this is for holding javascript data
Melanie Galloway edited section_Science_1_Clumps_citep__.tex
about 8 years ago
Commit id: 33e071952e9e81d1c2605412fbbf8702e0b7834a
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-Clump size; perhaps there are size constraints limiting how clumps can be arranged?
-redshift - how do distributions evolve spatially over time?
[paragraph about what has been done @ high redshift, how can we do similar/more with GZH]
Although clumpy galaxies are most abundant at high redshift, there is a significant population that exist locally (z < 0.2). Analysis of this population is ideal for revealing the finer substructure of the clumps, which have typical sizes of 100pc ~ 1kpc. HST/ACS imaging is capable of resolving [some size] at z=0.2, while SDSS can only resolve features of [this size] at the same redshift.