The overall |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| in favour of Model BPL (equation 14) over Model PL (equation 13), using all available IPTA data, for different Solar system ephemeris models.
| Ephemeris . | |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| . | |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| (without PSR . |
|---|---|---|
| . | . | J1024−0719) . |
| DE405 | −0.4 | 0.3 |
| DE418 | −1.0 | −0.3 |
| DE421 | 0.2 | 0.8 |
| DE430 | −0.1 | 0.7 |
| DE435 | −0.8 | −0.1 |
| Ephemeris . | |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| . | |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| (without PSR . |
|---|---|---|
| . | . | J1024−0719) . |
| DE405 | −0.4 | 0.3 |
| DE418 | −1.0 | −0.3 |
| DE421 | 0.2 | 0.8 |
| DE430 | −0.1 | 0.7 |
| DE435 | −0.8 | −0.1 |
The overall |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| in favour of Model BPL (equation 14) over Model PL (equation 13), using all available IPTA data, for different Solar system ephemeris models.
| Ephemeris . | |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| . | |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| (without PSR . |
|---|---|---|
| . | . | J1024−0719) . |
| DE405 | −0.4 | 0.3 |
| DE418 | −1.0 | −0.3 |
| DE421 | 0.2 | 0.8 |
| DE430 | −0.1 | 0.7 |
| DE435 | −0.8 | −0.1 |
| Ephemeris . | |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| . | |$\log \mathcal {B}^{\text{BPL}}_{\text{PL}}$| (without PSR . |
|---|---|---|
| . | . | J1024−0719) . |
| DE405 | −0.4 | 0.3 |
| DE418 | −1.0 | −0.3 |
| DE421 | 0.2 | 0.8 |
| DE430 | −0.1 | 0.7 |
| DE435 | −0.8 | −0.1 |
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