Very Blue UV-Continuum Slopes of Star-Forming Galaxies at z~7 and the Evolution to z~2-4

Computer Science – Databases

Scientific paper

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Star Formation, Clusters Of Galaxies, Sky Surveys, Brightness, Redshift, Star Formation, Galaxy Clusters, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Magnitudes And Colors, Luminosities, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies

Scientific paper

The new WFC3/IR instrument on HST enables us to survey the sky in the near-IR 40× more efficiently than ever before, permitting enormous strides in the identification and characterization of galaxies at z>=7. Already, deep wide-area observations exist over some ~52 arcmin2 in the HUDF09+ERS fields. With these data, we have been able to identify more than 60 z~7 galaxy candidates, more than 40 z~8 galaxy candidates, and even some possible z~9 galaxies over a 3 magnitude range in luminosity, adding significantly to the 20-30 z~7 candidates known prior to WFC3/IR. One of the most interesting observables to examine in these high redshift galaxies are the UV-continuum slopes, since it provides us with constraints on the dust content, metallicities, ages, and possibly escape fractions of low-mass star-forming galaxies at very early times. Here, I provide a brief summary of our findings on the UV-continuum slopes β of z~7 galaxies from the early ultra-deep WFC3/IR data over the HUDF.

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