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Table 3
Proposed classification scheme for the two-Gaussian fits on Gaia-sampled Kepler data.
| Class | Class description | Subclass | Class # | Subclass description | No. of sources | % |
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| D | detached binaries | D-1 | 1 | one conspicuous eclipse | 429 | 21 |
| D-2 | 2 | two conspicuous eclipses | 105 | 5 | ||
| D+SD | detached and semi-detached | D+SD-1 | 3 | one conspicuous eclipse | 178 | 9 |
| D+SD-2 | 4 | two conspicuous eclipses | 180 | 9 | ||
| SD+CB | semi-detached and contact binaries | / | 5 | 208 | 10 | |
| CB | contact binaries | / | 6 | 115 | 6 | |
| CB+ELV | contact binaries and ellipsoidal variables | CB+ELV-a | 7 | eclipse depth ratio <1 | 212 | 11 |
| CB+ELV-b | 8 | eclipse depth ratio ~1 | 403 | 20 | ||
| ELF | ellipsoidal fits | / | 9 | 172 | 9 | |
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