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Table A.1

BAT and reference samples.

Name RA Dec Sample Scale Re,70 Band log(LFIR) log(L14−195 keV)
J2000 J2000 kpc/′′ kpc L erg/s
(1) (2) (3) (4) (5) (6) (7) (8) (9)

UGC 12914 0.4110 23.4825 Ref 0.297 5.876 ±0.032 70 10.16
UGC 12915 0.4256 23.4956 Ref 0.295 2.086 ±0.003 70 10.49
PG 0003+199 1.5805 20.2027 BAT 0.519 0.399 ±0.075 70 9.77 43.45
NGC 23 2.4716 25.9237 Ref 0.310 1.004 ±0.003 70 10.75
NGC 34 2.7780 –12.1076 Ref 0.398 0.253 ±0.017 70 11.28
Arp 256N 4.7081 –10.3604 Ref 0.549 3.159 ±0.016 70 10.34
Arp 256S 4.7122 –10.3771 Ref 0.544 0.876 ±0.010 70 11.13
2MASX J00253292+6821 6.3847 68.3625 BAT 0.246 0.307 ±0.050 70 9.07 42.77
CGCG 535-012 9.0875 45.6649 BAT 0.934 1.909 ±0.287 70 10.03 43.92
...

Notes. (1) Source name. (2), (3) Far-infrared source position, as measured from the Gaussian fits. (4) Sample – BAT or reference (Ref). (5) Scale for the adopted distance and cosmology. (6) Far-infrared half light radii at 70 μm. Half light radii are based on subtracting in quadrature observed width and PSF width. The errors are only statistical and do not include systematics due to the non-Gaussianity of the real source structure and the PSF. (7) Band used to derive Re,70. Re,70 is derived from Herschel-PACS 70 μm data, with few exceptions where it was scaled from Re,100 (measured at 100 μm), using Re,70 = 0.85 × Re,100. These are marked 100 in the Band column. (8) 40–120 μm far-infrared luminosity. (9) Swift-BAT extremely hard X-ray luminosity.

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