Tutorials¶
ESO ATMO 2021¶
- Tutorial
- What happens to a transit (transmission+emission) spectrum as a function of temperature
- What molecules are most important to planetary spectroscopy?
- Where in temperature space do chemical transitions seem to take place?
- Is this molecule affecting my spectrum?
- Understanding Models in the Context of Observing Modes
- Adding Clouds to the Story using
Virga
Early Release Workshop 2021¶
Sagan School 2021: Spectroscopy of Young Planets¶
Sagan School 2020: Writing a JWST Proposal¶
- Initial Setup
- What accuracy in planet properties do I need?
- What tools do I need? How do I use them?
- Use
PandExo
to run initial constant \((R_p/R_*)^2\) to determine approx precision - Use
PICASO
to determine first guess atmospheric transmission signal - Check
Exo.MAST
for available data so we can validate our assumptions - Use
PICASO
to determine first guess atmospheric emission signal - Can an atmosphere be detected: Addressing cloud concerns and quantifying statistical significance in transmission
- Can an atmosphere be detected: Addressing unknown climate and quantifying statistical significance in emission
- Can a specific molecule be detected?
- Can any physical parameters be constrained? Information content theory for initial constraint estimates
- Use