Notes. Dereddened mission line fluxes for the knots in the Proplyd 244–140 jet, in units of 10⁻¹⁷ erg s⁻¹ cm⁻². Line fluxes were computed through the Gaussian fitting of spectral profiles extracted from the aperture sizes given in Sect. 3.1. The average uncertainty in the lines fluxes is ~5 × 10⁻¹⁸ erg s⁻¹ cm⁻², which we calculate from the RMS noise in adjacent portions of the spectrum. Empty entries denote positions where either no knot emission is observed or the emission is below the detection threshold, or the knot emission could not be reliably disentangled from the proplyd envelope.