X-ray counterparts to stellar MeerKAT Galactic-plane compact radio sources

Open Access

Table 1

Power-law fits to luminosity relationships of RASS and eRASS1 samples.

Relation	RASS	eRASS1
L_X-L_ν,R	$L_{X} = 10^{17.2 \pm 1.6} L_{ν, R}^{0.8 \pm 0.1}$ $Mathematical equation: $\displaystyle L_{\rm X} = 10^{17.2 \pm 1.6} L_{\rm \nu,R}^{0.8 \pm 0.1}$$	$L_{X} = 10^{19.1 \pm 0.6} L_{ν, R}^{0.68 \pm 0.04}$ $Mathematical equation: $\displaystyle L_{\rm X} = 10^{19.1 \pm 0.6} L_{\rm \nu,R}^{0.68 \pm 0.04}$$
L_ν,R-L_bol	$L_{ν, R} = 10^{- 2.1 \pm 2.5} L_{b o l}^{0.53 \pm 0.07}$ $Mathematical equation: $\displaystyle L_{\rm \nu,R} = 10^{-2.1 \pm 2.5}\, L_{\rm bol}^{0.53 \pm 0.07}$$	$L_{ν, R} = 10^{- 2.6 \pm 1.5} L_{b o l}^{0.56 \pm 0.04}$ $Mathematical equation: $\displaystyle L_{\rm \nu,R} = 10^{-2.6 \pm 1.5} \,L_{\rm bol}^{0.56 \pm 0.04}$$
L_X-L_bol	$L_{X} = 10^{29.82 \pm 0.07} {(\frac{L_{b o l}}{10^{33}})}^{0.67 \pm 0.06}$ $Mathematical equation: $\displaystyle L_X = 10^{29.82 \pm 0.07} \left(\frac{L_{\rm bol}}{10^{33 }}\right)^{0.67 \pm 0.06}$$	$L_{X} = 10^{29.90 \pm 0.07} {(\frac{L_{b o l}}{10^{33}})}^{0.48 \pm 0.03}$ $Mathematical equation: $\displaystyle L_X = 10^{29.90 \pm 0.07} \left(\frac{L_{\rm bol}}{10^{33}}\right)^{0.48 \pm 0.03}$$

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