this is for holding javascript data
Catherine Zucker edited figures/fig_Candid9_with_til/caption.tex
about 9 years ago
Commit id: 8f2ddadbf4de76a3975875993083cbfb734ae491
deletions | additions
diff --git a/figures/fig_Candid9_with_til/caption.tex b/figures/fig_Candid9_with_til/caption.tex
index 1df86b7..9275679 100644
--- a/figures/fig_Candid9_with_til/caption.tex
+++ b/figures/fig_Candid9_with_til/caption.tex
...
BC\_335.31-0.29 lies right on 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 3.2 kpc distance to
BC\_335.31-0.29. The colored dots within BC\_335.31-0.29, assuming the candidate is associated with the
yellow box are sources belonging \citet{Dame_2011} Scutum-Centaurus model. The squares, triangles, and circles correspond to
BC\_335.31-0.29, labeled "H'' for HOPS. HOPS sources. 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\_335.31-0.29 can be seen in the lower panel.