Table 6
CME candidates.
| No | SDSS ID | RA | Dec | Type | Flare | S∕N bin | Lines with wing enhancement |
|---|---|---|---|---|---|---|---|
| 1 | J052700.12+010136.8 | 81.75054 | 1.02691 | M 3.2e* [1] known WTT[2] | No | High | Hα, Hβ, Hγ |
| 2 | J085556.66+174942.0 | 133.98612 | 17.82835 | M 4e[3] | Yes | High | Hα, Hβ, Hγ |
| 3 | J110743.30+075624.9 | 166.93047 | 7.94027 | M 4e[3] | No | High | Hα, Hβ, Hγ, Hδ, Hϵ, H8 |
| 4 | J042139.64+264913.8 | 65.41520 | 26.82050 | M 6e*[4] | Yes | Medium | Hα, Hβ, Hγ, Hδ |
| 5 | J053709.91-011050.3 | 84.29134 | −1.18067 | M 5e*[5] known WTT[6] | Yes | high | Hα,Hβ,Hγ,Hδ,Hϵ,H8,CaIIH&K |
| 6 | J052839.66-000322.5 | 82.16528 | −0.05627 | M 4e[3] | Yes | high | Hα, Hβ, Hγ, Hδ |
Notes. Listed properties including SDSS ID, right ascension and declination, spectral subtype, if an associated flare is visible, S/N bin, and the lines showing the enhancement. Significant enhancements in line wings (above all error bars) are marked in bold font. *The “e” for emission line star was added to these stars based on the visual inspection.
References. Spectral type sources: [1] Suárez et al. (2017), [2] McGehee (2006), [3] West et al. (2011), [4] Luhman et al. (2017), [5] Briceño et al. (2019), [6]Koenig et al. (2015).
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