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Update app.py

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  1. app.py +2 -0
app.py CHANGED
@@ -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 – 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: 120–300 nm | Wavelength: 100–300 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 – 50,000**. **Ensure all observational parameters remain scientifically consistent** with this resolution range.
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+ Example table:
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+
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  | Requirements | Necessary Values | Desired Values | Justification | Comments |
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  |---------------------|------------------------------------|--------------------------------------|----------------------------------------------------------------------------|----------------------------------------------|
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  | UV Observations | Wavelength: 120–300 nm | Wavelength: 100–300 nm | Essential for characterizing atomic/molecular emissions (H, C, O, S, etc.) | Key for detecting volatiles in exoplanetary atmospheres |