Table 6.
Rotation periods taken from the literature or derived from ZTF light curves for 197 M35 members.
| ID | Prot (d) | Prot (d) | Class (a) | Subclass (b) | Blend (c) | Prot (d) | Flag (d) | Prot (d) | Type (e) | Prot (d) | Final |
|---|---|---|---|---|---|---|---|---|---|---|---|
| M09 | SF20 | SF20 | SF20 | SF20 | L16 | L16 | N15 | N15 | ZTF | prot (d) | |
| 5483 | – | – | – | – | – | 0.48 | 1 | 0.48 | Rot | 0.48 | 0.48 |
| 7118 | 1.10 | 1.11 | Rotating | RotVar | 0 | 1.11 | 1 | 1.10 | Rot | 1.11 | 1.11 |
| 5356 | – | – | – | – | – | – | – | – | – | 7.01 | 7.01 |
| 5459 | 7.30 | – | – | – | – | 7.19 | 1 | – | – | – | 7.30 |
| 7076 | – | 2.44 | Rotating | RotVar | 0 | – | – | – | – | – | 2.44 |
| ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes. This table is only partially presented. Its complete version is available at the CDS.
Rotating accounts for rotational variables, Pulsating for pulsating variables, EB for eclipsing binaries, and Misc for indeterminate variables.
RotVar accounts for rotational variables of indeterminate type, GDor for γ Doradus pulsators, EB for eclipsing binaries, and Misc for indeterminate variables.
0 = high probability that it is a blend; 1 = candidate variable; 2 = difficult to classify; 30 = difficult to classify star that, by comparison with the literature, could be a possible blend; 31 = difficult to classify star for which a correspondence in the literature was found.
Rot are rotating stars, EB eclipsing binaries, Long-Period long-period variables, and delta Sct δ Scuti stars.
References. M09 is Meibom et al. (2009), SF20 is Soares-Furtado et al. (2020), N15 is Nardiello et al. (2015), and L16 is Libralato et al. (2016).
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