Table B.1.
Moffat PSF model parameters estimated at the observed Mg II and [O II] wavelength of the science object.
| ID |
 |
 |
βMg II | ϕMg II |
![$ FWHM_{\mathrm{X}}^{\mathrm{[O\,II]}} $](/articles/aa/full_html/2024/07/aa49362-24/aa49362-24-eq115.gif){kind=small} |
![$ FWHM_{\mathrm{Y}}^{\mathrm{[O\,II]}} $](/articles/aa/full_html/2024/07/aa49362-24/aa49362-24-eq116.gif){kind=small} |
β[O II] | ϕ[O II] |
|---|---|---|---|---|---|---|---|---|
| [arcsec] | [arcsec] | [deg] | [arcsec] | [arcsec] | [deg] | |||
| J0047+0154 | 1.88 | – | 5.0 | – | 1.67 | – | 4.6 | – |
| J0130-0014 | 1.37 | 1.24 | 18.4 | 9.61 | 1.34 | 1.29 | > 20 | 9.59 |
| J0141-0304 | 0.88 | 0.73 | 4.1 | 3.21 | 0.76 | 0.72 | 3.9 | 4.8 |
| J0804+4726 | 1.99 | – | 4.7 | – | 1.86 | – | 3.9 | – |
| J0811+4141 | 1.94 | – | 5.0 | – | 1.74 | – | 4.6 | – |
| J0834+4805 | 2.0 | – | 4.9 | – | 1.95 | – | 4.7 | – |
| J0844+5312 | 1.25 | 1.15 | 3.3 | 179 | 1.14 | 1.04 | 3.3 | 0.01 |
| J0912+5050 | 2.09 | – | 6.7 | – | 1.91 | – | 5.8 | – |
| J0919+4906 | 1.85 | – | 3.6 | – | 1.74 | – | 3.5 | – |
| J0940+5932 | 1.99 | – | 4.0 | – | 1.85 | – | 4.1 | – |
| J1014+5501 | 1.69 | 1.35 | 5.8 | 1.59 | 1.51 | 1.23 | 4.8 | 0.01 |
| J1033+6353 | 1.66 | – | 4.9 | – | 1.55 | – | 4.8 | – |
| J1046+5827 | 0.99 | 0.97 | 3.5 | 91. | 0.91 | 0.96 | 3.9 | 91.13 |
| J1137+3605 | 0.99 | 0.99 | 3.6 | 91.1 | 0.9 | 0.96 | 3.9 | 91.13 |
| J1154+2443 | 0.94 | 0.88 | 4.8 | 89.5 | 0.94 | 0.92 | 5.5 | 89.52 |
| J1157+5801 | 1.02 | 0.99 | 3.4 | 3.19 | 0.92 | 1.0 | 3.0 | 3.19 |
| J1243+4646 | 1.02 | 0.89 | 4.4 | 3.19 | 1.04 | 0.93 | 5.0 | 4.79 |
| J1256+4509 | 1.05 | 1.01 | 4.7 | 89.5 | 0.95 | 0.92 | 5.4 | 89.53 |
| J1352+5617 | 0.99 | 0.98 | 3.7 | 91.1 | 0.91 | 0.96 | 3.9 | 91.13 |
| J1503+3644 | 0.89 | 1.01 | 3.9 | 179 | – | – | – | – |
| J1517+3705 | 1.51 | – | 3.7 | – | 1.43 | – | 4.4 | – |
| J1648+4957 | 1.66 | – | 4.5 | – | 1.52 | – | 4.4 | – |
Notes. For the LRS2 observations, the PSF is close to circular and therefore only one value of FWHM is given (FWHMX). For KCWI observations, we provide the two spatial dimensions FWHMX and FWHMY as well as the rotation angle ϕ. β is the Moffat shape parameter. At the redshift of our sample (z ≈ 0.35) the Mg II and [O II] lines fall at ≈3785 Å and ≈5040 Å, respectively. The errors on the PSF parameters are on average 0.001″, 0.05, and 0.001 degree for the FWHM, β and ϕ values of the KCWI data respectively, and 0.02″ and 0.5 for the FWHM and β values of the LRS2 data respectively (see Appendix B).
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