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Table 1.

Summary of AGN and host galaxy properties of the COS-AGNi GA-NIFS sample.

Target RA Dec zspec Type log NH log L2−10keV log Lbol log M SFR A V tot $ A_{\mathrm {V}}^{\mathrm {tot}} $ A V nar $ A_{\mathrm {V}}^{\mathrm {nar}} $
(deg) (deg) (cm−2) (erg s−1) (erg s−1) (M) (M yr−1) (mag) (mag)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
COS590 149.755412 +2.73853 3.52385 ± 0.00002 1 <23.2 44.41 45.57 ± 0.14 10.7 ± 0.07 <11 0.6±0.1 1.3±0.1
COS1118 149.879192 +2.22584 3.64300 ± 0.00003 1 <20 44.30 45.2 ± 0.15 10.48 ± 0.17 <43 1.1±0.1 0.9±0.1
COS349 150.004377 +2.03892 3.5093 ± 0.0003 1 <20 44.26 46.17 ± 0.02 <10.56 <116 0.9±0.1a
COS1656-A 150.271546 +1.61383 3.5101 ± 0.0004 2 44.43 <45.84 10.95 ± 0.04 <80 2.2±0.9
COS2949 150.402917 +1.87889 2.0478 ± 0.0003 2 23.65 0.23 + 0.28 $ {}^{+0.28}_{-0.23} $ 44.48 0.26 + 0.24 $ {}^{+0.24}_{-0.26} $ 45.36 ± 0.11 10.44 ± 0.1 57 ± 2 3.2±0.1b
COS1638* <23.5 44.50 46.78 ± 0.02 11.08 ± 0.19 1947 ± 58
      COS1638-A 150.735557 +2.19953 3.5057 ± 0.0001 1 46.7 ± 0.3 0.9±0.1a 1.2±0.1
      COS1638-B 150.735847 +2.19962 3.5109 ± 0.0001 2 46.2 ± 0.3 4.2±0.8

Notes. (1) Target ID; (2)-(3) Coordinates; (4) Spectroscopic redshift determined from the narrow component of the [O III] line; (5) AGN Type; (6)-(7) Column density and X-ray luminosity from Marchesi et al. (2016); (8)-(10) SED fitting results (AGN bolometric luminosity, stellar mass, star formation rate; Circosta et al., in prep.); (11)-(12) Dust extinction for total emission and narrow components, respectively.

*

: The parameters of COS1638 refer to X-ray data and SED fitting performed on photometry that are spatially integrated over AGNi A and B of this dual system.

: Bolometric luminosity as measured in Perna et al. (2025b).

: Dual AGN that is not spatially resolved in COSMOS-Legacy, X-ray parameters are referred to the integrated system.

: X-ray properties estimated from dedicated fitting of the X-ray spectrum using the spectroscopic redshift measured in this work.

a

: Dust extinction measured as the median of the other Type 1 COS-AGNi (COS1118, COS590).

b

: Dust extinction measured as the median of the other Type 2 COS-AGNi (COS1638-B, COS1656-A).

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