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Figure 1:
Astrometric/photometric errors and their standard deviations. Crosses are for Night1, stars for Night2, diamonds for Night3, triangles for Night4, and squares for Night5. Errors are estimated for each magnitude bin of the luminosity function computed by StarFinder. The translation to get the absolute photometry can be done with the zero-point of each night (![]() |
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Figure 2:
Upper line: Sgr A*/![]() ![]() ![]() ![]() ![]() ![]() ![]() |
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Figure 3:
Left: distance of Sgr A*/![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() |
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Figure 4:
Encircled H II components positions on a 2.4
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