1. Image stamps of an example fit for a bulge+disc object with B/T = 0
Image stamps of an example fit for a bulge+disc object with B/T = 0.5, again following the placement of stamps described in the caption of Fig. A8.
Image stamps of an example fit for a bulge+disc object with B/T = 0.5, again following the placement of stamps described in the caption of Fig. A8. This object has a more equal contribution from the bulge and disc components. As with the previous examples, examination of the residual stamps for all four bands illustrates the good quality of the fits achieved by the adopted modelling technique, with no evidence of any additional structure in the bluer bands which has failed to be reproduced by the best-fitting models.
V. A. Bruce et al. MNRAS 2014;444:
© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society