fix hcn reference

arjunsavel · Jan 24, 2024 · d438720 · d438720
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diff --git a/paper/paper.bib b/paper/paper.bib
@@ -269,7 +269,7 @@ @article{karman:2019
   doi={10.1016/j.icarus.2019.02.034},
   publisher={Elsevier}
 }
-@article{barber2014exomol,
+@article{barber:2014,
   title={ExoMol line lists--III. An improved hot rotation-vibration line list for HCN and HNC},
   author={Barber, RJ and Strange, JK and Hill, C and Polyansky, OL and Mellau, G Ch and Yurchenko, SN and Tennyson, Jonathan},
   journal={Monthly Notices of the Royal Astronomical Society},

diff --git a/paper/paper.md b/paper/paper.md
@@ -131,7 +131,7 @@ thermal emission spectrum of the
 fiducial hot Jupiter WASP-77Ab [@line:2021; @mansfield:2022; @august:2023] as observed at IGRINS.
 The retrieval pairs `PyMultiNest` [@buchner:2014] sampling with the `CHIMERA` radiative transfer code [@line:2013],
 with opacity from $\rm H_2O$ [@polyansky:2018], $\rm CO$ [@rothman:2010], $\rm CH_4$ [@hargreaves:2020],
-$\rm NH_3$ [@coles:2019], $\rm HCN$ [@yurchenko:2011], $\rm H_2S$ [@azzam:2016], and $\rm H_2-H_2$
+$\rm NH_3$ [@coles:2019], $\rm HCN$ [@barber:2014], $\rm H_2S$ [@azzam:2016], and $\rm H_2-H_2$
 collosion-induced absorption [@karman:2019].
 The non-compressed retrieval uses the data and retrieval framework from [@line:2021], run in an upcoming article (Savel et al. 2024, submitted).
 For this experiment, we use the PCA-based compression scheme implemented in `cortecs`, preserving 3 principal components