Fig. 1
Sky images constructed in different photometric passbands for the cluster ID27. Multiband images in the WFC3+ACS passbands are made from the PHAT mosaics downloaded at the MAST (Mikulski Archives for Space Telescopes)1. Panels show combinations of passbands: a) PHAT clusters (blue dots) plotted on the Spitzer 24 μm map – the cluster under consideration is marked with a red dot; b) GALEX FUV (blue) + NUV (red) (76′′×76′′); c)F275W + F336W + F475W (13′′×13′′); d)F336W + F475W + F814W (13′′×13′′); e) the 24 μm passband centred on the cluster (76′′×76′′); f) F336W + F814W + F110W (5′′×5′′); g)F275W + F814W + F160W (13′′×13′′); h) F814W + F110W + F160W (13′′×13′′). In panels c), d), f), g), and h) the green circle shows aperture of 2″ radius, while the red circle marks the aperture used by the PHAT team for photometry.
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