Calibration of star formation rate tracers for short- and long-lived star formation episodes

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Table 14:

IMF correction factors for SFR estimators, to be applied on values from Tables 5-8 when IMF slope $\alpha =1$ , 3.
	EB( $\alpha =1$ )			EB( $\alpha=3$ )
Magnitude	10 Myr	30 Myr	250 Myr	10 Myr	30 Myr	250 Myr
$L_{\rm {FIR}}$	0.37	0.45	0.54	2.55	2.09	1.55
$N_{\rm {Lyc}}$	0.25	0.25	0.25	3.68	3.67	3.67
$L_{ \rm {rad}}$	0.37	0.66	0.74	2.95	1.89	1.75
L₁₅₀₀	0.41	0.49	0.60	2.41	1.97	1.49
L₂₀₀₀	0.40	0.50	0.63	2.39	1.92	1.40
L₃₅₀₀	0.36	0.46	0.64	2.50	1.92	1.26
L₄₄₀₀	0.45	0.64	1.16	2.20	1.61	0.98
L₅₅₀₀	0.46	0.66	1.21	2.27	1.68	1.00
L_22 200	0.60	0.90	1.52	2.34	1.82	1.16

Source LaTeX | All tables | In the text

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