The mmax-Mecl relation in the LEGUS clusters | Astronomy & Astrophysics (A&A)

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Table D.4

Same as Table D.1 but with dynamical ejections with a 2σ ejection fraction and an age uncertainty of 1 Myr.

Bin	Mass range (M_⊙)	Sampling method	N	⟨L_Hα/M_cl⟩	σ_{⟨L_Hα/M_cl⟩}	Median	MAD
1	(5.0 − 22.9) × 10²	optimal	45	33.66	0.05	33.62	0.003
	(5.0 − 22.9) × 10²	random	30	35.82	0.04	35.994	0.006

	(5.17 − 23.17) × 10²	J23	293	34.038	0.016

2	(2.3 − 14.9) × 10³	optimal	51	34.35	0.08	33.843	0.003
	(2.3 − 14.9) × 10³	random	39	35.8	0.04	35.451	0.002

	(2.35 − 14.52) × 10³	J23	73	34.176	0.119

3	(1.5 − 10.0) × 10⁴	optimal	54	34.8348	0.0352	34.941	0.001
	(1.5 − 10.0) × 10⁴	random	27	35.75	0.05	35.3193	0.0007

	(1.881 − 8.567) × 10⁴	J23	9	33.900	0.079

4	(0.5 − 100.0) × 10³	optimal	150	34.79	0.06
4	(0.5 − 100.0) × 10³	random	96	35.76	0.02

5	316 − 10⁵	optimal	160	34.85	0.05
5	316 − 10⁵	random	153	35.77	0.06

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