
If you use this package, please cite Crompvoets et al. 2025. Please also cite the original producers of the data used/producers of the software used to create the data used for this work: YSOs: Richardson et al. (2024)Brown dwarfs: ATMO -- Phillips et al. (2020)White dwarfs: Blouin et al. (2018)Field stars: PARSEC -- Bressen et al. (2012)Galaxies: CIGALE -- Burgarella et al. 2005, Noll et al. 2009 Boquin et al. (2020)
Repository associated with the code found in Crompvoets et al. 2026, Introducing SESHAT: A Tool for Object Classification from JWST Catalogs (arXiv:2510.07747), accepted into the Astronomical Journal.
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
