The UV continua and inferred stellar populations of galaxies at z ≃ 7-9 revealed by the Hubble Ultra-Deep Field 2012 campaign

We use the new ultra-deep, near-infrared imaging of the Hubble Ultra-Deep Field (HUDF) provided by our UDF12 Hubble Space Telescope (HST) Wide Field Camera 3/IR campaign to explore the rest-frame ultraviolet (UV) properties of galaxies at redshifts z > 6.5. We present the first unbiased measurement of the average UV power-law index, <beta >, (f(lambda) alpha lambda(beta)) for faint galaxies at z similar or equal to 7, the first meaningful measurements of <beta > at z similar or equal to 8, and tentative estimates for a new sample of galaxies at z similar or equal to 9. Utilizing galaxy selection in the new F140W (J(140)) imaging to minimize colour bias, and applying both colour and power-law estimators of beta, we find <beta > = -2.1 +/- 0.2 at z similar or equal to 7 for galaxies with M-UV similar or equal to -18. This means that the faintest galaxies uncovered at this epoch have, on average, UV colours no more extreme than those displayed by the bluest star-forming galaxies at low redshift. At z similar or equal to 8 we find a similar value, <beta > = -1.9 +/- 0.3. At z similar or equal to 9, we find <beta > = -1.8 +/- 0.6, essentially unchanged from z similar or equal to 6 to 7 (albeit highly uncertain). Finally, we show that there is as yet no evidence for a significant intrinsic scatter in beta within our new, robust z similar or equal to 7 galaxy sample. Our results are most easily explained by a population of steadily star-forming galaxies with either similar or equal to solar metallicity and zero dust, or moderately sub-solar (similar or equal to 10-20 per cent) metallicity with modest dust obscuration (A(V) similar or equal to 0.1-0.2). This latter interpretation is consistent with the predictions of a state-of-the-art galaxy-formation simulation, which also suggests that a significant population of very-low metallicity, dust-free galaxies with beta similar or equal to -2.5 may not emerge until M-UV > -16, a regime likely to remain inaccessible until the James Webb Space Telescope.