Abstract
We report the discovery of significant mass/light offsets in the strong
gravitational lensing system SDSS\,J1011$+$0143. We use the high-resolution
Hubble Space Telescope (HST) F555W- and F814W-band imaging
and SDSS spectroscopy of this system, which consists of a close galaxy pair
with a projected separation of $4.2$ kpc at $z_lens 0.331$
lensing a Lyman-alpha emitter (LAE) at $z_source = 2.701$. Comparisons
between the mass peaks inferred from lens models and light peaks from
HST imaging data reveal significant spatial mass/light offsets as
large as $(1.72 0.24 0.34)$ kpc in both filter bands. Such large
mass/light offsets, not seen in isolated field lens galaxies and relaxed galaxy
groups, may be related to the interactions between the two lens galaxies. The
detected mass/light offsets can potentially serve as an important test for the
self-interacting dark matter model. However, other mechanisms such as dynamical
friction on spatially differently distributed dark matter and stars could
produce similar offsets. Detailed hydrodynamical simulations of galaxy-galaxy
interactions with self-interacting dark matter could accurately quantify the
effects of different mechanisms. The background LAE is found to contain three
distinct star-forming knots with characteristic sizes from 116 pc to 438 pc. It
highlights the power of strong gravitational lensing in probing the otherwise
too faint and unresolved structures of distance objects below sub-kiloparsec or
even 100-parsec scales through its magnification effect.
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