KROSS: Mapping the Ha emission across the star-formation sequence at z~1
  We present first results from the KMOS Redshift One Spectroscopic Survey
(KROSS), an ongoing large kinematical survey of a thousand, z~1 star forming
galaxies, with VLT KMOS. Out of the targeted galaxies (~500 so far), we detect
and spatially resolve Ha emission in ~90% and 77% of the sample respectively.
Based on the integrated Ha flux measurements and the spatially resolved maps we
derive a median star formation rate (SFR) of ~7.0 Msun/yr and a median physical
size of <r$_{\rm e}$> = 5.1kpc. We combine the inferred SFRs and effective
radii measurements to derive the star formation surface densities ({\Sigma}SFR)
and present a "resolved" version of the star formation main sequence (MS) that
appears to hold at sub-galactic scales, with similar slope and scatter as the
one inferred from galaxy integrated properties. Our data also yield a trend
between {\Sigma}SFR and {\Delta}(sSFR) (distance from the MS) suggesting that
galaxies with higher sSFR are characterised by denser star formation activity.
Similarly, we find evidence for an anti-correlation between the gas phase
metallicity (Z) and the {\Delta}(sSFR), suggesting a 0.2dex variation in the
metal content of galaxies within the MS and significantly lower metallicities
for galaxies above it. The origin of the observed trends between {\Sigma}SFR -
{\Sigma}(sSFR) and Z - {\Delta}(sSFR) could be driven by an interplay between
variations of the gas fraction or the star formation efficiency of the galaxies
along and off the MS. To address this, follow-up observations of the our sample
that will allow gas mass estimates are necessary.
