CARS host properties (cars_dr1.host_properties)

Unique identifier for the CARS target

Official designator from the Hamburg/ESO survey (HES)

Logarithm of median stellar mass inferred from SED MCMC fitting

Logarithm of 16% quantile of stellar mass inferred from SED MCMC fitting

Logarithm of 84% quantile of stellar mass inferred from SED MCMC fitting

Logarithm of median 1-30micron IR torus component luminosity inferred from SED MCMC fitting

Logarithm of 16% quantile of 1-30micron IR torus component luminosity from SED MCMC fitting

Logarithm of 84% quantile of 1-30micron IR torus component luminosity inferred from SED MCMC fitting

g-band AB magnitude of the AGN component after 2D image modelling

i-band AB magnitude of the AGN component after 2D image modelling

Logarithm of median 8-1000micron star-forming component luminosity inferred from SED MCMC fitting

Logarithm of 16% quantile of 8-1000micron star-forming component luminosity from SED MCMC fitting

Logarithm of 84% quantile of 8-1000micron star-forming component luminosity from SED MCMC fitting

Logarithm of median 42.5-122.5micron star-forming component luminosity inferred from SED MCMC fitting

Logarithm of 16% quantile of 42.5-122.5micron star-forming component luminosity from SED MCMC fitting

Logarithm of 84% quantile of 42.5-122.5micron star-forming component luminosity´ from SED MCMC fitting

Flag indicating if log_L_IR, log_L_FIR, SFR_IR are 5sigma upper limits

median IR-based star formation rate using the conversion in Murphy et al. (2011)

16% quantile of IR-based star formation rate using the conversion in Murphy et al. (2011)

84% quantile of IR-based star formation rate using the conversion in Murphy et al. (2011)

extinction-corrected Ha flux solely taken below the Kewley et al. (2001,2006) maximum starburst BPT demarcation line

error of the extinction-corrected Ha flux

SFR estimated from the corresponding Halpha luminosity using the Calzetti 2007 calibration

Standard error of SFR estimated from the corresponding Halpha luminosity using the Calzetti 2007 calibration

Classification of BPT diagram appearance used for the rainbow decomposition of Ha fluxes as described in Smirnova-Pinchukova et al. (2021)

extinction-corrected Ha flux after applying a decomposition of ionization source with the rainbow algorithm as desribed in Smirnova-Pinchukova et al. (2021)

standard error of the extinction-corrected Ha flux

median Ha-based SFR after BPT rainbow analysis using the conversion in Calzetti et al. (2007)

Standar error of Ha-based SFR after BPT rainbow analysis

Flag indicating if Ha_flux_BPT, and SFR_Ha_BPT are 5sigma upper limits

area of the host galaxy with any detectable ionized gas emission lines

fraction of the ionized gas area classified to originate from the star-forming region in the BPT

fraction of the ionized gas area classified to originate from the LINER region in the BPT

fraction of the ionized gas area classified to originate from the intermediate region in the BPT

fraction of the ionized gas area classified to originate from the AGN region in the BPT

Projected maximum angular extent of the ENLR

Projected maximum physical extent of the ENLR

Projected angular extent of the ENLR at a limiting surface brightness of 10⁻15 erg/s/cm2/arcsec2/(1+z)4

Projected maximum physical extent of the ENLR at a limiting surface brightness of 10⁻15 erg/s/cm2/arcsec2/(1+z)4

Projected angular extent of the ENLR at a limiting surface brightness of 10⁻16 erg/s/cm2/arcsec2/(1+z)4

Projected maximum physical extent of the ENLR at a limiting surface brightness of 10⁻16 erg/s/cm2/arcsec2/(1+z)4

Projected angular extent of the ENLR at a limiting surface brightness of 10⁻17 erg/s/cm2/arcsec2/(1+z)4

Projected maximum physical extent of the ENLR at a limiting surface brightness of 10⁻17 erg/s/cm2/arcsec2/(1+z)4

Resolution limit of the ENLR size in kpc

ENLR size error in arcsec

ENLR size error in kpc

radial gradient of 12+log(O/H) based on the N2S2 index using r_eff as the radial scale. Absolute reference metallicity scale is following the N2S2 calibration

12+log(O/H) abundance based on the N2S2 index at the galaxy centre from the radial fit. Absolute reference metallicity scale is following the N2S2 calibration

radial gradient of 12+log(O/H) based on the N2S2 index using r_eff as the radial scale. Absolute reference metallicity scale is following the N2S2 calibration

12+log(O/H) abundance based on the N2S2 index at the galaxy centre from the radial fit. Absolute reference metallicity scale is following the N2S2 calibration

radial gradient of 12+log(O/H) based on the N2S2 index using r_eff as the radial scale. Absolute reference metallicity scale is following the Tremonti04 SDSS calibration

12+log(O/H) abundance based on the N2S2 index at the galaxy centre from the radial fit. Absolute reference metallicity scale is following the Tremonti04 SDSS calibration

radial gradient of 12+log(O/H) based on the N2S2 index using r_eff as the radial scale. Absolute reference metallicity scale is following the Tremonti04 SDSS calibration

12+log(O/H) abundance based on the N2S2 index at the galaxy centre from the radial fit. Absolute reference metallicity scale is following the Tremonti04 SDSS calibration