Notes. For each clump we give: the ID of the clump (col. 1), its coordinates (col. 2 and 3), its size in square kiloparsecs as derived from the MUSE data analysis (col. 4), the line-of-sight velocity with respect to the galaxy center (col. 5), the velocity dispersion of the line from the Gaussian fit (col. 6), the integrated line intensity in Jy both derived using a Gaussian fit (col. 7) and integrating all the positive contribution within ±3 Hα velocity dispersion (col. 8), the error on the line flux (col. 9), the S/N of the CO(2−1) line (col. 10), the visual flag used to classify clumps (col. 11), the final integrated line flux (col. 12), and the corresponding H₂ mass in 10⁹ M_⊙ (col. 13). The full table is available at the CDS.