Resulting parameters for our sample of absorbing galaxies.
|Quasar field||Host-galaxy identifiers
|θ⋆ (")||b (kpc)||log10[M⋆ (M⊙)]||SFR[O II] (M⊙ yr−1)||SFRHβ (M⊙ yr−1)||σ (km s−1)||[O/H] (dex)||[M/H]em (dex)|
|(mag) SED||(mag) BDEC||(mag) SFR|
|HE 1122-1649||3.6a||25.6||0.68249(3)||0.11||–||1.68 ± 0.23||1.55 ± 0.19||†||−0.84 ± 0.05|
|Q 0153+0009||4.9b||36.6||0.77085(3)||0.00||–||–||16.14 ± 1.54||††||0.04 ± 0.20|
|Q 1209+107 PA2||7.2b||38.3||0.39238(1)||0.68||≤0||3.20 ± 0.12||3.34 ± 0.09||∼8.05‡||0.30 ± 0.20|
|Q 1323–0021||1.4b||10.2||0.71717(8)||0.68||–||–||§||0.27 ± 0.03||–||–||0.62 ± 0.35|
|Q 1436–0051||6.2c||45.5||0.73749(3)||0.68||–||≤0||1.02 ± 0.07⋆⋆||0.48 ± 0.10||††||0.21 ± 0.12|
|Q 1436–0051||4.4b||34.9||0.92886(2)||1.02||–||–||–||–||–||0.21 ± 0.55|
|Q 2328+0022||1.7b||11.9||0.65194(6)||0.00||–||–||0.47 ± 0.05||–||–||−0.23 ± 0.22|
|Q 2335+1501||3.8d||27.0||0.67989(2)||1.36||–||4.47 ± 0.17||6.31 ± 2.51||†||0.33 ± 0.34|
Notes. Values for refer to the heliocentric rest-frame corrected measurement, with the bracket notation reflecting the uncertainty in the profile-fit. θ is the angular separation between quasar and host, measured in arcsec from known photometry. θ is translated into an impact parameter (b) measured in kpc using the the spectroscopically determined emission-line redshift and the assumed cosmology. refers to the nebular extinctions (SED, BDEC, SFR) derived from the χ2-minimising SED solution; the Balmer decrement; and based on the ratio of the SFR in Hα and [O II] under the assumption that they trace similar time-scales, respectively. Stellar mass estimates were determined from the maximum likelihood analysis of the SEDs χ2-distributions. The star-formation rate estimates were corrected for intrinsic and Galactic extinction, and were converted to a Chabrier IMF. σ corresponds to the velocity dispersion based on the profile fits to the emission lines after resolution correction using Eq. (1), and [O/H] to the preferred oxygen abundance derived from emission line ratios according to the M 08 prescriptions. [M/H]em refers to the metallicity in emission, inferred by applying a correction factor and truncation radius to the absorption metallicity.
Upper limit on EB−V imposed from dust-content priors (Sect. 3.6).
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