DNS and candidate sources. The columns are: pulsar name, magnetic field strength of the recycled millisecond pulsar (A) and the young pulsar (B), periods of the two pulsars, and the gravitational decay times. Decay times longer than 50 Gyr are denoted as ∞. The full set of parameters is known only for double pulsar J0737 + 3039A/B. The parameters from the first four systems of the table were used in Figs 6 and 7. The data for J1946 + 2052 are from Stovall et al. (2018). The data for all other systems were taken from Tauris et al. (2017) table 1 and references therein.
| Pulsar name . | BA . | BB . | PA . | PB . | τGW . |
|---|---|---|---|---|---|
| . | (109 G) . | (109 G) . | (ms) . | (ms) . | (Myr) . |
| J0737 − 3039 | 6.4 | 1590 | 22.7 | 2773.5 | 86 |
| J1946 + 2052 | 4.0 | – | 17 | – | 46 |
| J1913 + 1102 | 2.12 | – | 27.3 | – | 480 |
| B1913 + 16 | 22.8 | – | 59.0 | – | 301 |
| J0453 + 1559 | 3.0 | – | 45.8 | – | 2730 |
| J1518 + 4904 | 1.07 | – | 40.9 | – | ∞ |
| B1534 + 12 | 9.7 | – | 37.9 | – | ∞ |
| J1753 − 2240 | 9.7 | – | 95.1 | – | ∞ |
| J1755 − 2550a | – | 880 | – | 315.2 | ∞ |
| J1756 − 2251 | 5.5 | – | 28.5 | – | 1660 |
| J1811 − 1736 | 9.8 | – | 104.2 | – | ∞ |
| J1829 + 2456 | 1.48 | – | 41.0 | – | ∞ |
| J1906 + 0746a | – | 1730 | – | 144.1 | 309 |
| J1930 − 1852 | 58.5 | – | 185.5 | – | ∞ |
| J1807 − 2500Ba | 0.59 | – | 4.19 | – | ∞ |
| B2127 + 11C | 12.5 | – | 30.5 | – | 217 |
| Pulsar name . | BA . | BB . | PA . | PB . | τGW . |
|---|---|---|---|---|---|
| . | (109 G) . | (109 G) . | (ms) . | (ms) . | (Myr) . |
| J0737 − 3039 | 6.4 | 1590 | 22.7 | 2773.5 | 86 |
| J1946 + 2052 | 4.0 | – | 17 | – | 46 |
| J1913 + 1102 | 2.12 | – | 27.3 | – | 480 |
| B1913 + 16 | 22.8 | – | 59.0 | – | 301 |
| J0453 + 1559 | 3.0 | – | 45.8 | – | 2730 |
| J1518 + 4904 | 1.07 | – | 40.9 | – | ∞ |
| B1534 + 12 | 9.7 | – | 37.9 | – | ∞ |
| J1753 − 2240 | 9.7 | – | 95.1 | – | ∞ |
| J1755 − 2550a | – | 880 | – | 315.2 | ∞ |
| J1756 − 2251 | 5.5 | – | 28.5 | – | 1660 |
| J1811 − 1736 | 9.8 | – | 104.2 | – | ∞ |
| J1829 + 2456 | 1.48 | – | 41.0 | – | ∞ |
| J1906 + 0746a | – | 1730 | – | 144.1 | 309 |
| J1930 − 1852 | 58.5 | – | 185.5 | – | ∞ |
| J1807 − 2500Ba | 0.59 | – | 4.19 | – | ∞ |
| B2127 + 11C | 12.5 | – | 30.5 | – | 217 |
aSources may have companion white dwarfs.
DNS and candidate sources. The columns are: pulsar name, magnetic field strength of the recycled millisecond pulsar (A) and the young pulsar (B), periods of the two pulsars, and the gravitational decay times. Decay times longer than 50 Gyr are denoted as ∞. The full set of parameters is known only for double pulsar J0737 + 3039A/B. The parameters from the first four systems of the table were used in Figs 6 and 7. The data for J1946 + 2052 are from Stovall et al. (2018). The data for all other systems were taken from Tauris et al. (2017) table 1 and references therein.
| Pulsar name . | BA . | BB . | PA . | PB . | τGW . |
|---|---|---|---|---|---|
| . | (109 G) . | (109 G) . | (ms) . | (ms) . | (Myr) . |
| J0737 − 3039 | 6.4 | 1590 | 22.7 | 2773.5 | 86 |
| J1946 + 2052 | 4.0 | – | 17 | – | 46 |
| J1913 + 1102 | 2.12 | – | 27.3 | – | 480 |
| B1913 + 16 | 22.8 | – | 59.0 | – | 301 |
| J0453 + 1559 | 3.0 | – | 45.8 | – | 2730 |
| J1518 + 4904 | 1.07 | – | 40.9 | – | ∞ |
| B1534 + 12 | 9.7 | – | 37.9 | – | ∞ |
| J1753 − 2240 | 9.7 | – | 95.1 | – | ∞ |
| J1755 − 2550a | – | 880 | – | 315.2 | ∞ |
| J1756 − 2251 | 5.5 | – | 28.5 | – | 1660 |
| J1811 − 1736 | 9.8 | – | 104.2 | – | ∞ |
| J1829 + 2456 | 1.48 | – | 41.0 | – | ∞ |
| J1906 + 0746a | – | 1730 | – | 144.1 | 309 |
| J1930 − 1852 | 58.5 | – | 185.5 | – | ∞ |
| J1807 − 2500Ba | 0.59 | – | 4.19 | – | ∞ |
| B2127 + 11C | 12.5 | – | 30.5 | – | 217 |
| Pulsar name . | BA . | BB . | PA . | PB . | τGW . |
|---|---|---|---|---|---|
| . | (109 G) . | (109 G) . | (ms) . | (ms) . | (Myr) . |
| J0737 − 3039 | 6.4 | 1590 | 22.7 | 2773.5 | 86 |
| J1946 + 2052 | 4.0 | – | 17 | – | 46 |
| J1913 + 1102 | 2.12 | – | 27.3 | – | 480 |
| B1913 + 16 | 22.8 | – | 59.0 | – | 301 |
| J0453 + 1559 | 3.0 | – | 45.8 | – | 2730 |
| J1518 + 4904 | 1.07 | – | 40.9 | – | ∞ |
| B1534 + 12 | 9.7 | – | 37.9 | – | ∞ |
| J1753 − 2240 | 9.7 | – | 95.1 | – | ∞ |
| J1755 − 2550a | – | 880 | – | 315.2 | ∞ |
| J1756 − 2251 | 5.5 | – | 28.5 | – | 1660 |
| J1811 − 1736 | 9.8 | – | 104.2 | – | ∞ |
| J1829 + 2456 | 1.48 | – | 41.0 | – | ∞ |
| J1906 + 0746a | – | 1730 | – | 144.1 | 309 |
| J1930 − 1852 | 58.5 | – | 185.5 | – | ∞ |
| J1807 − 2500Ba | 0.59 | – | 4.19 | – | ∞ |
| B2127 + 11C | 12.5 | – | 30.5 | – | 217 |
aSources may have companion white dwarfs.
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