Table A.1.
Sample of local (U)LIRGs.
| Object | Region | DL(a) | log LIR/L⊙(a) | log  (b) |
Ref.(b) | AGN (c) | Ref.(c) |
|---|---|---|---|---|---|---|---|
| (Mpc) | (erg s−1) | ||||||
| VV 114 E | SW-s1 | 85.5 | 11.71 | ⋯ | No/Obs.? | D23, R23, B24 | |
| SW-s2( † ) | ⋯ | ⋯ | ⋯ | B24, GA24 | |||
| NE | 41.02 | G06 | No/Obs.? | D23, R23, B24 | |||
| IRAS 05189−2524 | nucleus | 188 | 12.10 | 43.79 | I11 | Type 2 | P21 |
| IRAS 07251−0248 | E nucleus | 400 | 12.45 | 40.09 | I11, R21 | No/Obs. | P21, PS21 |
| IRAS 08572+3915 | NW nucleus | 261 | 12.15 | 41.31 | I11, R21 | LINER | V13 |
| IRAS 09111−1007 | W nucleus | 242 | 12.05 | 40.50 | I11 | LINER? | D97 |
| NGC 3256 | N nucleus | 38.9 | 11.64 | 40.39 | L02 | No | L00 |
| S nucleus | 39.73 | L02 | No/Obs. | O15 | |||
| outflow( * ) | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | |
| IRAS 13120−5453 | nucleus | 136 | 12.27 | 41.86 | R21 | Type 2 | P21 |
| IRAS 14348−1447 | NE nucleus | 375 | 12.41 | 41.12 | R21 | LINER?/Obs.? | P21, PS21 |
| SW nucleus | 41.53 | R21 | LINER?/Obs. | P21, PS21 | |||
| Arp 220 | W nucleus | 78 | 12.19 | 40.77 | C02 | LINER | P20 |
| E nucleus | 40.64 | C02 | LINER | P20 | |||
| II Zw 096 | D1 | 161 | 11.94 | 41.32 | I11 | No/Obs.? | I22, GB24 |
| C0( ‡ ) | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | |
| D0( ‡ ) | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | |
| IRAS 22491−1808 | E nucleus | 352 | 12.23 | 40.65 | I11 | No/Obs. | P21, PS21 |
| NGC 7469 | nucleus | 70.8 | 11.65 | 43.73 | B03, PS11 | Type 1 | O93, U22, A23, B24 |
Notes. (a) Luminosity distance and 8-1000 μm IR luminosity from Armus et al. (2009) and Pereira-Santaella et al. (2021). (b) Observed 2–10 keV X-ray luminosity and reference. (c) AGN classification based on optical spectroscopy and references. Obs. indicates dust obscured AGN based on indirect evidences from the mid-IR and sub-mm. “?” indicates inconclusive classification. ( † ) SW-s2 is located ∼100 pc away from the nucleus SW-s1. The highly excited CO and H2O mid-IR absorptions of this region were analyzed by González-Alfonso et al. (2024) and Buiten et al. (2024). ( * ) This region encompasses the collimated molecular outflow launched by the southern nucleus of NGC 3256. It is located ∼110 pc away from the nucleus and corresponds to region N1 of Pereira-Santaella et al. (2024). ( ‡ ) These two regions of II Zw 096 are bright star-forming clumps located 0.5–1 kpc from the nucleus D1 (Inami et al. 2022).
References. (A23) Armus et al. 2023; (B03) Blustin et al. 2003; (B24) Bianchin et al. 2024; (B24) Buiten et al. 2024; (C02) Clements et al. 2002; (D23) Donnan et al. 2023; (D97) Duc et al. 1997; (G06) Grimes et al. 2006; (GA24) González-Alfonso et al. 2024; (GB24) García-Bernete et al. 2024b; (I11) Iwasawa et al. 2011; (I22) Inami et al. 2022; (L00) Lípari et al. 2000; (L02) Lira et al. 2002; (O93) Osterbrock & Martel 1993; (O15) Ohyama et al. 2015; (P20) Perna et al. 2020; (P21) Perna et al. 2021; (PS11) Pereira-Santaella et al. 2011; (PS21) Pereira-Santaella et al. 2021; (R21) Ricci et al. 2021; (R23) Rich et al. 2023; (U22) Vivian et al. 2022; (V13) Veilleux et al. 2013.
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