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Table 1.

Basic information about the GPs with X-ray detections.

Source LAMOST RA Dec Redshift deVRad_r ( * ) cModelMag_r ( * ) EW([O iii]λ5007)
obsid (deg) (deg) (arcsec) mag [Å]
J1330−0043 436715102 202.5529 −0.717766 0.2385 0.22 ± 0.07 19.77 ± 0.03 31.32 ± 5.61
J0035+0431 767313017 8.810202 4.525338 0.3695 0.15 ± 0.04 19.65 ± 0.02 22.30 ± 1.06
J0205+1504 866310055 31.337868 15.0712304 0.2491 0.14 ± 0.03 19.66 ± 0.02 24.42 ± 4.40
J0227+2355 386613234 36.872930 23.924930 0.2575 0.12 ± 0.03 19.95 ± 0.03 62.32 ± 1.76
J1605+4405 902705057 241.462475 44.094555 0.3202 0.14 ± 0.02 19.13 ± 0.01 458.90 ± 2.91
J0906+0242 797002178 136.6335 2.712472 0.2691 0.11 ± 0.05 19.67 ± 0.02 17.53 ± 0.99

J0749+3337 (1) 117.403215 33.621219 0.2733 0.53 ± 0.02 18.35 ± 0.01 236.15 ± 14.45
J0822+2241 (1) 125.698590 22.695578 0.2163 0.23 ± 0.02 18.61 ± 0.01 939.28 ± 265.63
J1339+1516 (2) 204.867933 15.278369 0.1920 0.12 ± 0.02 18.80 ± 0.01 1173.51 ± 316.50

Notes. ( * )Obtained from SDSS DR18. https://skyserver.sdss.org/dr18/

(1)With X-ray detections from XMM-Newton, see Svoboda et al. (2019), Kawamuro et al. (2019) for reference. These two sources are named GP1 and GP2 in Svoboda et al. (2019).

(2)With X-ray non-detection from XMM-Newton, see Svoboda et al. (2019) for reference. This source is named GP3 in Svoboda et al. (2019).

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