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Correction to: Astrophys Space Sci (2020) 365:41 https://doi.org/10.1007/s10509-020-3748-0
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.
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Agrawal, V.K., Nandi, A. & Ramadevi, M.C. Correction to: AstroSat/LAXPC view of GX 17+2: spectral evolution along the Z-track. Astrophys Space Sci 365, 56 (2020). https://doi.org/10.1007/s10509-020-03770-0
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DOI: https://doi.org/10.1007/s10509-020-03770-0