--- library_name: keras-hub pipeline_tag: text-generation --- Hey I am CosmoGemma 👋 I can answer cosmology questions from astroph.CO research articles. This is a Gemma_2b_en fine-tuned on QA pairs (3.5k) generated from Cosmology and Nongalactic Astrophysics articles (arXiv astro-ph.CO) from 2018-2022 and tested on QA pairs (1k) generated from 2023 articles, scoring over 75% accuracy. All codes/data used to develop CosmoGemma can be found at the following GitHub repository: https://github.com/sultan-hassan/CosmoGemma Example to run CosmoGemma locally: Requirement: ``` keras==3.6.0 keras_nlp==0.15.1 python==3.10 ``` If not available, install them using: ``` pip install -q -U keras-nlp pip install -q -U "keras>=3" ``` Script: ``` import os os.environ["KERAS_BACKEND"] = "jax" # Or "torch" or "tensorflow". # Avoid memory fragmentation on JAX backend. os.environ["XLA_PYTHON_CLIENT_MEM_FRACTION"]="1.00" import keras import keras_nlp gemma_lm = keras_nlp.models.CausalLM.from_preset("hf://sultan-hassan/CosmoGemma_2b_en") template = "Instruction:\n{instruction}\n\nResponse:\n{response}" Question = "write your question here" prompt = template.format( instruction=Question, response="", ) out = gemma_lm.generate(prompt, max_length=1024) ind = out.index('\n\nResponse:\n') + len('\n\nResponse:\n') print ("Question:", Question) print ("Answer:", out[ind:]) ``` Training dataset Dataset has been generated from the llama3.1:8b-instruct-fp16 model to generate QA pairs from abstracts of the Cosmology and Nongalactic Astrophysics articles (arXiv astro-ph.CO) from 2018-2022. Examples for some questions from the training dataset: ``` Question: What are some common methods for model selection in astrophysics? Answer: The goodness of fit, the likelihood ratio test, Bayesian model selection using Bayes factors, and the classical as well as the Bayesian information theoretic approaches. Question: What type of coupling in inflationary models can affect the prediction of inflationary parameters? Answer: Non-minimal coupling to gravity. Question: What type of distribution is used to model the probability of non-linear density field? Answer: A superposition of a Gaussian and a lognormal distribution. Question: Can the shape of central cluster galaxies be used as a predictor of weak-lensing mass bias in individual clusters? Answer: Yes, we find that on average, the lensing masses of clusters with the roundest / most elliptical 25% of BCGs are biased ~20% high / low compared to the average. Question: What could be the cause of remaining excess power in a signal after foreground mitigation? Answer: Residual foreground emission from sources or diffuse emission far away from the phase centre, polarization leakage, chromatic calibration errors, ionosphere, or low-level radio-frequency interference Question: What is the precision of photometric redshift estimates for LRGs? Answer: 0.02 Question: What is the form of the scaling relation used to calculate X-ray luminosity? Answer: $L_{\rm{X}} \propto \text{A}_{\rm{X}}M_{\text{200c}}^{\text{B}_{\rm{X}}} E(z)^2 (1+z)^{\gamma_{\rm{X}}}$ ``` This is a [`Gemma` model](https://keras.io/api/keras_nlp/models/gemma) uploaded using the KerasNLP library and can be used with JAX, TensorFlow, and PyTorch backends. This model is related to a `CausalLM` task. Model config: * **name:** gemma_backbone * **trainable:** True * **vocabulary_size:** 256000 * **num_layers:** 18 * **num_query_heads:** 8 * **num_key_value_heads:** 1 * **hidden_dim:** 2048 * **intermediate_dim:** 32768 * **head_dim:** 256 * **layer_norm_epsilon:** 1e-06 * **dropout:** 0 * **query_head_dim_normalize:** True * **use_post_ffw_norm:** False * **use_post_attention_norm:** False * **final_logit_soft_cap:** None * **attention_logit_soft_cap:** None * **sliding_window_size:** 4096 * **use_sliding_window_attention:** False This model card has been generated automatically and should be completed by the model author. See [Model Cards documentation](https://huggingface.co/docs/hub/model-cards) for more information.