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Table B.1.
Coefficients and their errors of second-order polynomial fits to the ratios of the XSL spectra to our MUSE spectra: Ratio = a0 + a1 × λ + a2 × λ2.
| ID | a0 | a1 | a2 | σ |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| [B86] 133 | 1.0875e+01 ± 4.9106e−01 | −2.6034e−03 ± 1.4250e−04 | 2.1119e−07 ± 1.0070e−08 | 8.9657e−01 |
| HD 057060 | 7.7783e+00 ± 1.5925e−01 | 4.1637e−04 ± 4.6240e−05 | 5.4824e−08 ± 3.2693e−09 | 2.9142e−01 |
| HD 064332 | 3.5697e+01 ± 3.4877e−01 | −3.9873e−03 ± 1.0127e−04 | 2.0084e−07 ± 7.1597e−09 | 6.3832e−01 |
| HD 067507 | −2.1863e+00 ± 6.3861e−01 | 3.2643e−03 ± 1.8542e−04 | −1.9423e−07 ± 1.3110e−08 | 1.1688e+00 |
| HD 085405 | −2.1686e+01 ± 3.6461e−01 | 7.1684e−03 ± 1.0587e−04 | −4.3791e−07 ± 7.4850e−09 | 6.6732e−01 |
| HD 096446 | 9.9209e−01 ± 7.7207e−03 | −1.4847e−05 ± 2.2418e−06 | 1.3103e−09 ± 1.5850e−10 | 1.4131e−02 |
| HD 099648 | 5.1713e+00 ± 6.3635e−02 | 3.6673e−04 ± 1.8477e−05 | −2.7750e−08 ± 1.3064e−09 | 1.1647e−01 |
| HD 099998 | 6.1662e+00 ± 7.5652e−02 | 3.3898e−05 ± 2.1966e−05 | −1.2490e−08 ± 1.5530e−09 | 1.3847e−01 |
| HD 100733 | 5.1682e+01 ± 4.3041e−01 | −8.1477e−03 ± 1.2497e−04 | 6.4140e−07 ± 8.8351e−09 | 7.8776e−01 |
| HD 101712 | 1.6022e+01 ± 2.3634e−01 | −7.1526e−04 ± 6.8618e−05 | 4.8079e−08 ± 4.8512e−09 | 4.3258e−01 |
| HD 101712 | 6.7516e+00 ± 2.2716e−01 | 1.4180e−03 ± 6.5952e−05 | −8.2102e−08 ± 4.6627e−09 | 4.1578e−01 |
| HD 102212 | 5.0144e+01 ± 8.6927e−01 | −3.0969e−03 ± 2.5240e−04 | 3.6520e−07 ± 1.7845e−08 | 1.5910e+00 |
| HD 114960 | 4.0233e+01 ± 9.7355e−01 | −5.0542e−03 ± 2.5999e−04 | 4.4436e−07 ± 1.7128e−08 | 7.8302e−01 |
| HD 147550 | 2.1748e+00 ± 2.1553e−02 | 2.0414e−04 ± 6.2580e−06 | −1.4080e−08 ± 4.4245e−10 | 3.9450e−02 |
| HD 160346 | 5.7738e+00 ± 6.3278e−02 | −1.7415e−04 ± 1.8292e−05 | 1.1002e−08 ± 1.2900e−09 | 1.1465e−01 |
| HD 160365 | 4.5644e+00 ± 3.9193e−02 | 3.6423e−05 ± 1.1329e−05 | −4.6190e−09 ± 7.9902e−10 | 7.1011e−02 |
| HD 163810 | 3.6215e+00 ± 4.3395e−02 | −7.4719e−05 ± 1.2544e−05 | 2.6363e−09 ± 8.8470e−10 | 7.8619e−02 |
| HD 164257 | 2.9161e+00 ± 2.1773e−02 | −1.9122e−04 ± 6.3208e−06 | 1.3446e−08 ± 4.4681e−10 | 3.9867e−02 |
| HD 167278 | 7.6624e+00 ± 5.1776e−02 | −4.5347e−04 ± 1.4967e−05 | 2.0024e−08 ± 1.0555e−09 | 9.3807e−02 |
| HD 170820 | 5.0225e+00 ± 3.4454e−02 | −6.4631e−04 ± 1.0002e−05 | 4.1002e−08 ± 7.0704e−10 | 6.3086e−02 |
| HD 172230 | 2.4422e+00 ± 2.7921e−02 | 1.0172e−04 ± 8.0709e−06 | −5.0514e−09 ± 5.6920e−10 | 5.0586e−02 |
| HD 173158 | 8.3642e+00 ± 4.7810e−02 | −1.5581e−03 ± 1.3820e−05 | 1.0331e−07 ± 9.7467e−10 | 8.6622e−02 |
| HD 174966 | 4.5597e+00 ± 1.9866e−02 | −3.4119e−04 ± 5.7425e−06 | 2.3893e−08 ± 4.0499e−10 | 3.5995e−02 |
| HD 175640 | 2.5360e+00 ± 1.8827e−02 | 3.5332e−05 ± 5.4655e−06 | −2.5504e−09 ± 3.8634e−10 | 3.4474e−02 |
| HD 179821 | 2.8459e+00 ± 9.0632e−02 | −1.1607e−04 ± 2.6310e−05 | 1.3874e−08 ± 1.8598e−09 | 1.6596e−01 |
| HD 193281A | 2.9758e+00 ± 1.7990e−02 | −3.8776e−05 ± 5.2226e−06 | 5.5744e−09 ± 3.6918e−10 | 3.2940e−02 |
| HD 193896 | 3.5954e+00 ± 2.2904e−02 | −2.7330e−04 ± 6.6490e−06 | 1.9823e−08 ± 4.7000e−10 | 4.1936e−02 |
| HD 196892 | 3.9280e+00 ± 2.3032e−02 | −4.0473e−04 ± 6.6862e−06 | 2.8704e−08 ± 4.7263e−10 | 4.2171e−02 |
| HD 200081 | 2.0961e+00 ± 2.5504e−02 | 1.2569e−04 ± 7.4035e−06 | −5.3440e−09 ± 5.2332e−10 | 4.6702e−02 |
| HD 204155 | 3.0281e+00 ± 2.9675e−02 | −8.6000e−05 ± 8.5776e−06 | 4.6207e−09 ± 6.0491e−10 | 5.3764e−02 |
| HD 209290 | −3.2922e+00 ± 5.5030e−02 | 1.6589e−03 ± 1.5975e−05 | −9.6328e−08 ± 1.1292e−09 | 1.0076e−01 |
| HD 232078 | 2.5877e+00 ± 8.0086e−02 | −5.7710e−05 ± 2.3251e−05 | 9.4294e−09 ± 1.6436e−09 | 1.4658e−01 |
| HD 306799 | 1.5678e+01 ± 2.1450e−01 | −1.0232e−03 ± 6.2275e−05 | 5.6597e−08 ± 4.4024e−09 | 3.9253e−01 |
| IRAS 15060+0947 | −1.0062e+01 ± 7.1662e+00 | −4.3525e−03 ± 1.9079e−03 | 1.4548e−06 ± 1.2536e−07 | 5.5817e+00 |
Notes. The standard deviation of the residuals σ is also listed.
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