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6 changes: 4 additions & 2 deletions notebooks/simulator/lens_x2.ipynb
Original file line number Diff line number Diff line change
Expand Up @@ -12,8 +12,10 @@
"\n",
"Strong lenses with this complex mass distribution are more challenging to model than those with a single lens galaxy.\n",
"\n",
"This system is on the verge of being a group scale lens, but is included in this section of the workspace as it is\n",
"only two lens galaxies. The `modeling` examples in the `group` package are also applicable to this lens.\n",
"A system with two co-dominant lens galaxies and no shared dark-matter halo is exactly what the\n",
"`autolens_workspace`'s `multi_galaxy` package is dedicated to \u2014 its `start_here` and `modeling` examples are\n",
"directly applicable to this lens. (Systems where a dominant group-scale halo joins the galaxies belong one rung\n",
"up the regime ladder, in the `group` package.)\n",
"\n",
"This dataset is modeled in HowToLens chapter 3 and is used to illustrate the advanced **PyAutoLens** feature search\n",
"chaining.\n",
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6 changes: 4 additions & 2 deletions scripts/simulator/lens_x2.py
Original file line number Diff line number Diff line change
Expand Up @@ -7,8 +7,10 @@

Strong lenses with this complex mass distribution are more challenging to model than those with a single lens galaxy.

This system is on the verge of being a group scale lens, but is included in this section of the workspace as it is
only two lens galaxies. The `modeling` examples in the `group` package are also applicable to this lens.
A system with two co-dominant lens galaxies and no shared dark-matter halo is exactly what the
`autolens_workspace`'s `multi_galaxy` package is dedicated to — its `start_here` and `modeling` examples are
directly applicable to this lens. (Systems where a dominant group-scale halo joins the galaxies belong one rung
up the regime ladder, in the `group` package.)

This dataset is modeled in HowToLens chapter 3 and is used to illustrate the advanced **PyAutoLens** feature search
chaining.
Expand Down
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