The data for Newly Detected Old Galactic Globular Cluster Candidates Using Gaia DR3

GAIA_input - Raw data downloaded by GAIA

GAOSI - Gaussian interpolation and testing AND concer fits correlational graph values

The result after clustering_output

mh_gspphot - [Fe/H]  ag_gspphot - AG  m_M - distance modulus  - This is also the header of GC01.csv and GC02.csv under .data\gaosi\GAOS,  which are copied from the csv file in .data\gaosi\GAOSI\output2

Because GAIA lacked part of the data of [Fe/H] and AG after clustering, we adopted the Gaussian RV completion method of Qin et al. (2023) doi: 10.3847/1538-4365/acadd6 to supplement the data of [Fe/H] and AG. The data in these 3 folders is the result of the process we performed. .data\gaosi\GAOSI\output and .data\gaosi\GAOSI\output1 and .data\gaosi\GAOSI\output2 

.data\gaosi\GAOSI\output3  - Test the data after we finish the Gaussian interpolation

.data\gaosi\GAOSI\medain.csv -The median of the data before Gaussian interpolation

.data\gaosi\GAOSI\pyngc01_1sigma.csv and .data\gaosi\GAOSI\pyngc02_1sigma.csv -The mean, standard deviation, and error range of m_M and mh_gspphot and ag_gspphot