From d43872003bdc2384af63498bd93140202b8a40d4 Mon Sep 17 00:00:00 2001 From: arjunsavel Date: Wed, 24 Jan 2024 10:08:26 -0500 Subject: [PATCH] fix hcn reference --- paper/paper.bib | 2 +- paper/paper.md | 2 +- 2 files changed, 2 insertions(+), 2 deletions(-) diff --git a/paper/paper.bib b/paper/paper.bib index 7fff0a8..7bde32d 100644 --- 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 index a027858..a003e2c 100644 --- 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