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This report summarizes the collaborative efforts of the HXT group under the Galileo Project, led by S. Masuda from Nagoya University. Key contributors include T. Kosugi, T. Sakao, J. Sato, M. Sawa, and K. Yoshimura, focusing on Solar-B missions. The document reviews HXT data analysis, encompassing effective area measurements, energy response, and modulation patterns. It introduces software tools utilized for data processing, including IDL and Fortran, and presents various raw data formats, including HDA files and image data, alongside a guide for manual analysis.
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10-Julay-2002 S. Masuda (STEL, Nagoya Univ.) Galileo Project on HXT HXT group quite small !! members T. Kosugi (ISAS) Solar-B/manager T. Sakao (ISAS) Solar-B/XRT S. Masuda (Nagoya U.) J. Sato (Montana State U.) M. Sawa (NAOJ) K. Yoshimura (ISAS) ? ?
HXT data (1) instrument grid (modulation pattern) energy response (effective area) fine-gain change history co-alignment with SXT (2) software IDL software (SSW) fortran software (3) raw data (only HDA file?) counts data (4 bands) PH data (64 channels) (background) (4) image data HXT/SXT images HXT/GOES light curves png file → fits file? (5) manual data format analysis guide (6) others spectrum / total counts analysis results Sato’s catalogue