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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