Dust depletion of metals from local to distant galaxies - I. Peculiar nucleosynthesis effects and grain growth in the ISM

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Volume 666 (October 2022)

A&A, 666 (2022) A12

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202243994e]

Table 5

Orthogonal distance regression results of the fits for the depletion of Ti in the different environments.

Ti	A2_X	B2_X	χ²		v		r	p-value
Milky Way	0.02 ± 0.30	−1.73 ± 0.22	57.84	2.00	29	0.07	−0.81	4.13e-08	0.12
QSO-DLAs	−0.17 ± 0.07	−1.36 ± 0.19	61.24	2.36	26	0.16	−0.87	2.32e-09	0.13
LMC	−0.53 ± 0.12	−1.01 ± 0.13	2.83	0.35	8	0.96	−0.97	3.00e-06	0.05
SMC	−0.35 ± 0.04	−1.11 ± 0.06	0.79	0.07	11	0.86	−0.99	2.90e-10	0.02
GRB-DLAs	–	–	–	–	–	–	–	–	–
Merged fit	−0.06 ± 0.03	−1.64 ± 0.04	164.49	2.03	81	–	−0.97	≪	0.13

Notes. The columns list the χ², the reduced , the degrees of freedom v, the difference between the fit to the individual samples, and the merged fit to the individual sample (), the Pearson correlation coefficients r, the p-value, and intrinsic scatter .

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