Spectra of the nine blobs we found in our VLT/FORS2 2D spectra that show various emission lines, indicative of star formation at a common redshift of z = 0.102 (x axes are observed wavelengths). Blobs 94 and 98 have no optical counterpart on the Gemini i-band image but showed up in the trace of the FORS2 spectrum. In blobs 2 and 3 the Hα and the [O iii] (5007) line are very strong. In blob 3 we measure an equivalent width of 220 ± 20 Å and 170 ± 20 Å, respectively.