Table B.3
LTT 3780 RV analysis priors and parameters
| Parameter | Units | Prior | Posterior |
|---|---|---|---|
| γCARMENES | m/s | 𝒩(μCARMENES, σCARMENES)1 | ![]() |
| γHARPS,a | m/s | 𝒩(μHARPS,a, σHARPS,a)1 | −0.9 ± 0.5 |
| γHARPS-N | m/s | 𝒩(μHARPS-N, σHARPS-N)1 | ![]() |
| γMAROON-X,b | m/s | 𝒩(μMAROON-X,b, σMAROON-X,b)1 | 1.1 ± 0.3 |
| γMAROON-X,r | m/s | 𝒩(μMAROON-X,r, σMAROON-X,r)1 | ![]() |
| γNIRPS | m/s | 𝒩(μNIRPS, σNIRPS)1 | ![]() |
| ρGP | days | 𝒩(104, 15)2 | ![]() |
| log τ | days | 𝒰(log (2PGP), log (100PGP)) | ![]() |
| log σCARMENES | m2/s2 | 𝒰(−5, 5) | ![]() |
| log σHARPS,a | m2/s2 | 𝒰(−5, 5) | ![]() |
| log σHARPS-N | m2/s2 | 𝒰(−5, 5) | ![]() |
| log σMAROON-X,b | m2/s2 | 𝒰(−5, 5) | ![]() |
| log σMAROON-X,r | m2/s2 | 𝒰(−5, 5) | ![]() |
| log σNIRPS | m2/s2 | 𝒰(−5, 5) | ![]() |
| log Kb | m/s | 𝒰(−5, 5) | 1.18 ± 0.04 |
| Kb | m/s | _4 | 3.26 ± 0.14 |
| Pb | days | 𝒮𝒩(0.76837931, 0.00000042, 0.00000039)3 | 0.7683793 ± 0.0000004 |
| t0,b | BJD-2450000 | 𝒮𝒩(9606.58098, 0.00040,0.00032)3 | 9606.5810 ± 0.0004 |
| log Kc | m/s | 𝒰(−5, 5) | 1.47 ± 0.03 |
| Kc | m/s | _4 | 4.35 ± 0.13 |
| Pc | days | 𝒩(12.252284, 0.000013)3 | 12.25228 ± 0.00001 |
| t0,c | BJD-2450000 | 𝒮𝒩(9600.54227, 0.00065,00066)3 | 9600.5423 ± 0.0007 |
| hc | − | 𝒰(−1, 1) | ![]() |
| kc | − | 𝒰(−1, 1) | ![]() |
| ec | − | _4 | < 0.11 |
| Mb | M⊕ | _3 | 2.34 ± 0.10 |
| Mc | M⊕ | _3 | 7.89 ± 0.26 |
The priors and posteriors of the planetary and GP parameters for the LTT 3780 system. LTT 3780 b was restricted to have an eccentricity of 0 due to its short period; the eccentricity of LTT 3780 c was allowed to vary. The MAROON-X, r and MAROON-X, b subscripts refer to the red and blue MAROON-X data respectively; the HARPS, a subscript refers to the archival HARPS data (as opposed to the HARPS data taken simultaneously with NIRPS, which was not included for lack of information content.) 𝒮𝒩 refers to a split-normal distribution, parameterized as 𝒮𝒩(μ, σ−, σ+).
1 Normal distribution, based on the mean and standard deviation of the data points fit from this instrument.
2 Obtained from Cloutier et al. (2020).
3 Obtained from Bonfanti et al. (2024).
4 Derived from other parameters.
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