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Update app.py
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app.py
CHANGED
@@ -48,14 +48,14 @@ Generate a **detailed and structured** response based on the given **science con
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- Instrument: Should only be Imager, Spectrograph, Polarimeter and Coronagraph).
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- Necessary Values: The necessary values or parameters (wavelength range, spectral resolution where applicable, spatial resolution where applicable, contrast ratio where applicable).
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- Desired Values: The desired values or parameters (wavelength range, spectral resolution where applicable, spatial resolution where applicable).
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- Justification: Detailed scientific explanation of why these observations are important for the science objectives.
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- Comments: Additional notes or remarks regarding each observation.
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#### **Table Format**
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| Wavelength Band | Instrument | Necessary Values | Desired Values | Justification
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#### **Guiding Constraints (Exclusions & Prioritization)**
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- **Wavelength Band Restriction:** Only include **UV, Visible, and Infrared** bands.
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@@ -65,6 +65,7 @@ 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**.
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- **Contrast Ratio:** Limit contrast ratio to the range **10^4 - 10^6**.
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- **Ensure that all parameters remain scientifically consistent.**
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**Use this table format as a guideline, generate a detailed table dynamically based on the input.**. Ensure that all values align with the provided constraints and instructions.
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- Instrument: Should only be Imager, Spectrograph, Polarimeter and Coronagraph).
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- Necessary Values: The necessary values or parameters (wavelength range, spectral resolution where applicable, spatial resolution where applicable, contrast ratio where applicable).
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- Desired Values: The desired values or parameters (wavelength range, spectral resolution where applicable, spatial resolution where applicable).
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- Number of Objects Observed: Estimate the number of objects that need to be observed for a statistically meaningful result or for fulfilling the science objective.
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- Justification: Detailed scientific explanation of why these observations are important for the science objectives.
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- Comments: Additional notes or remarks regarding each observation.
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#### **Table Format**
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| Wavelength Band | Instrument | Necessary Values | Desired Values | Number of Objects Observed | Justification | Comments |
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|----------------------|------------------------------------|------------------------------------|---------------------------------|---------------------------------|-------------------|----------|
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#### **Guiding Constraints (Exclusions & Prioritization)**
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- **Wavelength Band Restriction:** Only include **UV, Visible, and Infrared** bands.
|
|
|
65 |
- **Exclusion of Existing Facilities:** **Do not reference** existing observatories such as JWST, Hubble, or ground-based telescopes. This work pertains to a **new mission**.
|
66 |
- **Spectral Resolution Constraint:** Limit spectral resolution (**R**) to the range **10,000 – 50,000**.
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- **Contrast Ratio:** Limit contrast ratio to the range **10^4 - 10^6**.
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- **Estimate the "Number of Objects Observed" based on the observational strategy, parameters, instruments, statistical requirements, and feasibility.**
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- **Ensure that all parameters remain scientifically consistent.**
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**Use this table format as a guideline, generate a detailed table dynamically based on the input.**. Ensure that all values align with the provided constraints and instructions.
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