Constraining the origin and models of chemical enrichment in galaxy clusters using the Athena X-IFU

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Volume 642 (October 2020)

A&A, 642 (2020) A90

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Table 3.

Top ten best-fit combinations of AGB+SN_cc+SN_Ia models with our X-IFU mock observed abundance ratios at z = 0.1, with 0.1 < SN_Ia/SNe < 0.6 (see text).

	AGB model	SN_cc model	SN_Ia model	SN_Ia frac.	AGB frac.
1.314	K10_0.02	Ro10_2E-3	100-3-c3	0.430	0.340
1.366	K10_0.02	Ro10_2E-3	500-5-c3	0.420	0.330
1.490 ^( † )	K10_0.02	Ro10_2E-4	Th03	0.452	0.319
1.591	K10_0.02	Ro10_2E-3	100-5-c3	0.431	0.328
1.722	K10_0.02	Ro10_2E-3	300-5-c3	0.431	0.325
1.982	K10_0.02	Ro10_2E-3	500-3-c3	0.376	0.328
2.182	K10_0.02	Ro10_2E-4	100-3-c3	0.463	0.337
2.505	K10_0.008	Ro10_2E-3	500-5-c3	0.393	0.388
2.583	K10_0.02	Ro10_2E-3	300-3-c3	0.372	0.325
2.594	K10_0.008	Ro10_2E-4	Th03	0.429	0.377

Notes. The models mentioned here are all further detailed in Appendix A. The models used as input in the cosmological simulations are given in bold. ^( † )This model combination is considered fixed in Sect. 4.

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