Star formation and accretion rates within 500 pc as traced by Gaia DR3 XP spectra

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Table 3.

Results of the power law fits log(L_acc) = m ⋅ log(L_⋆)+c and log(Ṁ_acc) = m · log(M_⋆) +c, for the different samples of YSOs defined in Sect. 2.7, and for values calculated from both GSP-Phot extinction and med-GSP-Phot extinction.

Flag	Extinction	N. sources	m_{L_acc}	c_{L_acc}	$m_{{\dot{M}}_{acc}}$ $m_{\dot M_\text{acc}}$	$c_{{\dot{M}}_{acc}}$ $c_{\dot M_\text{acc}}$
IR	GSP-Phot	1564	1.51 ± 0.01	−1.42 ± 0.02	2.5 ± 0.1	−9.31 ± 0.05
pEW	GSP-Phot	2836	1.53 ± 0.01	−1.29 ± 0.01	2.25 ± 0.06	−9.72 ± 0.03
combined	GSP-Phot	656	1.41 ± 0.02	−1.19 ± 0.02	2.4 ± 0.1	−8.93 ± 0.05

IR	med-GSP-Phot	4086	1.57 ± 0.01	−1.37 ± 0.01	2.38 ± 0.04	−8.87 ± 0.02
pEW	med-GSP-Phot	5934	1.53 ± 0.01	−1.30 ± 0.01	2.20 ± 0.04	−9.29 ± 0.02
combined	med-GSP-Phot	1871	1.50 ± 0.02	−1.16 ± 0.02	2.19 ± 0.05	−8.66 ± 0.03

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