Table A.3.
List of optical fluxes for our sample of AGN.
| Name | RA | De | z | Type | [OII]3727Å | [NeIII]3868Å | ... | [SII]6717,31Å | F(Hβ) | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | ... | (11) | (12) | (13) |
| IRAS00198-7926 | 00h21m53.6141s | -79d10m07.9572s | 0.07 | S2 | - | - | ... | 0.96±0.30 | 4.42±1.83 | LUM01 |
| NGC185 | 00h38m57.8837s | +48d20m14.6616s | -0.0007 | S2 | - | - | ... | 4.5±1.0 | 0.09±0.24 | HO97 |
| MCG-01-24-012 | 09h20m46.2653s | -08d03m21.9564s | 0.020 | S2 | 4.56±0.08 | 1.27±0.03 | ... | 1.86±0.03 | 1.04±0.21 | KOS17 |
| NGC4593 | 12h39m39.4550s | -05d20m39.0156s | 0.009 | S1.0 | 0.10±0.03 | 0.12±0.03 | ... | 0.023±0.007 | 367±57 | MOR88,MAL17 |
| NGC5506 | 14h13m14.8757s | -03d12m27.6984s | 0.006 | S1h | 8.0±2.2 | 1.83±0.48 | ... | 1.92±0.42 | 139±23 | MAL17,SHU80, |
| DUR88 | ||||||||||
| IRAS08572+3915 | 09h00m25.3829s | +39d03m54.2988s | 0.058 | ULIRG | 2.707±0.49 | - | ... | 1.22±0.18 | 1.11±0.47 | RUP08 |
| Arp299A | 11h28m33.7s | +58d33m49s | 0.010 | LIRG | - | - | ... | 0.69±0.10 | 21.2±2.1 | GAR06 |
| NGC6240 | 16h52m58.8862s | +02d24m0.36288s | 0.024 | LIN | 45.9±12.5 | 0.99±0.26 | ... | 3.43±1.06 | 89.99±15.55 | MAL17,CON12 |
Notes. Column (1): name of the galaxy. Columns (2) and (3): coordinates. Column (4): redshift. Column (5): spectral type. Columns (6)-(11): optical emission line fluxes and their errors relative to Hβ emission and reddening-corrected. Column (12): sum of emission lines [S II]6717Å and [S II]6731Å relative to Hβ emission and reddening-corrected. Column (13): Flux of hydrogen line Hβ and its error in 1e−14 erg/s/cm2 and reddening-corrected. Column (13): References for optical emission lines. The complete version of this table is available at the CDS.
References. BOK75 (Boksenberg et al. 1975), BUC06 (Buchanan et al. 2006), BUT09 (Buttiglione et al. 2009), CON12 (Contini 2012), COS77 (Costero & Osterbrock 1977), DUC97 (Duc et al. 1997), DUR88 (Durret & Bergeron 1988), ERK97 (Erkens et al. 1997), GAR06 (García-Marín et al. 2006), GOO83 (Goodrich & Osterbrock 1983), GU06 (Gu et al. 2006), HO93 (Ho et al. 1993), HO97 (Ho et al. 1997), KIM95 (Kim et al. 1995), KIM98 (Kim et al. 1998), KOS78 (Koski 1978), KOS17 (Koss et al. 2017), KRA94 (Kraemer et al. 1994), LUM01 (Lumsden et al. 2001), MAL86 (Malkan 1986), MAL17 (Malkan et al. 2017), MOR88 (Morris & Ward 1988), MOO96 (Moorwood et al. 1996), MOU06 (Moustakas & Kennicutt 2006), OLI94 (Oliva et al. 1994), OST75 (Osterbrock & Miller 1975), OST76 (Osterbrock & Koski 1976), OST93 (Osterbrock & Martel 1993), PAS79 (Pastoriza 1979), PHI78 (Phillips 1978), PHI83 (Phillips et al. 1983), RUP08 (Rupke et al. 2008), SHA07 (Shang et al. 2007), SHU80 (Shuder 1980), SIM98 (Simpson & Meadows 1998), STO97 (Storchi-Bergmann et al. 1997), VAC97 (Vaceli et al. 1997), VEI99 (Veilleux et al. 1999), WES85 (Westin 1985), WIL79 (Wilson & Penston 1979), WIN92 (Winkler 1992), WU98 (Wu et al. 1998)
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