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Galaxy And Mass Assembly (GAMA) : detection of low surface brightness galaxies from SDSS data

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Figure

Figure 2. Histograms of thepanel), with a median of 0.233, and of the g − r colour of GAMA dwarf galaxies (top r − i colour of the same galaxies(bottom panel), with a median of 0.154
Table 1. The filter, apparent magnitudes (m) for a fiducial source,the range of signals (S) calculated for different images, sky-noisevalues (σ sky), and weights (ω) to be applied to the images beforeco-adding.
Figure 5. 12 confirmed LSBGs from the co-added, masked, and smoothed images created from SDSS g, r, and i bands
Figure 6. Sky positions of the 343 LSBGs across all fields, G09, G12, andG15 (top, middle, bottom, respectively; red circles)
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