Table A.1.
VVV-PSF photometry for our Mira and LPV+ candidates(a)(b)
| ID | HJD | mag | e(mag) | bandpass | |
|---|---|---|---|---|---|
| 308501099316 | * | 58369.027430 | 14.939 | 0.025 | H |
| 308501099316 | * | 58373.991807 | 15.000 | 0.027 | H |
| 308501099316 | * | 58340.092523 | 18.090 | 0.166 | J |
| 308501099316 | * | 58369.040062 | 18.896 | 0.173 | J |
| 308501099316 | * | 58374.000068 | 18.293 | 0.165 | J |
| 308503118502 | 55497.008828 | 14.529 | 0.070 | Ks | |
| 308503118502 | 56113.250808 | 14.990 | 0.157 | Ks |
Notes.
The full table is available at the Centre de Données astronomiques de Strasbourg (CDS). A portion is shown here for guidance purposes only.
This table contains the following information: column 1 lists the VVV ID, with an asterisk in column 2 indicating the stars that are classified by us as Mira candidates; column 3 gives the Heliocentric Julian Date of the VVV observations; columns 4 and 5 give the corresponding J-, H-, or Ks-band magnitude and associated error, respectively; and the final column indicates the bandpass. We note that measurements with Ks ≲ 12 mag can be considered saturated (Contreras Ramos et al. 2017), and should thus only be used with extreme caution.
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