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Table 7

Crossmatch between MUSE emission line galaxies and X-ray sources flagged as AGN from the Chandra 7Ms source catalogue (Luo et al. 2017).

ID z ID Separation X-ray flux z
MUSE Wide MUSE Chandra 7Ms (“) (erg/s/cm2) Chandra

102007068 0.338 304 0.20 2.982e-16 0.340
102008071 0.338 312 0.86 6.491e-17 0.336
102031144 0.665 290 0.20 3.498e-16 0.664
102037154 1.412 287 0.51 5.925e-17 1.413
103022086 0.670 322 0.24 1.510e-16 0.671
104014050 3.662 337 0.17 1.269e-15 3.660
106036089 0.904 344 0.82 6.638e-17 0.956a
106048103 0.665 340 0.15 2.406e-15 0.666
108025145 0.736 407 0.49 7.387e-17 0.736
109030090 1.044 447 0.17 5.737e-16 1.043
111004005 0.604 367 0.28 4.594e-15 0.604
113001007 0.232 508 0.94 2.411e-17 0.220a
113010038 0.577 460 0.35 2.778e-16 0.577
114024110 1.035 443 0.26 8.709e-16 1.036
114028115 1.098 509 0.30 1.525e-16 1.097
115003085 3.710 551 0.11 2.158e-15 3.700
116003060 1.364 634 0.14 3.899e-17 1.363b
117034085 0.228 693 1.13 6.435e-17 2.302
119034073 1.015 814 0.15 4.348e-15 1.016
120023032 1.118 861 0.25 1.744e-16 1.120
123005089 0.544 640 0.51 4.219e-17 0.552b
123051191 4.510 625 1.33 2.102e-17 2.616b

Notes. All reshifts quoted are spectroscopic from extensive identification campaigns except for objects marked with a and b which are photometric redshifts from Skelton et al. (2014) or Hsu et al. (2014), respectively.

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