Number of data for version Jan. 20, 2026
| Milky Way | Local Group | |
| Num. of papers | 367 | 90 |
| Num. of objects* | 6,742 | 6,100 |
| Num. of abundance data** | 126,501 | 27,000 |
* Number of unique objects after removing duplicated object IDs
** Different ionization states of the same element are counted as a single datum for each object
- List of Papers
- List of Objects
- Updated on Jan 20, 2026
- Text data in tsv format (all the records)
- Version Jan 20, 2026
- Abundances are in units of [X/H] (including Li where we adopted A(Li) = 3.26) normalized by the solar abundances of Asplund et al. (2009).
- d(X) and f(X) stands for uncertainties and upper limits for element X, respectively.
- New columns: Facility, Resolution, SN, Solar Abundance
- Facility: observational facilities used to take spectra
- Resolution: the highest resolving power obtained to take spectra
- SN: the range of signal-to-noise ratio obtained to take spectra
- Solar Abundance: solar abundances adopted to derive [X/H] or log-e(X) in the original paper
- Text data in tsv format (recommended data set)
- Version April 7, 2026
- Some stars in the database were not correctly identified as the same objects when assigned different identifiers. This issue has been resolved in the current version.
- Abundances are in units of [X/H] (including Li where we adopted A(Li) = 3.26) normalized by the solar abundances of Asplund et al. (2009).
- Recommended list of data, provided by one record for one star, following our priority parameter. See SAGA paper series IV for the definition of the priority parameter.
- Version April 7, 2026