Due to the lack
of sensitivity
of past and
current infrared (IR) instrumentation, so far it has not been possible to get a glimpse into the earl... ▽ More Our
current knowledge
of star formation and accretion
luminosity at high - redshift (z > 3 - 4), as well as the possible connections between them, relies mostly on observations in the rest - frame ultraviolet (UV), which are strongly affected by dust obscuration.
Abstract: Our
current knowledge
of star formation and accretion
luminosity at high - redshift (z > 3 - 4), as well as the possible connections between them, relies mostly on observations in the rest - frame ultraviolet (UV), which are strongly affected by dust obscuration.