dennissergeev
commented
1 year ago Hi @seth-curtin1!
To be clear, both sp_sw_500ir_bd_hatp11 data used in the aeolus examples and the data in Lines et al. (2018) are from the 3D GCM we use, the Met Office Unified Model. We don't have many spectra publicly available, but you can try using for example the data from Zamyatina et al. (2023) by @mzamyatina available here, or from Christie et al. (2021) by @dachrist available here.
Hope this helps.
Is there a way that I can get data for other exoplanets in the same format as the "planet_transmission_day.nc" and "sp_sw_500ir_bd_hatp11" files? My goal is to try to find a simple way so that I can identify signatures of different molecules in planet atmospheres using the transmission spectrum. The Lines et al. (2018) paper that was mentioned on the synthetic observations page uses a graph for figure 3 in the results section and I'd like to see if I can do something similar.
Thank you for any help you may be able to provide!