PENELLOPE - VII. Revisiting empirical relations to measure accretion luminosity

Open Access

Fig. 3

Comparison of L_acc computed using the HST modeling with that from the XS-fit. Left: log $L_{acc}^{H S T}$ $\[L_{\text {acc }}^{H S T}\]$ vs. log $L_{acc}^{X S}$ $\[L_{\text {acc }}^{X S}\]$ , the pink line show the best fit, which is linear within the error with its dispersion. Right: differential analysis, the pink region corresponds to the standard deviation of log $L_{a c c}^{H S T}$ $\[L_{\mathrm{acc}}^{H S T}\]$ − log $L_{a c c}^{X S}$ $\[L_{\mathrm{acc}}^{X S}\]$ , computed as the quadrature sum of the individual errors.

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