Table A.1.
List of IR fluxes for our sample of AGN.
| Name | RA | De | z | Type | Brα | Pfα | [S IV]10.5μm | ... | [N II]122μm | [N II]205μm | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | ... | (20) | (21) | (22) |
| IRAS00198-7926 | 00h21m53.6141s | -79d10m07.9572s | 0.07 | S2 | - | - | 8.1±0.4 | ... | - | - | FO16,TW |
| NGC185 | 00h38m57.8837s | +48d20m14.6616s | -0.0007 | S2 | - | - | - | ... | - | - | FO16,TW |
| MCG-01-24-012 | 09h20m46.2653s | -08d03m21.9564s | 0.020 | S2 | - | - | 2.33±0.39 | ... | - | - | FO16,TW |
| NGC4593 | 12h39m39.4550s | -05d20m39.0156s | 0.009 | S1.0 | - | - | 3.9±0.6 | ... | 2.1±0.3 | - | FO16,TW |
| NGC5506 | 14h13m14.8757s | -03d12m27.6984s | 0.006 | S1h | - | - | 73.5±1.6 | ... | 14.1±1.2 | - | FO16,TW |
| IRAS08572+3915 | 09h00m25.3829s | +39d03m54.2988s | 0.058 | ULIRG | 2.53±0.25 | - | - | ... | 0.74±0.15 | - | ARM07,VEI09, |
| HC18,YAN21 | |||||||||||
| Arp299A | 11h28m33.7s | +58d33m49s | 0.010 | LIRG | - | - | 5.52±1.11 | ... | 10.05±0.78 | - | ALO00,INA13, |
| - | - | PEN21,SPI21 | |||||||||
| NGC6240 | 16h52m58.8862s | +02d24m0.36288s | 0.024 | LIN | 6.6±1.8 | - | 2.6±0.27 | ... | 23.15±2.22 | 18.46±0.39 | INA18,FO16 |
Notes. Column (1): name of the galaxy. Columns (2) and (3): coordinates. Column (4): redshift. Column (5): spectral type. Columns (6)-(21): IR emission line fluxes and their errors in 1e−14 erg/s/cm2. Column (22): references for hydrogen recombination line fluxes. The complete version of this table is available at the CDS.
References. ALO00 (Alonso-Herrero et al. 2000), ARM07 (Armus et al. 2007), B-S09 (Bernard-Salas et al. 2009), BEL03 (Bellamy et al. 2003), BEL04 (Bellamy & Tadhunter 2004), BEN04 (Bendo & Joseph 2004), BRA08 (Brauher et al. 2008), DAN05 (Dannerbauer et al. 2005), FO16 (Fernández-Ontiveros et al. 2016), GOL95 (Goldader et al. 1995), HC18 (Herrera-Camus et al. 2018), IMA04 (Imanishi & Wada 2004), IMA10 (Imanishi et al. 2010), INA13 (Inami et al. 2013), INA18 (Inami et al. 2018), LAM17 (Lamperti et al. 2017), LAN96 (Lancon et al. 1996), LUT02 (Lutz et al. 2002), MAR10 (Martins et al. 2010), MUE11 (Müller-Sánchez et al. 2011), MUR01 (Murphy et al. 2001), PEN21 (Peng et al. 2021), PIQ12 (Piqueras López et al. 2012), PS17 (Pereira-Santaella et al. 2017), REU02 (Reunanen et al. 2002), REU03 (Reunanen et al. 2003), RIF06 (Riffel et al. 2006), SEV01 (Severgnini et al. 2001), SMA12 (Smajić et al. 2012), SPI21 (Spinoglio et al. 2022), VEI97 (Veilleux et al. 1997), VEI09 (Veilleux et al. 2009), YAN21 (Yano et al. 2021), TW (This work).
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