Volume 532, August 2011
|Number of page(s)||43|
|Published online||14 July 2011|
Details of the analyzed observation runs.
In the following, the H-band lightcurves used are displayed (see Table A.1). In general in the upper panel of each figure the lower black datapoints mark the background measurements, the upper black curve shows the reference star S10 (if another reference star is used it is explicitly mentioned in the caption), and the green curve represents the flux density development of SgrA*. The lower panel shows the observational conditions by the FWHM of the 2-dimensional PSF (red in the direction of right ascension, purple in the direction of declination).
Observation from 13 June 2006. S2 is used as reference star for this lightcurve.
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© ESO, 2011
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