Table 1.
Galaxy properties: X-shooter, and SINFONI observation lists of our sample of galaxies.
| Properties |
X-shooter |
SINFONI |
|||||||
|---|---|---|---|---|---|---|---|---|---|
| Object name | Dist | Morph | log L | Obs. Date | AirM | Seeing | Obs. Date | AirM | Seeing |
| (Mpc) | (erg s−1) | (DD/MM/YY) | (″) | (DD/MM/YY) | (″) | ||||
| 1 | 2 | 3 | 4A | 5 | 6 | 7 | 8 | 9 | 10 |
| ESO 137-G034 | 35 | S0a(AB) | 42.76 | 19/05/19 | 1.2 | 0.78 | 18/04/14 | 1.2 | 0.75 |
| ESO 021-G004 | 39 | SA(s)0/a | 42.70 | 02/08/16 | 1.8 | 0.83 | – | – | – |
| MCG-05-14-12 | 41 | S0 | 42.65 | 11/12/13 | 1.0 | 0.61 | – | – | – |
| MCG-05-23-16 | 35 | S0 | 43.50 | 22/01/14 | 1.1 | 1.21 | 14/01/17 | 1.1 | 1.00 |
| MCG-06-30-15 | 27 | S? | 42.91 | 16/01/15 | 1.1 | 0.83 | 04/06/14 | 1.1 | 1.08 |
| NCG 1365 | 18 | Sb (B) | 42.60 | 10/12/13 | 1.0 | 1.34 | 18/11/10 | 1.1 | 0.78 |
| NGC 2110 | 27 | S? (AB) | 43.63 | 16/01/15 | 1.1 | 0.59 | 15/01/11 | 1.1 | 0.83 |
| NGC 2992 | 36 | Sa | 42.52 | 26/02/14 | 1.3 | 0.72 | 05/02/17 | 1.0 | 0.85 |
| NGC 3081 | 34 | (R)SAB(r)0/a | 43.29 | 20/02/14 | 1.2 | 0.82 | 14/03/17 | 1.2 | 0.76 |
| NGC 3783 | 38 | Sb (B) | 43.58 | 11/03/14 | 1.4 | 0.81 | 16/02/15 | 1.2 | 1.04 |
| NGC 4235 | 37 | Sa | 42.64 | 13/05/15 | 1.2 | 0.73 | – | – | – |
| NGC 4388 | 39 | SA(s)b (B) | 43.70 | – | – | – | 24/02/15 | 1.5 | 0.35 |
| NGC 4593 | 37 | Sb (B) | 43.20 | 10/03/14 | 1.3 | 0.80 | 23/01/15 | 1.1 | 0.88 |
| NGC 5128 | 3.8 | S0 p | 43.02 | 21/05/15 | 1.1 | 0.76 | – | – | – |
| NGC 5506 | 27 | Sa p | 43.30 | 03/03/16 | 1.1 | 0.64 | 12/03/15 | 1.098 | 0.72 |
| NGC 5728 | 39 | SAB(r)a: | 43.36 | 13/05/15 | 1.0 | 0.81 | 25/06/15 | 1.3 | 0.75 |
| NGC 6814 | 23 | SAB(rs)bc | 42.75 | 13/05/15 | 1.1 | 0.86 | 05/06/14 | 1.0 | 0.83 |
| NGC 7172 | 37 | Sa | 43.32 | 12/08/15 | 1.0 | 1.6 | 20/07/14 | 1.0 | 0.77 |
| NGC 7213 | 22 | Sa(s) | 42.49 | 13/07/16 | 1.3 | 0.47 | 16/07/14 | 1.1 | 0.83 |
| NGC 7582 | 22 | (R’)SB(s)ab (B) | 43.29 | 27/07/17 | 1.2 | 0.69 | 14/07/14 | 1.1 | 0.91 |
| 1 | 2 | 3 | 4B | 5 | 6 | 7 | 8 | 9 | 10 |
| ESO 093-G003 | 22 | SAB(r)0/a? | 9.86 | 22/01/14 | 1.3 | 0.98 | 06/04/17 | 1.4 | 0.86 |
| ESO 208-G021 | 17 | SAB0 | 10.88 | 12/12/13 | 1.1 | 0.95 | 14/03/17 | 1.2 | 1.02 |
| NGC 718 | 23 | SAB(s)a | 9.89 | 05/12/15 | 1.2 | 0.61 | 13/08/14 | 1.2 | 0.82 |
| NGC 1079 | 19 | (R)SAB(rs)0/a | 9.91 | 23/11/13 | 1.0 | 1.12 | 17/11/051 | 1.1 | 0.88 |
| NGC 1315 | 21 | SB0? | 10.07 | 11/12/13 | 1.0 | 0.83 | – | – | – |
| NGC 1947 | 19 | S0 p | 10.45 | 23/12/13 | 1.4 | 0.77 | – | – | – |
| NGC 2775 | 21 | SA(r)ab | 9.84 | 15/11/15 | 1.5 | 0.74 | – | – | – |
| NGC 3175 | 14 | SAB(s)a? | 10.07 | 09/03/14 | 1.2 | 1.13 | 06/04/17 | 1.0 | 0.88 |
| NGC 3351 | 11 | SB(r)b | 10.39 | 21/02/14 | 1.3 | 1.04 | 27/01/15 | 1.3 | 0.89 |
| NGC 3717 | 24 | SAb | 10.40 | 22/03/14 | 1.2 | 1.34 | – | – | – |
| NGC 3749 | 42 | SA(s)a | 10.48 | 22/03/14 | 1.0 | 0.93 | – | – | – |
| NGC 4224 | 41 | SA(s)a | 10.22 | 13/05/15 | 1.2 | 0.66 | 24/02/15 | 1.2 | 0.91 |
| NGC 4254 | 15 | SA(s)c | 10.22 | 02/06/16 | 1.3 | 0.77 | 09/03/15 | 1.5 | 0.84 |
| NGC 4260 | 31 | SB(s)a | 10.25 | – | – | – | – | – | – |
| NGC 5037 | 35 | SA(s)a | 10.30 | 13/05/15 | 1.0 | 0.70 | – | – | – |
| NGC 5845 | 25 | E | 10.46 | 16/03/16 | 1.2 | 0.69 | 14/03/17 | 1.2 | 0.61 |
| NGC 5921 | 21 | SB(r)bc | 10.08 | 16/06/15 | 1.2 | 0.71 | – | – | – |
| NGC 7727 | 26 | SAB(s)a p | 10.41 | 25/08/15 | 1.0 | 0.68 | 21/07/14 | 1.0 | 0.89 |
| IC 4653 | 26 | SB0/a(r) p | 9.48 | 19/05/2015 | 1.2 | 0.79 | 25/07/2017 | 1.6 | 1.11 |
Notes. Sector 1 (top): the LLAMA AGNs; Sector 2 (bottom): the LLAMA inactive galaxies. (1) Object name, (2) distance, (3) Galaxy morphology, (4) (a) logarithmic X-ray luminosity, (b) integrated H-band luminosity in logarithm in solar unit, (5) X-shooter observation date, (6) air mass during the observation, (7) seeing, (8) SINFONI observation date, (9) air mass during the observation, and (10) seeing. Galaxy morphologies and distances are taken from the NASA Extragalactic database. B and AB indicates the existence and absence of bar, respectively. The hard X-ray luminosities (14−195 keV) are taken from the Swift-BAT 70 months survey (Baumgartner et al. 2010), where X-ray luminosities were corrected for absorption based on X-ray fittings by Ricci et al. (2017a). The list of abbreviations: distance (Dist) observation (Obs), morphology (Morph), air mass (AirM), and peculiar (p). Seyfert types of the LLAMA AGNs are presented in Table 2.
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