{"total":10,"items":[{"citing_arxiv_id":"2606.30224","ref_index":82,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era","primary_cat":"astro-ph.CO","submitted_at":"2026-06-29T12:38:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Reviews how cross-correlating SKAO 21-cm LIM with other lines like [CII], CO, and Ly-alpha can mitigate systematics, enhance sensitivity, and disentangle cosmological from astrophysical parameters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30200","ref_index":70,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cosmology with Intensity Mapping via Statistics Beyond the Power Spectrum in the SKAO Era","primary_cat":"astro-ph.CO","submitted_at":"2026-06-29T12:16:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Reviews multiple higher-order statistics for 21-cm intensity mapping and forecasts their detectability with SKAO, incorporating noise and foreground effects.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.29903","ref_index":131,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"High-Redshift Signatures from the Cosmic Dawn and the Epoch of Reionization","primary_cat":"astro-ph.CO","submitted_at":"2026-06-29T07:38:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A review chapter summarizing theoretical 21-cm signatures from Cosmic Dawn and Reionization and their detectability with SKA-Low.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27858","ref_index":143,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Inferring Cosmology and Astrophysics from the High-redshift 21cm Signal with SKA-Low","primary_cat":"astro-ph.CO","submitted_at":"2026-06-26T08:56:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":1.0,"formal_verification":"none","one_line_summary":"A review chapter on tools for inferring galaxy and IGM properties from the 21 cm signal using the initial SKA-Low array configuration.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26435","ref_index":129,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Overview of 21cm Experiments at high redshift with SKAO","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T22:54:35+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":0.0,"formal_verification":"none","one_line_summary":"An overview summarizing SKA-Low 21cm experiments for power spectrum, tomography, 21-cm forest, and cross-correlations, plus critical telescope features, building on the 2015 SKA Science Book.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.24724","ref_index":119,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Imaging the 21-cm Signal from the Cosmic Dawn & Epoch of Reionization and the Connection with the Global Signal","primary_cat":"astro-ph.CO","submitted_at":"2026-06-23T15:49:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"This review summarizes SKA-Low's tomographic imaging potential for the 21-cm signal and its connection to the global 21-cm signal.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23791","ref_index":191,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"One Generator, Any Process: LLM-Conditioning for the LHC","primary_cat":"hep-ph","submitted_at":"2026-06-22T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"LLM embeddings condition a generative transformer to enable faster convergence, better performance, and generalization to unseen LHC processes using a single model.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.00219","ref_index":256,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables","primary_cat":"astro-ph.CO","submitted_at":"2026-05-29T18:00:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"21cmEMUv3 emulates the cylindrical 21cm power spectrum via score-based diffusion and six other 21cmFAST observables via LSTM networks at sub-percent accuracy, then uses the emulator to infer a lower limit on soft-band X-ray luminosity from HERA data.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.29016","ref_index":32,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Three-dimensional Conditional Diffusion Models for Cosmological 21 cm Lightcone Emulation","primary_cat":"astro-ph.IM","submitted_at":"2026-05-27T19:16:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Yeo-Johnson preprocessing combined with moderate amplitude compression provides the best trade-off for conditional diffusion models emulating 3D 21 cm lightcones, supported by MAE_std on the global signal, though biases remain in power spectra and higher-order statistics.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.10105","ref_index":100,"ref_count":4,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Application of Machine Learning to 21 cm Cosmology","primary_cat":"astro-ph.CO","submitted_at":"2026-05-11T07:19:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Review chapter organizing machine learning methods for 21 cm cosmology into observation, theory, and inference domains.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}