The ALPINE-ALMA [CII] Survey: Modelling ALMA and JWST lines to constrain the interstellar medium of z∼ 5 galaxies - Connecting UV, optical, and far-infrared line emission

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Volume 693 (January 2025)

A&A, 693 (2025) A34

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Table B.1

Slope (α) and intercept (β) of the linear regression for the CIII] 1909A˚, [OIII] 5007Å, and Hα lines.

SFH	k_s	CIII] 1909Å		[OIII] 5007Å		Hα
SFH	k_s	α	β	α	β	α	β
	0.34 ‘fiducial’	${0.53}_{- 0.21}^{0.22}$ ${0.53_{ - 0.21}^{0.22}}$	${39.70}_{- 0.38}^{0.38}$ ${39.70_{ - 0.38}^{0.38}}$	${0.38}_{- 0.21}^{0.21}$ ${0.38_{ - 0.21}^{0.21}}$	${40.72}_{- 0.38}^{0.38}$ ${40.72_{ - 0.38}^{0.38}}$	${0.84}_{- 0.21}^{0.21}$ ${0.84_{ - 0.21}^{0.21}}$	${41.33}_{- 0.37}^{0.38}$ ${41.33_{ - 0.37}^{0.38}}$
continous SF	1	${0.66}_{- 0.21}^{0.21}$ ${0.66_{ - 0.21}^{0.21}}$	${39.76}_{- 0.38}^{0.38}$ ${39.76_{ - 0.38}^{0.38}}$	${0.52}_{- 0.21}^{0.21}$ ${0.52_{ - 0.21}^{0.21}}$	${41.70}_{- 0.38}^{0.37}$ ${41.70_{ - 0.38}^{0.37}}$	${0.84}_{- 0.22}^{0.21}$ ${0.84_{ - 0.22}^{0.21}}$	${41.56}_{- 0.38}^{0.37}$ ${41.56_{ - 0.38}^{0.37}}$
	5	${0.66}_{- 0.21}^{0.21}$ ${0.66_{ - 0.21}^{0.21}}$	${40.56}_{- 0.37}^{0.38}$ ${40.56_{ - 0.37}^{0.38}}$	${0.87}_{- 0.21}^{0.21}$ ${0.87_{ - 0.21}^{0.21}}$	${41.93}_{- 0.38}^{0.37}$ ${41.93_{ - 0.38}^{0.37}}$	${0.90}_{- 0.22}^{0.21}$ ${0.90_{ - 0.22}^{0.21}}$	${41.70}_{- 0.37}^{0.38}$ ${41.70_{ - 0.37}^{0.38}}$
	10	${0.87}_{- 0.21}^{0.21}$ ${0.87_{ - 0.21}^{0.21}}$	${40.21}_{- 0.37}^{0.37}$ ${40.21_{ - 0.37}^{0.37}}$	${0.88}_{- 0.21}^{0.21}$ ${0.88_{ - 0.21}^{0.21}}$	${42.12}_{- 0.37}^{0.37}$ ${42.12_{ - 0.37}^{0.37}}$	${0.95}_{- 0.21}^{0.21}$ ${0.95_{ - 0.21}^{0.21}}$	${41.84}_{- 0.37}^{0.38}$ ${41.84_{ - 0.37}^{0.38}}$

	0.34 ‘fiducial’	${0.34}_{- 0.21}^{0.22}$ ${0.34_{ - 0.21}^{0.22}}$	${38.17}_{- 0.38}^{0.38}$ ${38.17_{ - 0.38}^{0.38}}$	${0.56}_{- 0.21}^{0.21}$ ${0.56_{ - 0.21}^{0.21}}$	${37.82}_{- 0.37}^{0.38}$ ${37.82_{ - 0.37}^{0.38}}$	${0.85}_{- 0.21}^{0.21}$ ${0.85_{ - 0.21}^{0.21}}$	${41.27}_{- 0.38}^{0.38}$ ${41.27_{ - 0.38}^{0.38}}$
quenching 5 Myr	1	${0.47}_{- 0.21}^{0.21}$ ${0.47_{ - 0.21}^{0.21}}$	${39.35}_{- 0.37}^{0.37}$ ${39.35_{ - 0.37}^{0.37}}$	${0.42}_{- 0.22}^{0.22}$ ${0.42_{ - 0.22}^{0.22}}$	${39.34}_{- 0.38}^{0.39}$ ${39.34_{ - 0.38}^{0.39}}$	${0.84}_{- 0.21}^{0.21}$ ${0.84_{ - 0.21}^{0.21}}$	${41.53}_{- 0.38}^{0.37}$ ${41.53_{ - 0.38}^{0.37}}$
	5	${0.58}_{- 0.21}^{0.21}$ ${0.58_{ - 0.21}^{0.21}}$	${39.26}_{- 0.37}^{0.37}$ ${39.26_{ - 0.37}^{0.37}}$	${0.76}_{- 0.21}^{0.21}$ ${0.76_{ - 0.21}^{0.21}}$	${40.22}_{- 0.38}^{0.38}$ ${40.22_{ - 0.38}^{0.38}}$	${1.08}_{- 0.21}^{0.21}$ ${1.08_{ - 0.21}^{0.21}}$	${41.20}_{- 0.38}^{0.38}$ ${41.20_{ - 0.38}^{0.38}}$
	10	${0.85}_{- 0.22}^{0.22}$ ${0.85_{ - 0.22}^{0.22}}$	${38.76}_{- 0.38}^{0.38}$ ${38.76_{ - 0.38}^{0.38}}$	${0.69}_{- 0.21}^{0.21}$ ${0.66_{ - 0.21}^{00.21}}$	${40.71}_{- 0.37}^{0.38}$ ${40.71_{ - 0.37}^{0.38}}$	${0.97}_{- 0.21}^{0.21}$ ${0.97_{ - 0.21}^{0.21}}$	${41.34}_{- 0.38}^{0.38}$ ${41.34_{ - 0.38}^{0.38}}$

Notes. Linear regression log(L_line/erg s⁻¹) = α log(SFR/M_⊙ yr⁻¹) + β computed with a Monte Carlo fitting technique. The α and β were obtained assuming the SB99 incident spectrum.

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