Table 1
Results from the modelling process for the 38 stars analysed with minimal or negligible contamination in the TESS aperture.
| Name | TIC | Morphology | Known binary? | 𝓑10 | 𝓑30 | 𝓑31 | BestModel |
|---|---|---|---|---|---|---|---|
| Abell 63 | 1842385646 | B | Yes | – | |||
| Abell 46 | 423311936 | E | Yes | PHOEBE | |||
| DS 1 | 120596335 | I | yes | PHOEBE | |||
| Abell 30 | 331986754 | R | Yes | >100 | >100 | −0.2 | 1E |
| LoTr 5 | 357307129 | E | Yes | >100 | >100 | >100 | 1E |
| PG 1520+525 | 193990614 | R | No | 13.5 | 7.5 | −5.9 | 1E |
| PNG 136.7+61.9 | 471013481 | na | No | 34.4 | 1.9 | −32.5 | 1E |
| Pa 165 | 367508287 | I | No | 23.9 | 20.2 | −3.6 | 1E |
| NGC 2867 | 387196603 | E | No | 13.3 | 16.7 | 3.4 | 1E |
| WPS 28 | 229966905 | na | no | 41.0 | 24.3 | −16.7 | 1E |
| Fr1-4 | 401795856 | na | No | 23.6 | 2.6 | −21.0 | 1E |
| NGC 7094 | 387371712 | E | No | >100 | >100 | −2.1 | 1E |
| RWT 152 | 65145453 | S | No | 34.9 | 17.8 | −17.1 | 1E |
| NGC 2371 | 446005482 | B | No | 25.5 | 20.8 | −4.7 | 1E |
| NGC 7293 | 69813909 | B | No | 74.4 | 70.2 | −4.2 | 1E |
| Hen 3-1863 | 290274851 | S | No | >100 | >100 | <−100 | 1E |
| WPS 54 | 453444667 | na | No | >100 | >100 | −20.8 | 1E |
| NGC 5189 | 341689253 | B | Yes | >100 | >100 | >100 | 3E |
| NGC 246 | 3905338 | E | Yes | 22.7 | 31.3 | 8.5 | 3E |
| NGC 2392 | 60947424 | E | Yes | >100 | >100 | > 100 | 3E |
| IC 2149 | 440340055 | B | No | > 100 | >100 | >100 | 3E |
| NGC 1501 | 84306468 | E | No | >100 | > 100 | 95.6 | 3E |
| PG 1034+001 | 124598476 | na | No | >100 | >100 | > 100 | 3E |
| IC 4593 | 119955971 | E | No | >100 | >100 | > 100 | 3E |
| K 1-16 | 233689607 | B | No | 24.6 | 36.8 | 12.2 | 3E |
| HDW 7 | 760317391 | R | No | −1.3 | −8.0 | −6.7 | FL |
| JnEr 1 | 741726060 | B | No | −2.8 | −8.3 | −5.5 | FL |
| Abell 28 | 471015303 | R | No | −0.9 | −7.1 | −6.2 | FL |
| EC 13290-1933 | 32145732 | na | No | −2.9 | −7.9 | −5.0 | FL |
| Abell 31 | 444036737 | E | No | −1.4 | −6.6 | −5.2 | FL |
| Abell 7 | 169305167 | E | No | −2.4 | −10.1 | −7.8 | FL |
| StDr 56(*) | 63505607 | na | No | −0.3 | −5.6 | −5.2 | FL |
| Fr 2-21(*) | 352568802 | na | no | 4.5 | 5.0 | 0.5 | FL |
| Sh 2-216 | 391260920 | R | No | −4.0 | −15.7 | −11.6 | FL |
| Fr 2-46 | 92709449 | na | No | −4.0 | −10.4 | −6.4 | FL |
| Lo1 | 146711168 | B | no | −1.9 | −8.6 | −6.6 | FL |
| IC 5148/50 | 2027562015 | R | No | −3.3 | −5.1 | −1.8 | FL |
| AMU 1(**) | 63373833 | B | Yes | −0.6 | −9.1 | −8.5 | FL |
Notes. (*)Although both StDr 56 and Fr 2-21 converge to a flat model, they have significant signals in their periodograms so we think they deserve a more detailed analysis (see Section 4.3). (**)AMU 1 has a confirmed binary system in the nucleus, detected with Kepler data.
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