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Table 1

Galaxy clusters selected in our sample, ranked from the highest to the lowest measured SFR in the BCG.

Name z SFR SFR Orig.a SFR Ref.b Mmol c Mmol Ref.d
M⊙ yr-1 1010M⊙
A1835 0.252 146 IR SED Ra12 5.0 Mn14
RXC J1504.1 0.215 140 Hα Og10 – –
RX J1532.9+3021 0.345 110 70 μm Ho12 12.5e Ed01
A1068 0.139 99.3 IR SED Ra12 3.7f Sa03
ZW 3146 0.291 93.1 IR SED Ra12 8.0e Ed01
Z0348 0.254 32.6 IR SED Ra12 – –

Notes.

(a)

Band or method employed to measure SFR;

(b)

reference for SFR: Ra12 = Rawle et al. (2012); Og10 = Ogrean et al. (2010); Ho12 = Hoffer et al. (2012);

(c)

molecular gas mass, Mmol;

(d)

reference for Mmol: Mn14 = McNamara et al. (2014); Ed01 = Edge (2001); Sa03 = Salomé & Combes (2003);

(e)

molecular gas masses originally reported in Edge (2001) have been recomputed using the cosmological parameters described in Sect. 1 and assuming an average Galactic value for the CO to molecular hydrogen conversion factor (Bolatto et al. 2013), i.e., XCO = 2 × 1020 cm-2 (K km s-1)-1;

(f)

molecular gas mass originally reported in Salomé & Combes (2003) has been recomputed assuming an average Galactic value for the CO to molecular hydrogen conversion factor (Bolatto et al. 2013), i.e., XCO = 2 × 1020 cm-2 (K km s-1)-1.

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