Transiting exoplanets


The observation modes available to observations of exoplanet is describe in the BOTS page.


For a description of the NIRSpec Exoplanet Exposure Time Calculator visit

The limiting magnitutude limits are presented here:

Signal to noise ratios has been computed as a funtion of magnitude of the host star:

And finaly, case studies conducted based on atmospheric models based on well known exoplanets: