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Table 5

Matches between PAO-UHECRs & Nearby Elliptical Samples.

RG Extended RC3 Extended RC3 Non-extended

C Model Match Frac. Match Frac. Match Frac.

BSS 4 7.4 3 9.4 9 1.2
ASS 0 0.3 0 0.1 12 1.3
BSA 5 7.1 4 8.8 8 1.2
H ASA 1 0.1 1 0.1 13 1.4
ASS+R 1 1.2 0 0.1 10 1.3
ASS+A 2 1.3 0 0.1 9 1.2
BSS(S) 2 1.7 0 0.0 9 1.3
BSS 5 5.6 5 7.3 13 1.8
ASS 2 1.5 1 1.0 9 1.2
BSA 5 7.5 5 9.5 11 1.6
He ASA 1 0.5 1 0.7 11 1.5
ASS+R 5 4.7 2 3.5 6 1.1
ASS+A 3 2.3 0 0.2 5 0.8
BSS(S) 1 1.1 0 0.3 7 0.9
BSS 10 10.7 10 13.1 18 3.6
ASS 1 5.1 1 6.1 6 2.4
BSA 7 8.5 7 11.0 15 3.6
O ASA 1 2.4 1 3.2 5 2.3
ASS+R 2 5.9 2 5.5 10 2.6
ASS+A 3 6.3 3 6.5 9 2.5
BSS(S) 2 3.9 2 3.5 10 2.1
BSS 11 13.3 11 17.0 25 4.8
ASS 2 8.8 1 10.2 9 3.9
BSA 8 10.7 8 13.3 19 4.9
Al ASA 1 5.1 1 5.2 10 3.9
ASS+R 4 8.7 4 9.2 20 3.7
ASS+A 1 6.3 0 5.6 11 3.7
BSS(S) 0 5.1 0 3.5 10 3.0
BSS 15 24.5 14 29.8 19 5.7
ASS 4 16.2 4 19.6 16 4.8
BSA 12 18.2 12 22.4 20 5.4
Ca ASA 2 8.7 1 8.9 10 4.6
ASS+R 4 9.7 4 11.3 19 4.6
ASS+A 3 10.0 3 9.7 16 4.6
BSS(S) 0 8.1 0 6.0 13 4.3
BSS 18 31.2 17 37.8 22 5.9
ASS 7 20.6 7 23.5 19 5.6
BSA 14 24.9 14 29.2 23 5.9
Fe ASA 5 15.9 4 16.1 14 5.5
ASS+R 6 13.8 6 14.6 23 5.7
ASS+A 2 12.3 1 11.2 17 5.3
BSS(S) 5 13.1 2 10.1 19 5.3

Notes. This table summarizes the match statistics between UHECRs detected by the Pierre Auger Observatory and three samples of ellipticals at D ≤ 75 Mpc: all 15 nearby extended (LLS ≥ 180 kpc) radiogalaxies (Cols. 3 and 4), all ellipticals from the RC3 catalog with extended (LLS ≥ 180 kpc) radio structure (Cols. 5 and 6) and a matched sample of ellipticals from the RC3 catalog without extended radio structure (Cols. 7 and 8; see text). Columns 1 and 2 list the UHECR composition and GMF model. The two columns for each sample of ellipticals list the number of UHECRs (of the total of 27) that can be matched (see text) to some member of the sample, and the fraction of the total (1350) Monte Carlo points that fall within the match distance-limit of the sample’s galaxies.

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