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Update app.py
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app.py
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@@ -45,6 +45,8 @@ Generate a **detailed and structured** response based on the given **science con
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- **Exclusion of Existing Facilities:** **Do not reference** existing observatories such as JWST, Hubble, or ground-based telescopes. This work pertains to a **new mission**.
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- **Spectral Resolution Constraint:** Limit spectral resolution (**R**) to the range **10,000 β 50,000**. **Ensure all observational parameters remain scientifically consistent** with this resolution range.
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| Requirements | Necessary Values | Desired Values | Justification | Comments |
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|---------------------|------------------------------------|--------------------------------------|----------------------------------------------------------------------------|----------------------------------------------|
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| UV Observations | Wavelength: 120β300 nm | Wavelength: 100β300 nm | Essential for characterizing atomic/molecular emissions (H, C, O, S, etc.) | Key for detecting volatiles in exoplanetary atmospheres |
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- **Exclusion of Existing Facilities:** **Do not reference** existing observatories such as JWST, Hubble, or ground-based telescopes. This work pertains to a **new mission**.
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- **Spectral Resolution Constraint:** Limit spectral resolution (**R**) to the range **10,000 β 50,000**. **Ensure all observational parameters remain scientifically consistent** with this resolution range.
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Example table:
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| Requirements | Necessary Values | Desired Values | Justification | Comments |
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|---------------------|------------------------------------|--------------------------------------|----------------------------------------------------------------------------|----------------------------------------------|
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| UV Observations | Wavelength: 120β300 nm | Wavelength: 100β300 nm | Essential for characterizing atomic/molecular emissions (H, C, O, S, etc.) | Key for detecting volatiles in exoplanetary atmospheres |
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