The 2–10 keV intrinsic luminosity at the source frame, average bolometric correction factor, and the Eddington ratio as measured from the bolometric corrected 2–10 keV source luminosity are presented in columns (2), (3), and (4), respectively. The innermost stable circular orbit risco in units of rg and radiative efficiency η = rg/2risco are listed in columns (5) and (6), respectively. Columns (7) and (8) represent the dimensionless mass accretion rate |$\dot{m}=\frac{\dot{M}}{\dot{M}_{\rm E}}=\frac{L_{\rm bol}}{\eta L_{\rm E}}$| and Eddington accretion limit |$\dot{m}_{\rm E}=1/\eta$|, respectively.
| Source . | L2–10 keV . | κ . | Lbol/LE . | risco . | η . | |$\dot{m}$| . | |$\dot{m}_{\rm E}$| . |
|---|---|---|---|---|---|---|---|
| . | (1041 erg s−1) . | . | . | (rg) . | . | . | . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . |
| J0107 | |$31.3^{+0.7}_{-0.7}$| | 20|$^{+7}_{-7}$| | 0.28|$^{+0.48}_{-0.19}$| | |$2.5_{-0.6}^{+1.2}$| | |$0.20_{-0.06}^{+0.06}$| | |$1.4_{-1.1}^{+4.2}$| | |$5.0_{-1.1}^{+2.4}$| |
| J0228 | |$18.4^{+0.7}_{-0.7}$| | 18|$^{+6}_{-6}$| | 0.75|$^{+1.24}_{-0.50}$| | |$2.8_{-1.2}^{+0.4}$| | |$0.18_{-0.02}^{+0.14}$| | |$4.2_{-3.4}^{+8.7}$| | |$5.6_{-2.5}^{+0.9}$| |
| J0940 | |$37.7^{+0.8}_{-0.8}$| | 21|$^{+7}_{-7}$| | 0.36|$^{+0.59}_{-0.24}$| | |$1.3_{-0.05}^{+0.3}$| | |$0.38_{-0.07}^{+0.02}$| | |$0.9_{-0.6}^{+2.1}$| | |$2.6_{-0.1}^{+0.6}$| |
| J1023 | |$12.8^{+0.2}_{-0.2}$| | 16|$^{+6}_{-5}$| | 0.29|$^{+0.51}_{-0.19}$| | |$4.1_{-1.9}^{+0.6}$| | |$0.12_{-0.02}^{+0.11}$| | |$2.4_{-2.0}^{+5.1}$| | |$8.3_{-3.9}^{+1.2}$| |
| J1140 | |$38.2^{+0.3}_{-0.3}$| | 21|$^{+7}_{-8}$| | 0.45|$^{+0.76}_{-0.31}$| | |$1.7_{-0.2}^{+0.2}$| | |$0.3_{-0.03}^{+0.03}$| | |$1.5_{-1.1}^{+3.0}$| | |$3.4_{-0.3}^{+0.4}$| |
| J1347 | |$33.0^{+0.5}_{-0.5}$| | 20|$^{+7}_{-7}$| | 0.47|$^{+0.80}_{-0.32}$| | |$3.1_{-1.2}^{+1.8}$| | |$0.16_{-0.06}^{+0.10}$| | |$2.9_{-2.3}^{+9.4}$| | |$6.2_{-2.4}^{+3.6}$| |
| J1357 | |$85.3^{+1.9}_{-1.9}$| | 26|$^{+9}_{-9}$| | 1.0|$^{+1.7}_{-0.7}$| | |$4.8_{-0.6}^{+0.3}$| | |$0.10_{-0.01}^{+0.01}$| | |$9.6_{-6.8}^{+17.9}$| | |$9.6_{-1.2}^{+0.6}$| |
| J1434 | |$3.0^{+0.1}_{-0.1}$| | 13|$^{+5}_{-4}$| | 0.04|$^{+0.08}_{-0.03}$| | |$3.7_{-1.4}^{+1.7}$| | |$0.14_{-0.04}^{+0.08}$| | |$0.3_{-0.2}^{+1.0}$| | |$7.4_{-2.8}^{+3.4}$| |
| J1541 | |$37.5^{+1.2}_{-1.2}$| | 21|$^{+7}_{-8}$| | 0.35|$^{+0.59}_{-0.24}$| | |$2.3_{-0.7}^{+1.2}$| | |$0.22_{-0.08}^{+0.10}$| | |$1.6_{-1.2}^{+4.9}$| | |$4.5_{-1.4}^{+2.3}$| |
| J1559 | |$40.1^{+0.1}_{-0.1}$| | 21|$^{+7}_{-7}$| | 0.38|$^{+0.63}_{-0.25}$| | |$1.24_{-0.0}^{+0.4}$| | |$0.40_{-0.11}^{+0.0}$| | |$0.9_{-0.6}^{+2.5}$| | |$2.5_{-0.0}^{+0.9}$| |
| J1626 | |$3.8^{+0.2}_{-0.2}$| | 14|$^{+4}_{-5}$| | 0.08|$^{+0.12}_{-0.05}$| | |$3.5_{-1.7}^{+0.9}$| | |$0.14_{-0.03}^{+0.13}$| | |$0.5_{-0.4}^{+1.2}$| | |$7.0_{-3.3}^{+1.8}$| |
| J1631 | |$3.1^{+0.2}_{-0.2}$| | 13|$^{+5}_{-4}$| | 0.05|$^{+0.08}_{-0.03}$| | |$3.2_{-0.9}^{+0.8}$| | |$0.16_{-0.03}^{+0.06}$| | |$0.3_{-0.2}^{+0.7}$| | |$6.4_{-1.8}^{+1.6}$| |
| POX52 | |$4.8^{+0.1}_{-0.1}$| | 14|$^{+5}_{-5}$| | 0.15|$^{+0.15}_{-0.08}$| | |$4.0_{-1.8}^{+1.7}$| | |$0.12_{-0.04}^{+0.10}$| | |$1.2_{-0.9}^{+2.1}$| | |$8.0_{-3.6}^{+3.3}$| |
| Source . | L2–10 keV . | κ . | Lbol/LE . | risco . | η . | |$\dot{m}$| . | |$\dot{m}_{\rm E}$| . |
|---|---|---|---|---|---|---|---|
| . | (1041 erg s−1) . | . | . | (rg) . | . | . | . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . |
| J0107 | |$31.3^{+0.7}_{-0.7}$| | 20|$^{+7}_{-7}$| | 0.28|$^{+0.48}_{-0.19}$| | |$2.5_{-0.6}^{+1.2}$| | |$0.20_{-0.06}^{+0.06}$| | |$1.4_{-1.1}^{+4.2}$| | |$5.0_{-1.1}^{+2.4}$| |
| J0228 | |$18.4^{+0.7}_{-0.7}$| | 18|$^{+6}_{-6}$| | 0.75|$^{+1.24}_{-0.50}$| | |$2.8_{-1.2}^{+0.4}$| | |$0.18_{-0.02}^{+0.14}$| | |$4.2_{-3.4}^{+8.7}$| | |$5.6_{-2.5}^{+0.9}$| |
| J0940 | |$37.7^{+0.8}_{-0.8}$| | 21|$^{+7}_{-7}$| | 0.36|$^{+0.59}_{-0.24}$| | |$1.3_{-0.05}^{+0.3}$| | |$0.38_{-0.07}^{+0.02}$| | |$0.9_{-0.6}^{+2.1}$| | |$2.6_{-0.1}^{+0.6}$| |
| J1023 | |$12.8^{+0.2}_{-0.2}$| | 16|$^{+6}_{-5}$| | 0.29|$^{+0.51}_{-0.19}$| | |$4.1_{-1.9}^{+0.6}$| | |$0.12_{-0.02}^{+0.11}$| | |$2.4_{-2.0}^{+5.1}$| | |$8.3_{-3.9}^{+1.2}$| |
| J1140 | |$38.2^{+0.3}_{-0.3}$| | 21|$^{+7}_{-8}$| | 0.45|$^{+0.76}_{-0.31}$| | |$1.7_{-0.2}^{+0.2}$| | |$0.3_{-0.03}^{+0.03}$| | |$1.5_{-1.1}^{+3.0}$| | |$3.4_{-0.3}^{+0.4}$| |
| J1347 | |$33.0^{+0.5}_{-0.5}$| | 20|$^{+7}_{-7}$| | 0.47|$^{+0.80}_{-0.32}$| | |$3.1_{-1.2}^{+1.8}$| | |$0.16_{-0.06}^{+0.10}$| | |$2.9_{-2.3}^{+9.4}$| | |$6.2_{-2.4}^{+3.6}$| |
| J1357 | |$85.3^{+1.9}_{-1.9}$| | 26|$^{+9}_{-9}$| | 1.0|$^{+1.7}_{-0.7}$| | |$4.8_{-0.6}^{+0.3}$| | |$0.10_{-0.01}^{+0.01}$| | |$9.6_{-6.8}^{+17.9}$| | |$9.6_{-1.2}^{+0.6}$| |
| J1434 | |$3.0^{+0.1}_{-0.1}$| | 13|$^{+5}_{-4}$| | 0.04|$^{+0.08}_{-0.03}$| | |$3.7_{-1.4}^{+1.7}$| | |$0.14_{-0.04}^{+0.08}$| | |$0.3_{-0.2}^{+1.0}$| | |$7.4_{-2.8}^{+3.4}$| |
| J1541 | |$37.5^{+1.2}_{-1.2}$| | 21|$^{+7}_{-8}$| | 0.35|$^{+0.59}_{-0.24}$| | |$2.3_{-0.7}^{+1.2}$| | |$0.22_{-0.08}^{+0.10}$| | |$1.6_{-1.2}^{+4.9}$| | |$4.5_{-1.4}^{+2.3}$| |
| J1559 | |$40.1^{+0.1}_{-0.1}$| | 21|$^{+7}_{-7}$| | 0.38|$^{+0.63}_{-0.25}$| | |$1.24_{-0.0}^{+0.4}$| | |$0.40_{-0.11}^{+0.0}$| | |$0.9_{-0.6}^{+2.5}$| | |$2.5_{-0.0}^{+0.9}$| |
| J1626 | |$3.8^{+0.2}_{-0.2}$| | 14|$^{+4}_{-5}$| | 0.08|$^{+0.12}_{-0.05}$| | |$3.5_{-1.7}^{+0.9}$| | |$0.14_{-0.03}^{+0.13}$| | |$0.5_{-0.4}^{+1.2}$| | |$7.0_{-3.3}^{+1.8}$| |
| J1631 | |$3.1^{+0.2}_{-0.2}$| | 13|$^{+5}_{-4}$| | 0.05|$^{+0.08}_{-0.03}$| | |$3.2_{-0.9}^{+0.8}$| | |$0.16_{-0.03}^{+0.06}$| | |$0.3_{-0.2}^{+0.7}$| | |$6.4_{-1.8}^{+1.6}$| |
| POX52 | |$4.8^{+0.1}_{-0.1}$| | 14|$^{+5}_{-5}$| | 0.15|$^{+0.15}_{-0.08}$| | |$4.0_{-1.8}^{+1.7}$| | |$0.12_{-0.04}^{+0.10}$| | |$1.2_{-0.9}^{+2.1}$| | |$8.0_{-3.6}^{+3.3}$| |
The 2–10 keV intrinsic luminosity at the source frame, average bolometric correction factor, and the Eddington ratio as measured from the bolometric corrected 2–10 keV source luminosity are presented in columns (2), (3), and (4), respectively. The innermost stable circular orbit risco in units of rg and radiative efficiency η = rg/2risco are listed in columns (5) and (6), respectively. Columns (7) and (8) represent the dimensionless mass accretion rate |$\dot{m}=\frac{\dot{M}}{\dot{M}_{\rm E}}=\frac{L_{\rm bol}}{\eta L_{\rm E}}$| and Eddington accretion limit |$\dot{m}_{\rm E}=1/\eta$|, respectively.
| Source . | L2–10 keV . | κ . | Lbol/LE . | risco . | η . | |$\dot{m}$| . | |$\dot{m}_{\rm E}$| . |
|---|---|---|---|---|---|---|---|
| . | (1041 erg s−1) . | . | . | (rg) . | . | . | . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . |
| J0107 | |$31.3^{+0.7}_{-0.7}$| | 20|$^{+7}_{-7}$| | 0.28|$^{+0.48}_{-0.19}$| | |$2.5_{-0.6}^{+1.2}$| | |$0.20_{-0.06}^{+0.06}$| | |$1.4_{-1.1}^{+4.2}$| | |$5.0_{-1.1}^{+2.4}$| |
| J0228 | |$18.4^{+0.7}_{-0.7}$| | 18|$^{+6}_{-6}$| | 0.75|$^{+1.24}_{-0.50}$| | |$2.8_{-1.2}^{+0.4}$| | |$0.18_{-0.02}^{+0.14}$| | |$4.2_{-3.4}^{+8.7}$| | |$5.6_{-2.5}^{+0.9}$| |
| J0940 | |$37.7^{+0.8}_{-0.8}$| | 21|$^{+7}_{-7}$| | 0.36|$^{+0.59}_{-0.24}$| | |$1.3_{-0.05}^{+0.3}$| | |$0.38_{-0.07}^{+0.02}$| | |$0.9_{-0.6}^{+2.1}$| | |$2.6_{-0.1}^{+0.6}$| |
| J1023 | |$12.8^{+0.2}_{-0.2}$| | 16|$^{+6}_{-5}$| | 0.29|$^{+0.51}_{-0.19}$| | |$4.1_{-1.9}^{+0.6}$| | |$0.12_{-0.02}^{+0.11}$| | |$2.4_{-2.0}^{+5.1}$| | |$8.3_{-3.9}^{+1.2}$| |
| J1140 | |$38.2^{+0.3}_{-0.3}$| | 21|$^{+7}_{-8}$| | 0.45|$^{+0.76}_{-0.31}$| | |$1.7_{-0.2}^{+0.2}$| | |$0.3_{-0.03}^{+0.03}$| | |$1.5_{-1.1}^{+3.0}$| | |$3.4_{-0.3}^{+0.4}$| |
| J1347 | |$33.0^{+0.5}_{-0.5}$| | 20|$^{+7}_{-7}$| | 0.47|$^{+0.80}_{-0.32}$| | |$3.1_{-1.2}^{+1.8}$| | |$0.16_{-0.06}^{+0.10}$| | |$2.9_{-2.3}^{+9.4}$| | |$6.2_{-2.4}^{+3.6}$| |
| J1357 | |$85.3^{+1.9}_{-1.9}$| | 26|$^{+9}_{-9}$| | 1.0|$^{+1.7}_{-0.7}$| | |$4.8_{-0.6}^{+0.3}$| | |$0.10_{-0.01}^{+0.01}$| | |$9.6_{-6.8}^{+17.9}$| | |$9.6_{-1.2}^{+0.6}$| |
| J1434 | |$3.0^{+0.1}_{-0.1}$| | 13|$^{+5}_{-4}$| | 0.04|$^{+0.08}_{-0.03}$| | |$3.7_{-1.4}^{+1.7}$| | |$0.14_{-0.04}^{+0.08}$| | |$0.3_{-0.2}^{+1.0}$| | |$7.4_{-2.8}^{+3.4}$| |
| J1541 | |$37.5^{+1.2}_{-1.2}$| | 21|$^{+7}_{-8}$| | 0.35|$^{+0.59}_{-0.24}$| | |$2.3_{-0.7}^{+1.2}$| | |$0.22_{-0.08}^{+0.10}$| | |$1.6_{-1.2}^{+4.9}$| | |$4.5_{-1.4}^{+2.3}$| |
| J1559 | |$40.1^{+0.1}_{-0.1}$| | 21|$^{+7}_{-7}$| | 0.38|$^{+0.63}_{-0.25}$| | |$1.24_{-0.0}^{+0.4}$| | |$0.40_{-0.11}^{+0.0}$| | |$0.9_{-0.6}^{+2.5}$| | |$2.5_{-0.0}^{+0.9}$| |
| J1626 | |$3.8^{+0.2}_{-0.2}$| | 14|$^{+4}_{-5}$| | 0.08|$^{+0.12}_{-0.05}$| | |$3.5_{-1.7}^{+0.9}$| | |$0.14_{-0.03}^{+0.13}$| | |$0.5_{-0.4}^{+1.2}$| | |$7.0_{-3.3}^{+1.8}$| |
| J1631 | |$3.1^{+0.2}_{-0.2}$| | 13|$^{+5}_{-4}$| | 0.05|$^{+0.08}_{-0.03}$| | |$3.2_{-0.9}^{+0.8}$| | |$0.16_{-0.03}^{+0.06}$| | |$0.3_{-0.2}^{+0.7}$| | |$6.4_{-1.8}^{+1.6}$| |
| POX52 | |$4.8^{+0.1}_{-0.1}$| | 14|$^{+5}_{-5}$| | 0.15|$^{+0.15}_{-0.08}$| | |$4.0_{-1.8}^{+1.7}$| | |$0.12_{-0.04}^{+0.10}$| | |$1.2_{-0.9}^{+2.1}$| | |$8.0_{-3.6}^{+3.3}$| |
| Source . | L2–10 keV . | κ . | Lbol/LE . | risco . | η . | |$\dot{m}$| . | |$\dot{m}_{\rm E}$| . |
|---|---|---|---|---|---|---|---|
| . | (1041 erg s−1) . | . | . | (rg) . | . | . | . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . |
| J0107 | |$31.3^{+0.7}_{-0.7}$| | 20|$^{+7}_{-7}$| | 0.28|$^{+0.48}_{-0.19}$| | |$2.5_{-0.6}^{+1.2}$| | |$0.20_{-0.06}^{+0.06}$| | |$1.4_{-1.1}^{+4.2}$| | |$5.0_{-1.1}^{+2.4}$| |
| J0228 | |$18.4^{+0.7}_{-0.7}$| | 18|$^{+6}_{-6}$| | 0.75|$^{+1.24}_{-0.50}$| | |$2.8_{-1.2}^{+0.4}$| | |$0.18_{-0.02}^{+0.14}$| | |$4.2_{-3.4}^{+8.7}$| | |$5.6_{-2.5}^{+0.9}$| |
| J0940 | |$37.7^{+0.8}_{-0.8}$| | 21|$^{+7}_{-7}$| | 0.36|$^{+0.59}_{-0.24}$| | |$1.3_{-0.05}^{+0.3}$| | |$0.38_{-0.07}^{+0.02}$| | |$0.9_{-0.6}^{+2.1}$| | |$2.6_{-0.1}^{+0.6}$| |
| J1023 | |$12.8^{+0.2}_{-0.2}$| | 16|$^{+6}_{-5}$| | 0.29|$^{+0.51}_{-0.19}$| | |$4.1_{-1.9}^{+0.6}$| | |$0.12_{-0.02}^{+0.11}$| | |$2.4_{-2.0}^{+5.1}$| | |$8.3_{-3.9}^{+1.2}$| |
| J1140 | |$38.2^{+0.3}_{-0.3}$| | 21|$^{+7}_{-8}$| | 0.45|$^{+0.76}_{-0.31}$| | |$1.7_{-0.2}^{+0.2}$| | |$0.3_{-0.03}^{+0.03}$| | |$1.5_{-1.1}^{+3.0}$| | |$3.4_{-0.3}^{+0.4}$| |
| J1347 | |$33.0^{+0.5}_{-0.5}$| | 20|$^{+7}_{-7}$| | 0.47|$^{+0.80}_{-0.32}$| | |$3.1_{-1.2}^{+1.8}$| | |$0.16_{-0.06}^{+0.10}$| | |$2.9_{-2.3}^{+9.4}$| | |$6.2_{-2.4}^{+3.6}$| |
| J1357 | |$85.3^{+1.9}_{-1.9}$| | 26|$^{+9}_{-9}$| | 1.0|$^{+1.7}_{-0.7}$| | |$4.8_{-0.6}^{+0.3}$| | |$0.10_{-0.01}^{+0.01}$| | |$9.6_{-6.8}^{+17.9}$| | |$9.6_{-1.2}^{+0.6}$| |
| J1434 | |$3.0^{+0.1}_{-0.1}$| | 13|$^{+5}_{-4}$| | 0.04|$^{+0.08}_{-0.03}$| | |$3.7_{-1.4}^{+1.7}$| | |$0.14_{-0.04}^{+0.08}$| | |$0.3_{-0.2}^{+1.0}$| | |$7.4_{-2.8}^{+3.4}$| |
| J1541 | |$37.5^{+1.2}_{-1.2}$| | 21|$^{+7}_{-8}$| | 0.35|$^{+0.59}_{-0.24}$| | |$2.3_{-0.7}^{+1.2}$| | |$0.22_{-0.08}^{+0.10}$| | |$1.6_{-1.2}^{+4.9}$| | |$4.5_{-1.4}^{+2.3}$| |
| J1559 | |$40.1^{+0.1}_{-0.1}$| | 21|$^{+7}_{-7}$| | 0.38|$^{+0.63}_{-0.25}$| | |$1.24_{-0.0}^{+0.4}$| | |$0.40_{-0.11}^{+0.0}$| | |$0.9_{-0.6}^{+2.5}$| | |$2.5_{-0.0}^{+0.9}$| |
| J1626 | |$3.8^{+0.2}_{-0.2}$| | 14|$^{+4}_{-5}$| | 0.08|$^{+0.12}_{-0.05}$| | |$3.5_{-1.7}^{+0.9}$| | |$0.14_{-0.03}^{+0.13}$| | |$0.5_{-0.4}^{+1.2}$| | |$7.0_{-3.3}^{+1.8}$| |
| J1631 | |$3.1^{+0.2}_{-0.2}$| | 13|$^{+5}_{-4}$| | 0.05|$^{+0.08}_{-0.03}$| | |$3.2_{-0.9}^{+0.8}$| | |$0.16_{-0.03}^{+0.06}$| | |$0.3_{-0.2}^{+0.7}$| | |$6.4_{-1.8}^{+1.6}$| |
| POX52 | |$4.8^{+0.1}_{-0.1}$| | 14|$^{+5}_{-5}$| | 0.15|$^{+0.15}_{-0.08}$| | |$4.0_{-1.8}^{+1.7}$| | |$0.12_{-0.04}^{+0.10}$| | |$1.2_{-0.9}^{+2.1}$| | |$8.0_{-3.6}^{+3.3}$| |
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