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X-ray spectra from Chandrayaan/XSM fitted with differential evolution algorithm

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DataCite Commons2025-10-28 更新2026-05-04 收录
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https://repod.icm.edu.pl/citation?persistentId=doi:10.18150/LIZVTW
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We employ the differential evolution (DE) method to analyze observations from the Solar X-Ray Monitor on board the Chandrayaan-2 spacecraft.In the data set, we provide:PNG files showing 5000 iteration steps of the differential evolution algorithm.PNG files containing Soft X-ray spectra calculated with a CHIANTI code (https://www.chiantidatabase.org/) for a temperature range 1-34.9 MK in 0.1 MK steps.PNG file showing reconstructed X-ray sources with isophotes. They were used for source's size estimation.
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RepOD
创建时间:
2025-10-22
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