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Main Authors:	Liu, Y., Sun, H., Xu, D., Svinkin, D. S., Delaunay, J., Tanvir, N. R., Gao, H., Zhang, C., Chen, Y., Wu, X. -F., Zhang, B., Yuan, W., An, J., Bruni, G., Frederiks, D. D., Ghirlanda, G., Hu, J. -W., Li, A., Li, C. -K., Li, J. -D., Malesani, D. B., Piro, L., Raman, G., Ricci, R., Troja, E., Vergani, S. D., Wu, Q. -Y., Yang, J., Zhang, B. -B., Zhu, Z. -P., Postigo, A. de Ugarte, Demin, A. G., Dobie, D., Fan, Z., Fu, S. -Y., Fynbo, J. P. U., Geng, J. -J., Gianfagna, G., Hu, Y. -D., Huang, Y. -F., Jiang, S. -Q., Jonker, P. G., Julakanti, Y., Kennea, J. A., Kokomov, A. A., Kuulkers, E., Lei, W. -H., Leung, J. K., Levan, A. J., Li, D. -Y., Li, Y., Littlefair, S. P., Liu, X., Lysenko, A. L., Ma, Y. -N., Martin-Carrillo, A., O'Brien, P., Parsotan, T., Quirola-Vasquez, J., Ridnaia, A. V., Ronchini, S., Rossi, A., Mata-Sanchez, D., Schneider, B., Shen, R. -F., Thakur, A. L., Tohuvavohu, A., Torres, M. A. P., Tsvetkova, A. E., Ulanov, M. V., Wei, J. -J., Xiao, D., Yin, Y. -H. I., Bai, M., Burwitz, V., Cai, Z. -M., Chen, F. -S., Chen, H. -L., Chen, T. -X., Chen, W., Chen, Y. -F., Chen, Y. -H., Cheng, H. -Q., Cui, C. -Z., Cui, W. -W., Dai, Y. -F., Dai, Z. -G., Eder, J., Fan, D. -W., Feldman, C., Feng, H., Feng, Z., Friedrich, P., Gao, X., Guan, J., Han, D. -W, Han, J., Hou, D. -J., Hu, H. -B., Hu, T., Huang, M. -H., Huo, J., Hutchinson, I., Ji, Z., Jia, S. -M., Jia, Z. -Q., Jiang, B. -W., Jin, C. -C., Jin, G., Jin, J. -J., Keereman, A., Lerman, H., Li, J. -F., Li, L. -H., Li, M. -S., Li, W., Li, Z. -D., Lian, T. -Y., Liang, E. -W., Ling, Z. -X., Liu, C. -Z., Liu, H. -Y., Liu, H. -Q., Liu, M. -J., Liu, Y. -R., Lu, F. -J., LU, H. -J., Luo, L. -D., Ma, F. L., Ma, J., Mao, J. -R., Mao, X., McHugh, M., Meidinger, N., Nandra, K., Osborne, J. P., Pan, H. -W., Pan, X., Ravasio, M. E., Rau, A., Rea, N., Rehman, U., Sanders, J., Santovincenzo, A., Song, L. -M., Su, J., Sun, L. -J., Sun, S. -L., Sun, X. -J., Tan, Y. -Y., Tang, Q. -J., Tao, Y. -H., Tong, J. -Z., Wang, H., Wang, J., Wang, L., Wang, W. -X., Wang, X. -F., Wang, X. -Y., Wang, Y. -L., Wang, Y. -S., Wei, D. -M., Willingale, R., Xiong, S. -L., Xu, H. -T., Xu, J. -J., Xu, X. -P., Xu, Y. -F., Xu, Z., Xue, C. -B., Xue, Y. -L., Yan, A. -L., Yang, F., Yang, H. -N., Yang, X. -T., Yang, Y. -J, Yu, Y. -W., Zhang, J., Zhang, M., Zhang, S. -N., Zhang, W. -D., Zhang, W. -J., Zhang, Y. -H., Zhang, Z., Zhang, Z. -L., Zhao, D. -H., Zhao, H. -S., Zhao, X. -F., Zhao, Z. -J., Zhou, L. -X., Zhou, Y. -L., Zhu, Y. -X., Zhu, Z. -C., Zuo, X. -X.
Format:	Preprint
Published:	2024
Subjects:	High Energy Astrophysical Phenomena
Online Access:	https://arxiv.org/abs/2404.16425
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author	Liu, Y. Sun, H. Xu, D. Svinkin, D. S. Delaunay, J. Tanvir, N. R. Gao, H. Zhang, C. Chen, Y. Wu, X. -F. Zhang, B. Yuan, W. An, J. Bruni, G. Frederiks, D. D. Ghirlanda, G. Hu, J. -W. Li, A. Li, C. -K. Li, J. -D. Malesani, D. B. Piro, L. Raman, G. Ricci, R. Troja, E. Vergani, S. D. Wu, Q. -Y. Yang, J. Zhang, B. -B. Zhu, Z. -P. Postigo, A. de Ugarte Demin, A. G. Dobie, D. Fan, Z. Fu, S. -Y. Fynbo, J. P. U. Geng, J. -J. Gianfagna, G. Hu, Y. -D. Huang, Y. -F. Jiang, S. -Q. Jonker, P. G. Julakanti, Y. Kennea, J. A. Kokomov, A. A. Kuulkers, E. Lei, W. -H. Leung, J. K. Levan, A. J. Li, D. -Y. Li, Y. Littlefair, S. P. Liu, X. Lysenko, A. L. Ma, Y. -N. Martin-Carrillo, A. O'Brien, P. Parsotan, T. Quirola-Vasquez, J. Ridnaia, A. V. Ronchini, S. Rossi, A. Mata-Sanchez, D. Schneider, B. Shen, R. -F. Thakur, A. L. Tohuvavohu, A. Torres, M. A. P. Tsvetkova, A. E. Ulanov, M. V. Wei, J. -J. Xiao, D. Yin, Y. -H. I. Bai, M. Burwitz, V. Cai, Z. -M. Chen, F. -S. Chen, H. -L. Chen, T. -X. Chen, W. Chen, Y. -F. Chen, Y. -H. Cheng, H. -Q. Cui, C. -Z. Cui, W. -W. Dai, Y. -F. Dai, Z. -G. Eder, J. Fan, D. -W. Feldman, C. Feng, H. Feng, Z. Friedrich, P. Gao, X. Guan, J. Han, D. -W Han, J. Hou, D. -J. Hu, H. -B. Hu, T. Huang, M. -H. Huo, J. Hutchinson, I. Ji, Z. Jia, S. -M. Jia, Z. -Q. Jiang, B. -W. Jin, C. -C. Jin, G. Jin, J. -J. Keereman, A. Lerman, H. Li, J. -F. Li, L. -H. Li, M. -S. Li, W. Li, Z. -D. Lian, T. -Y. Liang, E. -W. Ling, Z. -X. Liu, C. -Z. Liu, H. -Y. Liu, H. -Q. Liu, M. -J. Liu, Y. -R. Lu, F. -J. LU, H. -J. Luo, L. -D. Ma, F. L. Ma, J. Mao, J. -R. Mao, X. McHugh, M. Meidinger, N. Nandra, K. Osborne, J. P. Pan, H. -W. Pan, X. Ravasio, M. E. Rau, A. Rea, N. Rehman, U. Sanders, J. Santovincenzo, A. Song, L. -M. Su, J. Sun, L. -J. Sun, S. -L. Sun, X. -J. Tan, Y. -Y. Tang, Q. -J. Tao, Y. -H. Tong, J. -Z. Wang, H. Wang, J. Wang, L. Wang, W. -X. Wang, X. -F. Wang, X. -Y. Wang, Y. -L. Wang, Y. -S. Wei, D. -M. Willingale, R. Xiong, S. -L. Xu, H. -T. Xu, J. -J. Xu, X. -P. Xu, Y. -F. Xu, Z. Xue, C. -B. Xue, Y. -L. Yan, A. -L. Yang, F. Yang, H. -N. Yang, X. -T. Yang, Y. -J Yu, Y. -W. Zhang, J. Zhang, M. Zhang, S. -N. Zhang, W. -D. Zhang, W. -J. Zhang, Y. -H. Zhang, Z. Zhang, Z. Zhang, Z. -L. Zhao, D. -H. Zhao, H. -S. Zhao, X. -F. Zhao, Z. -J. Zhou, L. -X. Zhou, Y. -L. Zhu, Y. -X. Zhu, Z. -C. Zuo, X. -X.
author_facet	Liu, Y. Sun, H. Xu, D. Svinkin, D. S. Delaunay, J. Tanvir, N. R. Gao, H. Zhang, C. Chen, Y. Wu, X. -F. Zhang, B. Yuan, W. An, J. Bruni, G. Frederiks, D. D. Ghirlanda, G. Hu, J. -W. Li, A. Li, C. -K. Li, J. -D. Malesani, D. B. Piro, L. Raman, G. Ricci, R. Troja, E. Vergani, S. D. Wu, Q. -Y. Yang, J. Zhang, B. -B. Zhu, Z. -P. Postigo, A. de Ugarte Demin, A. G. Dobie, D. Fan, Z. Fu, S. -Y. Fynbo, J. P. U. Geng, J. -J. Gianfagna, G. Hu, Y. -D. Huang, Y. -F. Jiang, S. -Q. Jonker, P. G. Julakanti, Y. Kennea, J. A. Kokomov, A. A. Kuulkers, E. Lei, W. -H. Leung, J. K. Levan, A. J. Li, D. -Y. Li, Y. Littlefair, S. P. Liu, X. Lysenko, A. L. Ma, Y. -N. Martin-Carrillo, A. O'Brien, P. Parsotan, T. Quirola-Vasquez, J. Ridnaia, A. V. Ronchini, S. Rossi, A. Mata-Sanchez, D. Schneider, B. Shen, R. -F. Thakur, A. L. Tohuvavohu, A. Torres, M. A. P. Tsvetkova, A. E. Ulanov, M. V. Wei, J. -J. Xiao, D. Yin, Y. -H. I. Bai, M. Burwitz, V. Cai, Z. -M. Chen, F. -S. Chen, H. -L. Chen, T. -X. Chen, W. Chen, Y. -F. Chen, Y. -H. Cheng, H. -Q. Cui, C. -Z. Cui, W. -W. Dai, Y. -F. Dai, Z. -G. Eder, J. Fan, D. -W. Feldman, C. Feng, H. Feng, Z. Friedrich, P. Gao, X. Guan, J. Han, D. -W Han, J. Hou, D. -J. Hu, H. -B. Hu, T. Huang, M. -H. Huo, J. Hutchinson, I. Ji, Z. Jia, S. -M. Jia, Z. -Q. Jiang, B. -W. Jin, C. -C. Jin, G. Jin, J. -J. Keereman, A. Lerman, H. Li, J. -F. Li, L. -H. Li, M. -S. Li, W. Li, Z. -D. Lian, T. -Y. Liang, E. -W. Ling, Z. -X. Liu, C. -Z. Liu, H. -Y. Liu, H. -Q. Liu, M. -J. Liu, Y. -R. Lu, F. -J. LU, H. -J. Luo, L. -D. Ma, F. L. Ma, J. Mao, J. -R. Mao, X. McHugh, M. Meidinger, N. Nandra, K. Osborne, J. P. Pan, H. -W. Pan, X. Ravasio, M. E. Rau, A. Rea, N. Rehman, U. Sanders, J. Santovincenzo, A. Song, L. -M. Su, J. Sun, L. -J. Sun, S. -L. Sun, X. -J. Tan, Y. -Y. Tang, Q. -J. Tao, Y. -H. Tong, J. -Z. Wang, H. Wang, J. Wang, L. Wang, W. -X. Wang, X. -F. Wang, X. -Y. Wang, Y. -L. Wang, Y. -S. Wei, D. -M. Willingale, R. Xiong, S. -L. Xu, H. -T. Xu, J. -J. Xu, X. -P. Xu, Y. -F. Xu, Z. Xue, C. -B. Xue, Y. -L. Yan, A. -L. Yang, F. Yang, H. -N. Yang, X. -T. Yang, Y. -J Yu, Y. -W. Zhang, J. Zhang, M. Zhang, S. -N. Zhang, W. -D. Zhang, W. -J. Zhang, Y. -H. Zhang, Z. Zhang, Z. Zhang, Z. -L. Zhao, D. -H. Zhao, H. -S. Zhao, X. -F. Zhao, Z. -J. Zhou, L. -X. Zhou, Y. -L. Zhu, Y. -X. Zhu, Z. -C. Zuo, X. -X.
contents	Long gamma-ray bursts (GRBs) are believed to originate from core collapse of massive stars. High-redshift GRBs can probe the star formation and reionization history of the early universe, but their detection remains rare. Here we report the detection of a GRB triggered in the 0.5--4 keV band by the Wide-field X-ray Telescope (WXT) on board the Einstein Probe (EP) mission, designated as EP240315a, whose bright peak was also detected by the Swift Burst Alert Telescope and Konus-Wind through off-line analyses. At a redshift of $z=4.859$, EP240315a showed a much longer and more complicated light curve in the soft X-ray band than in gamma-rays. Benefiting from a large field-of-view ($\sim$3600 deg$^2$) and a high sensitivity, EP-WXT captured the earlier engine activation and extended late engine activity through a continuous detection. With a peak X-ray flux at the faint end of previously known high-$z$ GRBs, the detection of EP240315a demonstrates the great potential for EP to study the early universe via GRBs.
format	Preprint
id	arxiv_https___arxiv_org_abs_2404_16425
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Soft X-ray prompt emission from a high-redshift gamma-ray burst EP240315a Liu, Y. Sun, H. Xu, D. Svinkin, D. S. Delaunay, J. Tanvir, N. R. Gao, H. Zhang, C. Chen, Y. Wu, X. -F. Zhang, B. Yuan, W. An, J. Bruni, G. Frederiks, D. D. Ghirlanda, G. Hu, J. -W. Li, A. Li, C. -K. Li, J. -D. Malesani, D. B. Piro, L. Raman, G. Ricci, R. Troja, E. Vergani, S. D. Wu, Q. -Y. Yang, J. Zhang, B. -B. Zhu, Z. -P. Postigo, A. de Ugarte Demin, A. G. Dobie, D. Fan, Z. Fu, S. -Y. Fynbo, J. P. U. Geng, J. -J. Gianfagna, G. Hu, Y. -D. Huang, Y. -F. Jiang, S. -Q. Jonker, P. G. Julakanti, Y. Kennea, J. A. Kokomov, A. A. Kuulkers, E. Lei, W. -H. Leung, J. K. Levan, A. J. Li, D. -Y. Li, Y. Littlefair, S. P. Liu, X. Lysenko, A. L. Ma, Y. -N. Martin-Carrillo, A. O'Brien, P. Parsotan, T. Quirola-Vasquez, J. Ridnaia, A. V. Ronchini, S. Rossi, A. Mata-Sanchez, D. Schneider, B. Shen, R. -F. Thakur, A. L. Tohuvavohu, A. Torres, M. A. P. Tsvetkova, A. E. Ulanov, M. V. Wei, J. -J. Xiao, D. Yin, Y. -H. I. Bai, M. Burwitz, V. Cai, Z. -M. Chen, F. -S. Chen, H. -L. Chen, T. -X. Chen, W. Chen, Y. -F. Chen, Y. -H. Cheng, H. -Q. Cui, C. -Z. Cui, W. -W. Dai, Y. -F. Dai, Z. -G. Eder, J. Fan, D. -W. Feldman, C. Feng, H. Feng, Z. Friedrich, P. Gao, X. Guan, J. Han, D. -W Han, J. Hou, D. -J. Hu, H. -B. Hu, T. Huang, M. -H. Huo, J. Hutchinson, I. Ji, Z. Jia, S. -M. Jia, Z. -Q. Jiang, B. -W. Jin, C. -C. Jin, G. Jin, J. -J. Keereman, A. Lerman, H. Li, J. -F. Li, L. -H. Li, M. -S. Li, W. Li, Z. -D. Lian, T. -Y. Liang, E. -W. Ling, Z. -X. Liu, C. -Z. Liu, H. -Y. Liu, H. -Q. Liu, M. -J. Liu, Y. -R. Lu, F. -J. LU, H. -J. Luo, L. -D. Ma, F. L. Ma, J. Mao, J. -R. Mao, X. McHugh, M. Meidinger, N. Nandra, K. Osborne, J. P. Pan, H. -W. Pan, X. Ravasio, M. E. Rau, A. Rea, N. Rehman, U. Sanders, J. Santovincenzo, A. Song, L. -M. Su, J. Sun, L. -J. Sun, S. -L. Sun, X. -J. Tan, Y. -Y. Tang, Q. -J. Tao, Y. -H. Tong, J. -Z. Wang, H. Wang, J. Wang, L. Wang, W. -X. Wang, X. -F. Wang, X. -Y. Wang, Y. -L. Wang, Y. -S. Wei, D. -M. Willingale, R. Xiong, S. -L. Xu, H. -T. Xu, J. -J. Xu, X. -P. Xu, Y. -F. Xu, Z. Xue, C. -B. Xue, Y. -L. Yan, A. -L. Yang, F. Yang, H. -N. Yang, X. -T. Yang, Y. -J Yu, Y. -W. Zhang, J. Zhang, M. Zhang, S. -N. Zhang, W. -D. Zhang, W. -J. Zhang, Y. -H. Zhang, Z. Zhang, Z. Zhang, Z. -L. Zhao, D. -H. Zhao, H. -S. Zhao, X. -F. Zhao, Z. -J. Zhou, L. -X. Zhou, Y. -L. Zhu, Y. -X. Zhu, Z. -C. Zuo, X. -X. High Energy Astrophysical Phenomena Long gamma-ray bursts (GRBs) are believed to originate from core collapse of massive stars. High-redshift GRBs can probe the star formation and reionization history of the early universe, but their detection remains rare. Here we report the detection of a GRB triggered in the 0.5--4 keV band by the Wide-field X-ray Telescope (WXT) on board the Einstein Probe (EP) mission, designated as EP240315a, whose bright peak was also detected by the Swift Burst Alert Telescope and Konus-Wind through off-line analyses. At a redshift of $z=4.859$, EP240315a showed a much longer and more complicated light curve in the soft X-ray band than in gamma-rays. Benefiting from a large field-of-view ($\sim$3600 deg$^2$) and a high sensitivity, EP-WXT captured the earlier engine activation and extended late engine activity through a continuous detection. With a peak X-ray flux at the faint end of previously known high-$z$ GRBs, the detection of EP240315a demonstrates the great potential for EP to study the early universe via GRBs.
title	Soft X-ray prompt emission from a high-redshift gamma-ray burst EP240315a
topic	High Energy Astrophysical Phenomena
url	https://arxiv.org/abs/2404.16425

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