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Table 1.

Main properties of the four targets studied in this work, along with the Keck OSIRIS observational setup.

Target RA Dec PA IPDfmp Redshift Band Texp × Nexp FWHM Seeing AO
J1026+6023 10:26:31.13 +60:23:30.13 102° 21 1.660 Hn5 900 s ×4 0.10″ 0.7″ LGS
J1608+2716 16:08:29.23 +27:16:26.74 −357° 14 2.575 Kn5 900 s ×6 0.09″ 0.7″ LGS
J1613+1708 16:13:20.01 +17:08:39.40 135° 14 1.547 Hbb 900 s ×4 0.11″ 0.7″ LGS
J2335+3201 23:35:22.52 +32:01:09.08 −106° 13 0.904 Jbb 600 s ×2 0.42″ 0.9″ NGS

Notes. We note that IPDfmp is the value of the ipd_frac_multi_peak parameter of the Gaia archive used for the GMP selection. Redshift were obtained from SDSS ground-based spectra, as reported in the Milliquas catalog. FWHMs were calculated on isolated sources. The seeing corresponds to the DIMM (Differential Image Motion Monitor) seeing mean value (at zenith, at 0.5 μm), as reported by the Maunakea Weather Center (http://mkwc.ifa.hawaii.edu/current/seeing/) for the same night of the observations.

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