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

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Volume 709 (May 2026)

A&A, 709 (2026) A4

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Table D.6

Statistical results including all effects.

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	87	34.36	0.07	33.14	0.06
	(5.0 − 22.9) × 10²	random	59	35.825	0.026	35.4396	0.0004

	(5.17 − 23.17) × 10²	J23	293	34.038	0.016

2	(2.3 − 14.9) × 10³	optimal	104	34.57	0.06	34.678	0.003
	(2.3 − 14.9) × 10³	random	79	35.801	0.026	35.015	0.005

	(2.35 − 14.52) × 10³	J23	73	34.176	0.119

3	(1.5 − 10.0) × 10⁴	optimal	107	34.913	0.022	34.976	0.005
	(1.5 − 10.0) × 10⁴	random	54	35.76	0.03	35.421	0.001

	(1.881 − 8.567) × 10⁴	J23	9	33.900	0.079

4	(0.5 − 100.0) × 10³	optimal	298	34.88	0.04
4	(0.5 − 100.0) × 10³	random	192	35.767	0.016

5	316 − 10⁵	optimal	320	34.94	0.04
5	316 − 10⁵	random	306	35.77	0.04

Notes. Same as Table D.1 but for the summed clusters of cases with a 2σ ejection fraction, an age uncertainty of 1 Myr, and with and without field stars (see Sect. 4.1) for the final comparison.

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