deletions | additions       diff --git a/figures/fig_Candid7_with_til/caption.tex b/figures/fig_Candid7_with_til/caption.tex  index e89597e..b20922e 100644  --- a/figures/fig_Candid7_with_til/caption.tex  +++ b/figures/fig_Candid7_with_til/caption.tex 
...
BC\_4.14-0.02 lies within $\approx$ 20 pc of the physical galactic midplane. The background is a GLIMPSE Spitzer 8 $\mu\textrm{m}$ image. The dashed line is color-coded by \citet{Dame_2011} LSR velocity and indicates the location of the physical galactic midplane. The solid colored lines indicate $\pm$ 20 pc from the galactic midplane at the 3.1 kpc distance to BC\_4.14-0.02, filament 7,  assuming the candidate is associated with the \citet{Dame_2011} Scutum-Centaurus model. The squares and circles correspond to HOPS and MALT90 sources, respectively. The label "with tilt" indicates that both the Sun's 25 pc elevation above the IAU mid-plane and the small tilt of the plane caused by the offset of the Galactic Center from the IAU (0,0) have been accounted for in this view. A closer look at BC\_4.14-0.02 filament 7  can be seen in the inset.