deletions | additions       diff --git a/figures/fig_Candid10_with_ti/caption.tex b/figures/fig_Candid10_with_ti/caption.tex  index 9e8a305..2d8104d 100644  --- a/figures/fig_Candid10_with_ti/caption.tex  +++ b/figures/fig_Candid10_with_ti/caption.tex 
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BC\_332.21-0.04 Filament 10  lies within $\approx$ 15 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 3.3 kpc distance to BC\_332.21-0.04, filament 10,  assuming the candidate is associated with the \citet{Dame_2011} Scutum-Centaurus model. The squares and diamonds 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\_332.21-0.04 filament 10  can be seen in the inset.