The Eurybates family of the Jupiter Trojan asteroids: members, orbital and spectral properties

This dataset contains identified members of the Eurybates family, a collisional family of the Jupiter Trojans.

The members were identified in Marschall et al 2022 (Implications for the collisional strength of Jupiter Trojans from the Eurybates family) using the hierarchical clustering method (HCM).

Two tables presented in the accepted manuscript are available here in machine-readable form.

Table 3. List of all 400 Eurybates family members identified by the hierarchical clustering method (HCM) including the likely interloper (5258) Rhoeo (see discussion in Sec. 2). The table gives the asteroid number (nr.), the provisional designation (prov. des.), the absolute magnitude (H), the diameter (D), as well as the proper semi-major axis (a_prop), eccentricity (e_prop), and inclination (i_prop).

Tabel 4. Color data for Eurybates family members identified by the hierarchical clustering method (HCM) including the likely interloper (5258). The table gives the asteroid number (nr.), the provisional designation (prov. des.), the absolute magnitude (H), the diameter (D), as well as the g-i color from the Sloan Digital Sky Survey, the spectral slopes between 0.3$ to 0.9 \mu m (S), and the g-r color from the Zwicky Transient Facility Observations, ZTF.