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Update app.py
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app.py
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@@ -45,7 +45,7 @@ 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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Example
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| Requirements | Necessary Values | Desired Values | Justification | Comments |
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|---------------------|------------------------------------|--------------------------------------|----------------------------------------------------------------------------|----------------------------------------------|
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@@ -53,7 +53,9 @@ Example table:
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| Infrared Observations | Wavelength: 2.5–3.0 μm | Wavelength: 2.0–3.0 μm | Tracks water/CO2 in icy bodies and planetesimals | Enables detection of the 3 μm absorption feature in icy bodies |
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| Spectroscopy | Spectral Resolution: R ≥ 10,000 | Spectral Resolution: R = 50,000 | Necessary for resolving fine spectral features of exoplanetary atmospheres | Ensures accurate molecular composition analysis |
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"""
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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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#### **Table Format Example** (Do NOT copy verbatim; generate based on the science context):
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| Requirements | Necessary Values | Desired Values | Justification | Comments |
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|---------------------|------------------------------------|--------------------------------------|----------------------------------------------------------------------------|----------------------------------------------|
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| Infrared Observations | Wavelength: 2.5–3.0 μm | Wavelength: 2.0–3.0 μm | Tracks water/CO2 in icy bodies and planetesimals | Enables detection of the 3 μm absorption feature in icy bodies |
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| Spectroscopy | Spectral Resolution: R ≥ 10,000 | Spectral Resolution: R = 50,000 | Necessary for resolving fine spectral features of exoplanetary atmospheres | Ensures accurate molecular composition analysis |
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**Use this table format as a guideline, but generate a new table dynamically based on the input.** Do not copy the example directly. Ensure that all values align with the provided constraints and exclusions.
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Ensure the response is **structured, clear, and follows this format** for consistency. **All included parameters must be scientifically consistent with each other.**
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"""
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