Question Answering
Transformers
Safetensors
English
mistral
text-generation
text-generation-inference
8-bit precision
gptq
Instructions to use Tijmen2/cosmosage_v1_gptq with libraries, inference providers, notebooks, and local apps. Follow these links to get started.
- Libraries
- Transformers
How to use Tijmen2/cosmosage_v1_gptq with Transformers:
# Use a pipeline as a high-level helper from transformers import pipeline pipe = pipeline("question-answering", model="Tijmen2/cosmosage_v1_gptq")# Load model directly from transformers import AutoTokenizer, AutoModelForCausalLM tokenizer = AutoTokenizer.from_pretrained("Tijmen2/cosmosage_v1_gptq") model = AutoModelForCausalLM.from_pretrained("Tijmen2/cosmosage_v1_gptq") - Notebooks
- Google Colab
- Kaggle
Update README.md
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README.md
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@@ -116,6 +116,27 @@ ratio in the presence of foregrounds for the LiteBIRD mission. The authors find
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can significantly affect the estimation of the tensor-to-scalar ratio, and that the knowledge of the beam far
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side-lobes is crucial for accurate results. The study also discusses the importance of accurately modeling the
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beam profile and the challenges in estimating the tensor-to-scalar ratio in the presence of foregrounds.
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```
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## Qualitative evaluation
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can significantly affect the estimation of the tensor-to-scalar ratio, and that the knowledge of the beam far
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side-lobes is crucial for accurate results. The study also discusses the importance of accurately modeling the
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beam profile and the challenges in estimating the tensor-to-scalar ratio in the presence of foregrounds.
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USER: Explain a detailed design for a future CMB satellite. What detector technology would you choose? What
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optics? Photometer vs spectrometer? etc.
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ASSISTANT: A detailed design for a future CMB satellite would involve several key components. Firstly, the
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choice of detector technology is crucial. One option could be using Transition Edge Sensor (TES) bolometers
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coupled to superconducting detectors, similar to those used in the Planck mission. These detectors are highly
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sensitive and can measure temperature fluctuations in the CMB with high precision. Another option could be
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using Kinetic Inductance Detectors (KIDs), which offer fast response time and are less susceptible to
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systematic effects.
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Next, the optics design should aim to minimize stray light and ensure high optical efficiency. This can be
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achieved by using a combination of reflective and refractive optics, along with a series of baffles and
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filters to block unwanted stray light.
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The choice between a photometer and a spectrometer depends on the science goals of the mission. A photometer
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would provide broadband measurements of the CMB temperature and polarization anisotropies, while a spectrometer
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would allow for more detailed studies of the spectral properties of the CMB.
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Finally, the spacecraft design should consider factors such as thermal control, power generation, attitude
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determination and control, communication, and data handling systems. It should also include redundant systems
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to ensure reliability and fault tolerance during the long duration of the mission.
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```
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## Qualitative evaluation
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