deletions | additions       diff --git a/figures/Candid3_pos_pos/caption.tex b/figures/Candid3_pos_pos/caption.tex  index 73f5ada..f919952 100644  --- a/figures/Candid3_pos_pos/caption.tex  +++ b/figures/Candid3_pos_pos/caption.tex 
...
Plane of the sky map integrated between 55-75 km/s, the approximate velocity range of the Scutum-Centaurus arm in the region around filament 2. The black dashed line indicates the location of the physical Galactic midplane, while the solid black lines indicate $\pm$ 20 pc from the galactic midplane at the 4.4 kpc distance to filament 2, assuming the candidate is associated with the \citet{Dame_2011} Scutum-Centaurus model. A trace of filament 2, as it would appear as a mid-IR extinction feature, is superimposed on the CO emission map. The correlation between BC\_25.24-0.45's filament 2's  mid-IR extinction feature and the Scutum-Centaurus's arm most intense CO emission hints that it may be a spine of Scutum-Centaurus as traced by lower density CO gas diff --git a/figures/Candid4_pos_pos/caption.tex b/figures/Candid4_pos_pos/caption.tex  index d638b50..c15a697 100644  --- a/figures/Candid4_pos_pos/caption.tex  +++ b/figures/Candid4_pos_pos/caption.tex 
...
Plane of the sky map integrated between 55-75 km/s, the approximate velocity range of the Scutum-Centaurus arm in the region around BC\_21.25-0.15. The black dashed line indicates the location of the physical galactic midplane, while the solid black lines indicate $\pm$ 20 pc from the galactic midplane at the 3.9 kpc distance to BC\_21.25-0.15, filament 4,  assuming the candidate is associated with the \citet{Dame_2011} Scutum-Centaurus model. A trace of BC\_21.25-0.15, filament 4,  as it would appear as a mid-IR extinction feature, is superimposed on the CO emission map. diff --git a/figures/Candid7_pos_pos/caption.tex b/figures/Candid7_pos_pos/caption.tex  index f5bb98d..c422b8b 100644  --- a/figures/Candid7_pos_pos/caption.tex  +++ b/figures/Candid7_pos_pos/caption.tex 
...
Plane of the sky map integrated between 0-20 km/s, the approximate velocity range of the Scutum-Centaurus arm in the region around BC_4.14-0.02. filament 7.  The black dashed line indicates the location of the physical galactic midplane, while the solid black 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. A trace of BC\_4.14-0.02, filament 7,  as it would appear as a mid-IR extinction feature, is superimposed on the CO emission map.