adsabs/AstroCLIMB huggingface dataset:
Paper: Whence the Interstellar Magnetic Field Shaping the Heliosphere?
Authors: P. C. Frisch, V. Piirola, A. B. Berdyugin, C. Heiles, A. A. Cole, K. Hill, A. M. Magalhães, S. J. Wiktorowicz, J. Bailey, D. V. Cotton, L. Kedziora-Chudczer, N. A. Schwadron, M. Bzowski, D. J. McComas, E. J. Zirnstein, H. O. Funsten, C. Harlingten, and Seth Redfield
Figure caption: Polarization position angles in the region of a possible shock interface between four local clouds defined by RL08, the cloud around the heliosphere (LIC, green), the Doradus cloud (DOR, purple), the Galactic Center cloud (GC, red) and the Blue Cloud (BC, black). Locations are shown for the downfield interstellar magnetic field (from Z16, large purple dot) and a cosmic microwave background dark spot with radius ∼10°–11° (Section 4).
Paper: Whence the Interstellar Magnetic Field Shaping the Heliosphere?
Authors: P. C. Frisch, V. Piirola, A. B. Berdyugin, C. Heiles, A. A. Cole, K. Hill, A. M. Magalhães, S. J. Wiktorowicz, J. Bailey, D. V. Cotton, L. Kedziora-Chudczer, N. A. Schwadron, M. Bzowski, D. J. McComas, E. J. Zirnstein, H. O. Funsten, C. Harlingten, and Seth Redfield
Figure caption: Polarization position angles of stars tracing the extended arc of polarization position angles that includes Filament A are plotted in red. The magnetic field traced by Filament A extends through the nose region of the heliosphere (“N”) and appears to be displaced in the heliotail region that is within the two cyan-colored lunes, Arc 1 and Arc 2. The Hipparcos numbers of the stars forming the extended Filament are listed in Appendix C.
Paper: Whence the Interstellar Magnetic Field Shaping the Heliosphere?
Authors: P. C. Frisch, V. Piirola, A. B. Berdyugin, C. Heiles, A. A. Cole, K. Hill, A. M. Magalhães, S. J. Wiktorowicz, J. Bailey, D. V. Cotton, L. Kedziora-Chudczer, N. A. Schwadron, M. Bzowski, D. J. McComas, E. J. Zirnstein, H. O. Funsten, C. Harlingten, and Seth Redfield
Figure caption: Left: the probability distribution for the upwind direction of the interstellar dust (“staub”) grains flowing into the heliosphere based on Ulysses and Galileo data (Appendix 9 in F99 and M. Landgraf 2022, private communication). The 1σ,  2σ, and 3σ contours of the best-fit upwind dust direction are indicated in dark, medium, and light gray. The minimum χ2 value (“x”) is located at λ, β = 259°, 8°. Right: polarization position angles are plotted in ecliptic coordinates for stars in a region around the heliosphere nose, with position angles of stars tracing Filament A shown in red and dots identifying data where P/ΔP < 1.95. The dotted line is the B–V plane. The green bar shows the axis of the 1σ uncertainty contour for the upwind direction of interstellar dust measured inside heliosphere. Note longitudes increase from right to left.
Paper: Whence the Interstellar Magnetic Field Shaping the Heliosphere?
Authors: P. C. Frisch, V. Piirola, A. B. Berdyugin, C. Heiles, A. A. Cole, K. Hill, A. M. Magalhães, S. J. Wiktorowicz, J. Bailey, D. V. Cotton, L. Kedziora-Chudczer, N. A. Schwadron, M. Bzowski, D. J. McComas, E. J. Zirnstein, H. O. Funsten, C. Harlingten, and Seth Redfield
Figure caption: The IBEX ribbon is shown in Galactic (top), ecliptic (middle), and celestial (bottom) coordinates for the 9 yr maps of 1.7 keV ribbon ENAs (Schwadron et al. 2018). Locations of Voyager 1 and Voyager 2 are shown with cyan-colored letters and dots. Positions of the 3 kHz emissions detected by Voyager 1 and Voyager 2 are shown as white dots. Locations of three QSO intraday variables are identified with red letters A (J1819+3845), B (PKS 1257-326), and C (PKS B1519-273). The cyan-colored “V” letters indicate the current locations of Voyager 1 and Voyager 2. The direction and opposite directions of the local interstellar magnetic field are indicated by the cyan-colored “UpB” and “DnB.” The upwind and downwind directions of the interstellar wind flowing the heliosphere are indicated by the cyan-colored “UpV” and “DnV.” Red dots show the cosmic microwave background multiple moments found by Copi et al. (2007) in the WMAP ILC3 map.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Illustration of the satellite platform and the payloads of Insight-HXMT. The coordinate system used in this study is shown in the upper left corner. It is adapted from Figure 1 in Luo et al. (2020).
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Effective areas of HXMT/CsI, , Fermi/LAT, Fermi/GBM, Konus-Wind, Swift/BAT, CALET/CGBM, and AstroSat/CZTI. The effective area of Fermi/GBM (NaI) is averaged over the unocculted sky. It is adapted from Figure 13 in Luo et al. (2020).
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: The deposited energy spectra of three types of BAND with an incident angle θ of 0°–180° are shown in NG mode. The azimuthal angle ϕ is 0°. Here the incident angle θ and the azimuthal angle ϕ denote the direction of gamma-rays in spherical coordinates of the HE/CsI detector.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: The deposited energy spectra of three types of BAND with an incident angle θ of 0° to 180° are shown in LG mode. The azimuthal angle ϕ is 0°. Here the incident angle θ and the azimuthal angle ϕ denote the direction of gamma-rays in spherical coordinates of the HE/CsI detector.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: A comparison between light curves with and without dead-time correction of a short GRB triggered on 2019 November 05 T06:11:08.65 UTC. The histogram of red lines and the error bars denote the light curve without dead-time correction, while the black histogram shows the light curve with dead-time correction. Here MET means the mission-elapsed time of HXMT.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: The distribution from the “GOLDEN” GRB samples of the time delays of Fermi/GBM (dashed), Swift/BAT (dotted), and GECAM (dot–dashed) relative to HXMT.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: The distribution of the low-energy spectral index α of “GOLDEN” GRBs from time-averaged spectral fits. The solid blue lines denote the total distribution of α from the BAND model (dashed red lines), the CPL model (dotted green lines), and the PL (dotted–dashed orange lines).
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: The distribution of the νFν peak energy Epeak of “GOLDEN” GRBs from time-averaged spectral fits. The solid blue lines denote the total distribution of Epeak from the BAND model (dashed red lines) and the CPL model (dotted green lines).
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: The distribution of the high-energy spectral index β of “GOLDEN” GRBs from time-averaged spectral fits.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Distribution of “GOLDEN” GRB durations in the 10–2000 keV energy range. The upper plot shows T50, and the lower plot shows T90.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Comparison between the durations (T90) of “GOLDEN” GRBs from a joint analysis and those obtained from HXMT/Cs I GRB counts. The red line denotes the case when these two are equal to each other.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Scatter plots of spectral hardness vs. duration for the two duration measures T50 (upper plot) and T90 (lower plot) as shown in Figure 10. The hardness is calculated as the ratio of the flux density from spectral parameters determined from time-averaged spectral fits in 50-300 keV to that in 10–50 keV. For clarity, the estimated errors are not shown, but they can be quite large for the weak events. Nevertheless, the anticorrelation of spectral hardness with burst duration is evident.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Distribution of the “GOLDEN” GRB peak flux on the 0.064 s timescale in the energy range of 10–2000 keV.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Distribution of the “GOLDEN” GRB peak flux on the 0.256 s timescale in the energy range of 10–2000 keV.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Distribution of the “GOLDEN” GRB peak flux on the 1.024 s timescale in the energy range of 10–2000 keV.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Distribution of the “GOLDEN” GRB fluence in the energy range of 10–2000 keV.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Light curve of GRB 200125B (HEB200125863) from 18 CsI detectors. Vertical lines indicate the regions selected for the fit to the time-averaged spectra. Green regions define the background region. Here MET means the mission-elapsed time of HXMT.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Joint analysis of the time-averaged spectrum of GRB 200125B (HEB200125863). Data from 18 HXMT/CsI detectors and from Fermi/GBM NaI detectors 0 and 1, and from the BGO detector 0 are used.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Photon flux light curve for GRB 200125B (HEB200125863) produced by the duration analysis. Data from 18 HE/CsI detectors and from Fermi/GBM NaI detector 0 and 1, and from the BGO detector 0 are used. Here MET means the mission-elapsed time of HXMT.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: The duration plot for GRB 200125B (HEB200125863). Horizontal dashed lines in dark red are drawn at 5% and 95% of the total fluence, while those in dark blue are at 25% and 75%. Vertical dotted lines are drawn at the times corresponding to these same fluences, thereby defining the T50 and T90 intervals. The dotted green horizontal lines correspond to 0% and 100% of the total integration of the flux. Here MET means the mission-elapsed time of HXMT.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Joint analysis of the time-averaged spectrum of GRB 210121A (HEB210121779). Data from 18 HE/CsI detectors and from the Fermi/GBM NaI detector 0 and 3, and from the BGO detector 0 are used.
Paper: The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years
Authors: Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang, Cheng-Kui Li, Xiao-Bo Li, Yue Huang, Cristiano Guidorzi, Filippo Frontera, Cong-Zhan Liu, Xu-Fang Li, Gang Li, Jin-Yuan Liao, Ce Cai, Qi Luo, Shuo Xiao, Qi-Bin Yi, Yao-Guang Zheng, Deng-Ke Zhou, Jia-Cong Liu, Wang-Chen Xue, Yan-Qiu Zhang, Chao Zheng, Zhi Chang, Zheng-Wei Li, Xue-Feng Lu, Ai-Mei Zhang, Yi-Fei Zhang, Yong-Jie Jin, Ti-Pei Li, Fang-Jun Lu, Li-Ming Song, Mei Wu, Yu-Peng Xu, Xiang Ma, Ming-Yu Ge, Shu-Mei Jia, Bing Li, Jian-Yin Nie, Ling-Jun Wang, Juan Zhang, Shi-Jie Zheng, Xue-Juan Yang, and Rong-Jia Yang
Figure caption: Joint analysis of the time-averaged spectrum of GRB 210112A (HEB210112068). Data from 18 HE/CsI detectors and from Swift/BAT are used.
Paper: Chemical Composition of Bright Stars in the Northern Hemisphere: Star–Planet Connection
Authors: G. Tautvaišienė, Š. Mikolaitis, A. Drazdauskas, E. Stonkutė, R. Minkevičiūtė, E. Pakštienė, H. Kjeldsen, K. Brogaard, Y. Chorniy, C. von Essen, F. Grundahl, M. Ambrosch, V. Bagdonas, A. Sharma, and C. Viscasillas Vázquez
Figure caption: Positions (R.A. and decl. in hours and degrees) of the stars (black dots) observed in this work (blue shadowed area) and in Paper I (pink shadowed area) in the TESS CVZ. The JWST CVZ is indicated as well.