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Home All issues Volume 659 (March 2022) A&A, 659 (2022) A125 Full HTML
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Table 2.

AGN host galaxy properties inferred from SED modeling.

Object z(a) (b) (c) (d) (e) SFRIR(f) (g)
HE 0021−1810 0.054 < 43.67 < 43.98 < 3.7 < 6.8
HE 0021−1819 0.053 7.6 ± 2.1
HE 0040−1105 0.042 < 43.82 < 44.03 < 4.1 7.7 ± 1.7
HE 0045−2145 0.021 … 8.1 ± 0.4
HE 0108−4743 0.024 7.6 ± 0.6
HE 0114−0015 0.046 7.8 ± 2.9
HE 0119−0118 0.055 8.4 ± 0.8
HE 0150−0344 0.048 … 7.8 ± 3.4
HE 0203−0031 0.043 < 7.0
HE 0212−0059 0.026 … 7.9 ± 0.6
HE 0224−2834 0.060 < 44.06 < 44.38 < 9.3 7.9 ± 3.2
HE 0227−0913 0.016 7.2 ± 1.9
HE 0232−0900 0.043 8.6 ± 1.0
HE 0253−1641 0.032 8.0 ± 1.1
HE 0345+0056 0.031 < 43.84 < 44.13 < 5.2 < 6.7
HE 0351+0240 0.035 < 6.9
HE 0412−0803 0.038 < 6.8
HE 0429−0247 0.042 < 44.10 < 44.43 < 10.5 < 7.3
HE 0433−1028 0.036 8.6 ± 0.6
HE 0853−0126 0.060 < 44.05 < 44.42 < 10.1 8.2 ± 2.4
HE 0853+0102 0.053 < 7.2
HE 0934+0119 0.051 < 7.0
HE 0949−0122 0.020 7.2 ± 2.3
HE 1011−0403 0.059 8.2 ± 1.8
HE 1017−0305 0.049 < 44.10 < 44.45 < 11.0 8.0 ± 1.6
HE 1029−1831 0.041 8.4 ± 1.0
HE 1107−0813 0.059 < 44.46 < 44.87 < 28.6 8.0 ± 2.5
HE 1108−2813 0.024 8.2 ± 0.7
HE 1126−0407 0.060 8.2 ± 2.0
HE 1237−0504 0.008 7.2 ± 1.5
HE 1248−1356 0.015 7.3 ± 1.1
HE 1310−1051 0.034 < 6.8
HE 1330−1013 0.022 < 43.69 < 43.89 < 3.0 7.5 ± 1.8
HE 1338−1423 0.041 < 6.9
HE 1353−1917 0.035 8.1 ± 1.4
HE 1417−0909 0.044 < 43.39 < 43.67 < 1.8 < 6.7
HE 2128−0221 0.053 < 43.75 < 44.02 < 4.0 < 6.9
HE 2211−3903 0.040 8.0 ± 1.2
HE 2222−0026 0.058 < 44.11 < 44.46 < 11.2 7.4 ± 3.9
HE 2233+0124 0.057 8.0 ± 1.8
HE 2302−0857 0.047 8.2 ± 1.4

Notes.

(a)

Redshift directly measured from the CARS IFU data as reported in Husemann et al. (2022).

(b)

Stellar masses and 1σ uncertainties from stellar template fitting reported by AGNFitter.

(c)

Integrated luminosity of the torus template reported by AGNFitter.

(d)

Luminosity of the matched star-forming IR template reported by AGNFitter integrated over the 42.5−122.5 μm wavelength range.

(e)

Same as (d) but integrated over the full 8−1000 μm wavelength range.

(f)

Estimated SFR based on L8 − 1000 μm using calibration of Murphy et al. (2011), see Eq. (1).

(g)

CO(1−0) line luminosity based on the flux measurements from Bertram et al. (2007) and listed in Husemann et al. (2022).

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