text:   from color-magnitude diagrams",5,"['New paper on dwarf galaxies! (and a first for me) in collaboration with Michele Mastropietro (@mic_mas), Sven De Rijcke, Carmen Gallart, Edouard Bernard and Robbert Verbeke (@Rbhfd): ""Observations"" of simulated dwarf galaxies (<LINK>).', 'In this paper, we observationally analyze a set of realistically simulated MoRIA dwarf galaxies (from the work of @Rbhfd), to look for any systematic bias in comparison of simulations with observations.', 'In particular, we use the synthetic color-magnidue diagram (CMD) technique to reconstruct the star formation history (SFH) of dwarf galaixes. We construct CMDs of simulated dwarfs from simulation star particle data and add observational errors to mimic real observations.', 'On comparing the reconstructed SFH from the synthetic CMD method with the ground truth from the simulation star particle data, we overall find a good agreement.', 'Our paper also explores:\n1) the effect of dust extinction on the CMD, and hence on the reconstructed SFH, and\n2) the dependence on the SFH on the aperture used.\n\nWe also analyze infrared CMDs, in view of the next generation astronomical facilities.']",20,07,1119