| log |$L^{\rm obs}_{\rm X}$| . | |$\dot{N}_{p = 0}$| . | |$\dot{N}_{p = 4}$| . |
|---|---|---|
| [1] . | [2] . | [3] . |
| 40–41 | |$1.2^{+1.2}_{-0.7}\times 10^{-5}$| | |$1.1^{+1.1}_{-0.6}\times 10^{-5}$| |
| 41–42 | |$4.0^{+4.0}_{-2.3}\times 10^{-6}$| | |$3.8^{+3.8}_{-2.2}\times 10^{-6}$| |
| 42–43 | |$9.0^{+9.0}_{-5.1}\times 10^{-7}$| | |$8.6^{+8.6}_{-4.8}\times 10^{-7}$| |
| 43–44 | |$1.2^{+1.2}_{-0.7}\times 10^{-7}$| | |$1.1^{+1.1}_{-0.6}\times 10^{-7}$| |
| 44–45 | |$1.1^{+1.1}_{-0.6}\times 10^{-9}$| | |$4.8^{+4.7}_{-2.7}\times 10^{-10}$| |
| 45–46 | |$1.8^{+1.8}_{-1.0}\times 10^{-10}$| | |$3.8^{+3.8}_{-2.2}\times 10^{-11}$| |
| 46–47 | |$3.1^{+3.1}_{-1.8}\times 10^{-11}$| | |$6.6^{+6.6}_{-3.7}\times 10^{-12}$| |
| 47–48 | |$2.6^{+2.5}_{-1.4}\times 10^{-12}$| | |$5.4^{+5.4}_{-3.1}\times 10^{-13}$| |
| log |$L^{\rm obs}_{\rm X}$| . | |$\dot{N}_{p = 0}$| . | |$\dot{N}_{p = 4}$| . |
|---|---|---|
| [1] . | [2] . | [3] . |
| 40–41 | |$1.2^{+1.2}_{-0.7}\times 10^{-5}$| | |$1.1^{+1.1}_{-0.6}\times 10^{-5}$| |
| 41–42 | |$4.0^{+4.0}_{-2.3}\times 10^{-6}$| | |$3.8^{+3.8}_{-2.2}\times 10^{-6}$| |
| 42–43 | |$9.0^{+9.0}_{-5.1}\times 10^{-7}$| | |$8.6^{+8.6}_{-4.8}\times 10^{-7}$| |
| 43–44 | |$1.2^{+1.2}_{-0.7}\times 10^{-7}$| | |$1.1^{+1.1}_{-0.6}\times 10^{-7}$| |
| 44–45 | |$1.1^{+1.1}_{-0.6}\times 10^{-9}$| | |$4.8^{+4.7}_{-2.7}\times 10^{-10}$| |
| 45–46 | |$1.8^{+1.8}_{-1.0}\times 10^{-10}$| | |$3.8^{+3.8}_{-2.2}\times 10^{-11}$| |
| 46–47 | |$3.1^{+3.1}_{-1.8}\times 10^{-11}$| | |$6.6^{+6.6}_{-3.7}\times 10^{-12}$| |
| 47–48 | |$2.6^{+2.5}_{-1.4}\times 10^{-12}$| | |$5.4^{+5.4}_{-3.1}\times 10^{-13}$| |
*Col. [1]: Luminosity range. Col. [2]: Frequency of the TDE occurrence (Mpc−3 yr−1) in the corresponding luminosity range for log LX* = 44.6 and p = 0. Col. [3]: Same as Col. [2] but for p = 4.
| log |$L^{\rm obs}_{\rm X}$| . | |$\dot{N}_{p = 0}$| . | |$\dot{N}_{p = 4}$| . |
|---|---|---|
| [1] . | [2] . | [3] . |
| 40–41 | |$1.2^{+1.2}_{-0.7}\times 10^{-5}$| | |$1.1^{+1.1}_{-0.6}\times 10^{-5}$| |
| 41–42 | |$4.0^{+4.0}_{-2.3}\times 10^{-6}$| | |$3.8^{+3.8}_{-2.2}\times 10^{-6}$| |
| 42–43 | |$9.0^{+9.0}_{-5.1}\times 10^{-7}$| | |$8.6^{+8.6}_{-4.8}\times 10^{-7}$| |
| 43–44 | |$1.2^{+1.2}_{-0.7}\times 10^{-7}$| | |$1.1^{+1.1}_{-0.6}\times 10^{-7}$| |
| 44–45 | |$1.1^{+1.1}_{-0.6}\times 10^{-9}$| | |$4.8^{+4.7}_{-2.7}\times 10^{-10}$| |
| 45–46 | |$1.8^{+1.8}_{-1.0}\times 10^{-10}$| | |$3.8^{+3.8}_{-2.2}\times 10^{-11}$| |
| 46–47 | |$3.1^{+3.1}_{-1.8}\times 10^{-11}$| | |$6.6^{+6.6}_{-3.7}\times 10^{-12}$| |
| 47–48 | |$2.6^{+2.5}_{-1.4}\times 10^{-12}$| | |$5.4^{+5.4}_{-3.1}\times 10^{-13}$| |
| log |$L^{\rm obs}_{\rm X}$| . | |$\dot{N}_{p = 0}$| . | |$\dot{N}_{p = 4}$| . |
|---|---|---|
| [1] . | [2] . | [3] . |
| 40–41 | |$1.2^{+1.2}_{-0.7}\times 10^{-5}$| | |$1.1^{+1.1}_{-0.6}\times 10^{-5}$| |
| 41–42 | |$4.0^{+4.0}_{-2.3}\times 10^{-6}$| | |$3.8^{+3.8}_{-2.2}\times 10^{-6}$| |
| 42–43 | |$9.0^{+9.0}_{-5.1}\times 10^{-7}$| | |$8.6^{+8.6}_{-4.8}\times 10^{-7}$| |
| 43–44 | |$1.2^{+1.2}_{-0.7}\times 10^{-7}$| | |$1.1^{+1.1}_{-0.6}\times 10^{-7}$| |
| 44–45 | |$1.1^{+1.1}_{-0.6}\times 10^{-9}$| | |$4.8^{+4.7}_{-2.7}\times 10^{-10}$| |
| 45–46 | |$1.8^{+1.8}_{-1.0}\times 10^{-10}$| | |$3.8^{+3.8}_{-2.2}\times 10^{-11}$| |
| 46–47 | |$3.1^{+3.1}_{-1.8}\times 10^{-11}$| | |$6.6^{+6.6}_{-3.7}\times 10^{-12}$| |
| 47–48 | |$2.6^{+2.5}_{-1.4}\times 10^{-12}$| | |$5.4^{+5.4}_{-3.1}\times 10^{-13}$| |
*Col. [1]: Luminosity range. Col. [2]: Frequency of the TDE occurrence (Mpc−3 yr−1) in the corresponding luminosity range for log LX* = 44.6 and p = 0. Col. [3]: Same as Col. [2] but for p = 4.
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