The design and performance of the XL-Calibur anticoincidence shield

Autor: Iyer, N. K., Kiss, M., Pearce, M., Stana, T. -A., Awaki, H., Bose, R. G., Dasgupta, A., De Geronimo, G., Gau, E., Hakamata, T., Ishida, M., Ishiwata, K., Kamogawa, W., Kislat, F., Kitaguchi, T., Krawczynski, H., Lisalda, L., Maeda, Y., Matsumoto, H., Miyamoto, A., Miyazawa, T., Mizuno, T., Rauch, B. F., Cavero, N. Rodriguez, Sakamoto, N., Sato, J., Spooner, S., Takahashi, H., Takeo, M., Tamagawa, T., Uchida, Y., West, A. T., Wimalasena, K., Yoshimoto, M.

Publikováno v: Nuclear Instruments and Methods A 1048 (2023) 167975

The XL-Calibur balloon-borne hard X-ray polarimetry mission comprises a Compton-scattering polarimeter placed at the focal point of an X-ray mirror. The polarimeter is housed within a BGO anticoincidence shield, which is needed to mitigate the consid

Externí odkaz: http://arxiv.org/abs/2212.04139

Study of finite volume number density fluctuation at RHIC energies in PNJL model for the search of QCD Critical Point

Autor: Sarkar, A., Deb, P., Bose, R.

The Quantum Chromo Dynamical (QCD) phase diagram can be explored in the heavy ion collision experiments. The non-monotonic behavior of the conserved number fluctuations are believed to be a signatures of the QCD phase transition and the Critical End

Externí odkaz: http://arxiv.org/abs/2202.00034

Fourier Neural Networks for Function Approximation

Autor: Bose, R Subhash Chandra, Yaswanth, Kakarla

The success of Neural networks in providing miraculous results when applied to a wide variety of tasks is astonishing. Insight in the working can be obtained by studying the universal approximation property of neural networks. It is proved extensivel

Externí odkaz: http://arxiv.org/abs/2111.08438

Detection of the Crab Nebula by the prototype Schwarzschild-Couder Telescope

Autor: Adams, C. B., Ambrosi, G., Ambrosio, M., Aramo, C., Batista, P. I., Benbow, W., Bertucci, B., Bissaldi, E., Bitossi, M., Boiano, A., Bonavolontà, C., Bose, R., Brill, A., Brown, A. M., Buckley, J. H., Cameron, R. A., Canestrari, R., Capasso, M., Caprai, M., Covault, C. E., Depaoli, D., Di Venere, L., Errando, M., Fegan, S., Feng, Q., Fiandrini, E., Furniss, A., Gent, A., Giglietto, N., Giordano, F., Giro, E., Halliday, R., Hervet, O., Holder, J., Humensky, T. B., Incardona, S., Ionica, M., Jin, W., Kieda, D., Licciulli, F., Loporchio, S., Marsella, G., Masone, V., Meagher, K., Meures, T., Mode, B. A. W., Mognet, S. A. I., Mukherjee, R., Okumura, A., Otte, N., Pantaleo, F. R., Paoletti, R., Pareschi, G., Di Pierro, F., Pueschel, E., Ribeiro, D., Riitano, L., Roache, E., Rousselle, J., Rugliancich, A., Santander, M., Shang, R., Stiaccini, L., Tajima, H., Taylor, L. P., Tosti, L., Tovmassian, G., Tripodo, G., Vagelli, V., Valentino, M., Vandenbroucke, J., Vassiliev, V. V., Williams, D. A., Zink, A.

Publikováno v: Proceedings of Science, PoS(ICRC2021)830

The Schwarzschild-Couder Telescope (SCT) is a medium-sized telescope technology proposed for the Cherenkov Telescope Array. It uses a novel dual-mirror optical design that removes comatic aberrations across its entire field of view. The SCT camera em

Externí odkaz: http://arxiv.org/abs/2109.06225

Detection of the Crab Nebula with the 9.7 m Prototype Schwarzschild-Couder Telescope

Autor: Adams, C. B., Alfaro, R., Ambrosi, G., Ambrosio, M., Aramo, C., Arlen, T., Batista, P. I., Benbow, W., Bertucci, B., Bissaldi, E., Biteau, J., Bitossi, M., Boiano, A., Bonavolontà, C., Bose, R., Bouvier, A., Brill, A., Brown, A. M., Buckley, J. H., Byrum, K., Cameron, R. A., Canestrari, R., Capasso, M., Caprai, M., Covault, C. E., Depaoli, D., Errando, M., Fegan, S., Feng, Q., Fiandrini, E., Foote, G., Fortin, P., Funk, S., Furniss, A., Garfias, F., Gent, A., Giglietto, N., Giordano, F., Giro, E., González, M. M., Guarino, V., Halliday, R., Hervet, O., Holder, J., Hughes, G., Humensky, T. B., Ionica, M., Iriarte, A., Jin, W., Johnson, C. A., Kaaret, P., Kieda, D., Kim, B., Kuznetsov, A., Lapington, J. S., Licciulli, F., Loporchio, S., Mason, V., Meagher, K., Meures, T., Mode, B. A. W., Mognet, S. A. I., Mukherjee, R., Nguyen, T., Nieto, D., Okumura, A., Otte, N., La Palombara, N., Pantaleo, F. R., Paoletti, R., Pareschi, G., Petrashyk, A., Di Pierro, F., Pueschel, E., Reynolds, P. T., Ribeiro, D., Richards, G., Roache, E., Ross, D., Rousselle, J., Rugliancich, A., Ruíz-Díaz-Soto, J., Santander, M., Schlenstedt, S., Schneider, M., Scuderi, S., Shang, R., Sironi, G., Stevenson, B., Stiaccini, L., Tajima, H., Taylor, L. P., Thornhill, J., Tosti, L., Tovmassian, G., Vagelli, V., Valentino, M., Vandenbroucke, J., Vassiliev, V. V., Di Venere, L., Wakely, S. P., Watson, J. J., White, R., Wilcox, P., Williams, D. A., Wood, M., Yu, P., Zink, A.

The Schwarzschild-Couder Telescope (SCT) is a telescope concept proposed for the Cherenkov Telescope Array. It employs a dual-mirror optical design to remove comatic aberrations over an $8^{\circ}$ field of view, and a high-density silicon photomulti

Externí odkaz: http://arxiv.org/abs/2012.08448