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Table A.2.
Galactic ISM properties of each TDE line of sight.
| TDE | Filter | PMW | θMW | E(B − V)MW | Pserk |
|---|---|---|---|---|---|
| (%) | (°) | (mag) | (%) | ||
| AT2019aalc | L | 0.44 ± 0.07 | 76 ± 9 | 0.0454 ± 0.0005 | ≲0.59 |
| AT2019aalc | I | 0.4 ± 0.2 | 77 ± 8 | 0.0454 ± 0.0005 | ≲0.53 |
| AT2024bgz | L | 0.3 ± 0.1 | 42 ± 9 | 0.0447 ± 0.0006 | ≲0.58 |
| AT2020afhd | L | 0.4 ± 0.2 | 167 ± 6 | 0.066 ± 0.001 | ≲0.85 |
| AT2020afhd | I | 0.44 ± 0.08 | 162 ± 8 | 0.066 ± 0.001 | ≲0.76 |
| AT2024pvu | L | 0.50 ± 0.03 | 58 ± 4 | 0.058 ± 0.005 | ≲0.75 |
| AT2024wsd | L | 0.61 ± 0.02 | 60.8 ± 0.02 | 0.060 ± 0.001 | ≲0.78 |
Notes. The Galactic reddening E(B − V)MW is calculated for a 5′×5′ field statistic (Schlegel et al. 1998). The Pserk is the polarisation degree estimated from the Galactic reddening and the Serkowski law (Serkowski et al. 1975).
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