Fig. 2

Comparative photometry of 2012 DR30 over four nights. The error bars are given relative to the internally consistent photometry (left ordinate), and is dominated by the photon noise, found via SExtractor’s FLUXERR_APER (RMS error vector for aperture flux) values. The absolute magnitude (right ordinate) is tied to the APASS catalogue, which had up to an 0.2 mr variation in the shift required for the standard stars, so it is provided for guidance rather than high precision.
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