Gaia Data Release 2
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Fig. 49

image

G-band light curve example of an LPV in the LMC near the south ecliptic pole. It shows the large number of observations gathered during the first month of commissioning phase, due to the use of a specific EPSL, which is at the origin of the apparent deficiency of LPV candidates seen in Fig. 45 in the region of the LMC near the ecliptic pole (see text). The black upward- and downward-pointing triangles and magenta crosses have the same meanings as in Fig. 8.

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