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Correction to: AstroSat/LAXPC view of GX 17+2: spectral evolution along the Z-track
Astrophysics and Space Science ( IF 1.8 ) Pub Date : 2020-03-19 , DOI: 10.1007/s10509-020-03770-0 V. K. Agrawal , Anuj Nandi , M. C. Ramadevi
中文翻译：
校正至：GX 17 + 2的AstroSat / LAXPC视图：沿Z轨迹的光谱演变
更新日期：2020-04-14
Astrophysics and Space Science ( IF 1.8 ) Pub Date : 2020-03-19 , DOI: 10.1007/s10509-020-03770-0 V. K. Agrawal , Anuj Nandi , M. C. Ramadevi
In the Discussion section of the initial online publication an incorrect percentage was specified for the observed contribution of the hard X-ray tail in the middle and upper flaring branch to the total flux of 3.0–80.0 keV. The original article has been corrected.
中文翻译：
校正至：GX 17 + 2的AstroSat / LAXPC视图：沿Z轨迹的光谱演变
在最初的在线出版物的“讨论”部分，为观察到的中部和上部燃烧分支中的硬X射线尾部对总通量3.0–80.0 keV的贡献指定了错误的百分比。原始文章已得到纠正。
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