The ALMA-ALPINE [CII] survey - The star formation history and the dust emission of star-forming galaxies at 4.5 < z < 6.2

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Volume 664 (August 2022)

A&A, 664 (2022) A73

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Table 6.

Summary of the power of two for correlation coefficients, r², from the mock analysis on the main physical parameters performed by CIGALE.

Run	L_dust	L_FUV	IRX	M_dust	β_calz94	SFR_10 Myr	f_burst	age_burst	τ_main	age_main	δ	M_star	A_FUV
τ_500 Myr_dl2014	0.98	0.89	0.91	0.98	0.89	0.96				0.81		0.95	0.92
τ_500 Myr_casey2012_OT	0.98	0.84	0.87	0.98	0.84	0.96				0.80		0.93	0.85
τ_20000 Myr_dl2014	0.97	0.92	0.89	0.97	0.87	0.95				0.71		0.94	0.89
τ_20000 Myr_casey2012_OT	0.98	0.90	0.89	0.98	0.87	0.97				0.74		0.95	0.89
τ_500 Myr_dl2014_burst	0.96	0.90	0.88	0.96	0.91	0.93	0.47	0.05		0.46		0.96	0.93
τ_500 Myr_casey2012_OT_burst	0.96	0.94	0.90	0.96	0.89	0.91	0.27	0.06		0.42		0.94	0.92
τ_multi_dl2014	0.98	0.56	0.87	0.98	0.73	0.96			0.20	0.65		0.13	0.90
τ_multi_casey2012_OT	0.98	0.64	0.88	0.98	0.80	0.97			0.18	0.62		0.19	0.91
τ_500 Myr_dl2014_delta	0.99	0.93	0.90	0.99	0.85	0.97				0.78	0.37	0.94	0.89
τ_500 Myr_casey2012_OT_delta	0.98	0.92	0.79	0.98	0.56	0.97				0.79	0.35	0.92	0.62

Notes. The delayed SFH with τ_main = 500 Myr is shown with “tau500” in the legend. If a final burst was added, “burst” is used in the legend. A constant SFH with τ_main = 20 Gyr is shown with “tau20000” in the legend, and multi-τ_main is shown as “multitau” in the legend.

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