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Table 1

DR3 quality flags and parameters used for HVS candidates, in particular for the 72 nearest extreme candidates studied in Sect. 3

Quantity/criterion DR3 column Critical values (? among 72) Remark
Throughout the paper:
RPlx parallax_over_error >5 (11) High priority
3–5 (61) Low priority

Sect. 3.1:
close NNs (11) Own NN search in DR3
IPD fmp ipd_frac_multi_peak >0 (18)
IPD fow ipd_frac_odd_win >0(5)
S olved astrometric_params_solved =95(10) Six-parameter solution
Dup duplicated_source >0(1)

Sects. 3.3; 3.4:
N per visibility_periods_used <med (22;41)
e_Plx parallax_error >q75 (15;26) in [mas]
e_pmRA pmra_error >q75 (15;25) in [mas yr−1]
e_pmDE pmdec_error >q75 (15; 26) in [mas yr−1]
go fAL astrometric_gof_al >q75 (36; 36) can be <0
epsi astrometric_excess_noise >q75 (33; 28) ≧0; in [mas]
sepsi astrometric_excess_noise_sig >q75 (35; 29)
amax astrometric_sigma5d_max >q75 (16; 23) in [mas]
IPDgofha ipd_gof_harmonic_amplitude >q75 (16; 18)
RUWE ruwe >q75 (37; 37)

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