Catalogue of ultraluminous X-ray sources in extragalactic globular clusters

This table lists all known ultraluminous X-ray sources (with detected X-ray emission above \(10^{39}\) erg/s) in extragalactic globular clusters, along with their observed X-ray and optical properties.

Source Properties:

Name Host galaxy Peak L_X X-ray Spectrum Behaviour Counterpart Optical Emission Magnitude (z) Colour (g-z) r_H (pc) Notes References
RZ2109 NGC 4472 3e39 0.15 keV FV, LV C [OIII] 20.4 0.84 BH?, U? Maccarone et al., 2007
CXOKMZJ033831.7-353058 NGC 1399 2e39 0.3 keV FV,T C ? 22.02(R) 2.04(C-R) Shih et al., 2010
CXOJ033831.8-352604 NGC 1399 2e39 0.4 keV LV? C [OIII],[NII] 21.275 1.6 R Cor Bor? Irwin et al., 2010
CXOUJ1229410+075744 NGC 4472 3e39 1.5 keV LV C ND 20.8 1.59 BH? Maccarone et al., 2011
CXOUJ124346.9+113234 NGC 4649 2e39 1.5 LV C ND 20.3 1.55 Roberts et al., 2012
CXOU1229345+0800320 NGC 4472 1e39 1.3keV N PC ? 22.1 0.92 Dage et al., 2019
CXOU1229423+08000808 NGC 4472 1e39 1.3keV N PC ? 19.5 1.11 Dage et al., 2019
CXOUJ1229345+0758515 NGC 4472 1e39 1.5 N PC ? 20.1 1.55 Dage et al., 2019
CXOU1243445+11315 NGC 4649 1e39 1.5 N PC ? 22.2 1.6 Dage et al., 2019
CXOUJ1243445+11315 NGC 1399 4e39 1.3 LV C ? 20.49 1.37 Dage et al., 2019
SC302 M87 1.5e39 1.0 keV FV C ? 19.76 1.01 UCD? Dage et al., 2020
CXOUJ123054.9+122438.5 M87 1e39 0.8 keV LV PC ? 22.56 1.70 1.88 Dage et al., 2020
CXOUJ123049.24+122334.5 M87 0.8e39 0.6 keV LV PC ? 21.66 1.08 2.20 Dage et al., 2020
CXOUJ123047.12+122416.0 M87 1.6e39 0.5 keV LV? PC ? 21.73/22.55 1.05/1.61 3.69/1.96 Dage et al., 2020
CXOUJ123050.1+122301.1 M87 1e39 1.0 keV LV PC ? 20.47 1.29 1.82 Dage et al., 2020
CXOUJ123049.9+122400.1 M87 1.1e39 1.5 N? PC ? 20.85 1.42 2.53 Dage et al., 2020
CXOUJ123041.7+122440.1 M87 1e39 1.5 keV N? PC ? 20.41 1.24 2.70 Dage et al., 2020
CXOUJ032242.5-371222 NGC 1316 1.4e39 1.6keV N PC ? 20.88 1.67 Dage et al., 2021
CXOUJ032241.0-371235.3 NGC 1316 1e39 1.3keV N PC ? 21.98 1.49 Dage et al., 2021
CXOUJ032240.8-371224 NGC 1316 2e39 0.7-2.0 keV N PC ? 23.10 0.94 Dage et al., 2021