. W., Li, L., Liu, J. T., Liu, X., Marcinkowski, R., Orsi, S., Pohl, M., Produit, N., Rapin, D., Rutczynska, A., Rybka, D., Shi, H. L., Song, L. M., Sun, J. C., Szabelski, J., Wu, B. B., Wang, R. J., Wen, X., Xu, H. H., Zhang, L., Zhang, L. Y., Zhang, S. N., Zhang, X. F., Zhang, Y. J., Zwolinska, A.
Gamma Ray Bursts (GRBs) are the strongest explosions in the universe which might be associated with creation of black holes. Magnetic field structure and burst dynamics may influence polarization of the emitted gamma-rays. Precise polarization detect
Externí odkaz:
http://arxiv.org/abs/1512.02784
Publikováno v:
In Astronomy and Computing January 2020 30
Autor:
Greiner, J., Mannheim, K., Aharonian, F., Ajello, M., Balasz, L. G., Barbiellini, G., Bellazzini, R., Bishop, S., Bisnovatij-Kogan, G. S., Boggs, S., Bykov, A., DiCocco, G., Diehl, R., Elsässer, D., Foley, S., Fransson, C., Gehrels, N., Hanlon, L., Hartmann, D., Hermsen, W., Hillebrandt, W., Hudec, R., Iyudin, A., Jose, J., Kadler, M., Kanbach, G., Klamra, W., Kiener, J., Klose, S., Kreykenbohm, I., Kuiper, L. M., Kylafis, N., Labanti, C., Langanke, K., Langer, N., Larsson, S., Leibundgut, B., Laux, U., Longo, F., Maeda, K., Marcinkowski, R., Marisaldi, M., McBreen, B., McBreen, S., Meszaros, A., Nomoto, K., Pearce, M., Peer, A., Pian, E., Prantzos, N., Raffelt, G., Reimer, O., Rhode, W., Ryde, F., Schmidt, C., Silk, J., Shustov, B. M., Strong, A., Tanvir, N., Thielemann, F. -K., Tibolla, O., Tierney, D., Trümper, J., Varshalovich, D. A., Wilms, J., Wrochna, G., Zdziarski, A., Zoglauer, A.
We propose to perform a continuously scanning all-sky survey from 200 keV to 80 MeV achieving a sensitivity which is better by a factor of 40 or more compared to the previous missions in this energy range. The Gamma-Ray Imaging, Polarimetry and Spect
Externí odkaz:
http://arxiv.org/abs/1105.1265
Autor:
Suarez-Garcia, E., Haas, D., Hajdas, W., Lamanna, G., Lechanoine-Leluc, C., Marcinkowski, R., Mtchedlishvili, A., Orsi, S., Pohl, M., Produit, N., Rapin, D., Rybka, D., Vialle, J. -P.
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A, 2010
The hard X-ray polarimeter POLAR aims to measure the linear polarization of the 50-500 keV photons arriving from the prompt emission of gamma-ray bursts (GRBs). The position in the sky of the detected GRBs is needed to determine their level of polari
Externí odkaz:
http://arxiv.org/abs/1011.3789
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