Abstract
The existence of mass substructure is an inevitable consequence of the
LCDM paradigm. Depite this clear theoretical prediction, a glaring
discrepancy with the number of luminous satellites around the Milky Way
{MW} has been identified, i.e. the "missing satellite problem".
Notwithstanding great progress to address this problem, it remains
unsolved. Moreover, the MW could be a biased environment, not
representative of the typical universe. Surface brightness aberrations
of gravitationally lensed images provide a complementary channel to
detect substructure beyond the local Universe in mostly massive
early-type galaxies. Simulations suggest a substructure mass fraction of
f_sub99% CL. We
request 30 orbits with HST WFC3-F390W to accomplish this goal.
Original language | English |
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Pages (from-to) | 12898 |
Journal | HST Proposal ID #12898. Cycle 20 |
Publication status | Published - Oct-2012 |