{"total":21,"items":[{"citing_arxiv_id":"2605.23083","ref_index":33,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A Strongly Parametrized Mass Ratio Model for the Stable Mass Transfer Channel: a Case Study of the $10 \\, \\rm{M}_{\\odot}$ Peak","primary_cat":"astro-ph.HE","submitted_at":"2026-05-21T22:30:15+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A parametrized analytical model for BBH mass ratios from the stable mass transfer channel is derived and applied to the 10 solar-mass peak in GWTC-4, favoring little mass-ratio reversal.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23048","ref_index":55,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"StanBKT: Rethinking Parameter Estimation in Bayesian Knowledge Tracing","primary_cat":"cs.HC","submitted_at":"2026-05-21T21:27:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"StanBKT provides a unified Bayesian inference framework for BKT models supporting HMC, variational inference, and hierarchical variants, evaluated on ASSISTments and intervention datasets.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.20112","ref_index":48,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Gravitational-wave constraints on $H_0$ are robust to (putative) redshift evolution in the binary black hole mass spectrum at current sensitivity","primary_cat":"astro-ph.CO","submitted_at":"2026-05-19T16:59:39+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Spectral-siren H0 constraints from GWTC-4.0 binary black holes remain robust when the mass spectrum is permitted to evolve with redshift at current detector sensitivity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.08544","ref_index":24,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Bayesian Doppler Imaging: Simultaneous Inference of Surface Maps and Geometric Parameters","primary_cat":"astro-ph.EP","submitted_at":"2026-05-08T23:10:07+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A fully Bayesian pixel-based Doppler imaging framework uses Gaussian Process priors and Hamiltonian Monte Carlo to simultaneously infer surface maps and geometric parameters from spectral data.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"spectra without external constraints. In contrast to clas- sical Doppler imaging, neitherv rot sininor the inclina- tion needs to be fixed a priori. 2.2.3.Conditional posterior of the surface map Here,W, Σ d, Σa, andµ a are evaluated at a posterior drawθ (s). With the Gaussian prior a|θ∼ N(µ a,Σ a),(23) and the Gaussian likelihood d|a,θ∼ N(Wa,Σ d),(24) the conditional distributionp(a|d,θ) is again Gaussian (see Appendix C), expressed as p(a|d,θ) =N(µ a|d,Σ a|d),(25) where Σa|d = Σ−1 a +W TΣ−1 d W \u0001−1 ,(26) µa|d = Σa|d W TΣ−1 d d+ Σ −1 a µa \u0001 .(27) The expression for Σa|d in Eq. (26) involves the inver- sion of thep×pmatrix Σ −1 a +W TΣ−1 d W. Whether this inversion is computationally demanding depends on the"},{"citing_arxiv_id":"2605.05493","ref_index":276,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A renormalization-group inspired lattice-based framework for piecewise generalized linear models","primary_cat":"stat.ME","submitted_at":"2026-05-06T22:27:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"RG-inspired lattice models for piecewise GLMs provide explicit interpretable partitions and a replica-analysis-derived scaling law for regularization that allows increasing complexity without expected rise in generalization loss.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.20723","ref_index":17,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Tokenised Flow Matching for Hierarchical Simulation Based Inference","primary_cat":"cs.LG","submitted_at":"2026-04-22T16:07:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"TFMPE combines likelihood factorisation with tokenised flow matching to enable efficient hierarchical SBI from single-site simulations, producing well-calibrated posteriors at lower computational cost on a new benchmark and real models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.19612","ref_index":115,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"QCD-factorization amplitudes from flavour symmetries: beyond the $SU(3)$ symmetric case","primary_cat":"hep-ph","submitted_at":"2026-04-21T15:59:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A data-driven SU(3)-breaking analysis of B to PP decays yields QCD-factorization amplitudes that resemble dynamical predictions and require no enhanced annihilation terms.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"form-factor at zero momentum transfer,Nucl. Phys. B722(2005) 149 [hep-ph/0504016]. [113] C. Bourrely, I. Caprini and L. Lellouch,Model-independent description ofB→πlνdecays and a determination of|Vub|,Phys. Rev. D79(2009) 013008 [0807.2722]. [114] M. Beneke and M. Neubert,Flavor singlet B decay amplitudes in QCD factorization,Nucl. Phys. B651(2003) 225 [hep-ph/0210085]. - 47 - [115] B. Meli' c and M. Reboud,Form factors and phenomenology ofB (s) andD (s) semileptonic decays toηandη′,JHEP10(2025) 025 [2507.13734]. [116] Y.-J. Zhang, X.-G. Wu, D.-D. Hu and L. Zeng,η−η′mixing and its application in the B+,D +,D + s →η(′)ℓ+νℓdecays,Phys. Rev. D112(2025) 076001 [2506.13214]. [117] R. Mandal, P.S. Patil and I. Ray,Probing the inverse moment ofB s-meson distribution"},{"citing_arxiv_id":"2604.08648","ref_index":35,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"High-dimensional inference for the $\\gamma$-ray sky with differentiable programming","primary_cat":"astro-ph.HE","submitted_at":"2026-04-09T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A differentiable forward model and likelihood enable probabilistic inference over many spatial morphologies for the Galactic Center gamma-ray Excess using variational methods on GPUs.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"with hundreds of parameters. This is in contrast to cur- rent public implementations of NPTF, which cannot effi- ciently include real-time generated templates at inference and are restricted to a modest number of parameters with traditional Monte Carlo sampling techniques. The constructed likelihood is wrapped using the prob- abilistic programming frameworkNumPyro[35], which al- lows for flexible specification of complex forward models as well as performing inference on them using gradient- D Public implementation of the pipeline 4 based techniques. In SVI an approximation for the posterior distribu- tion, parameterized byφand denotedq φ(θ), is ob- tained by minimizing the reverse KL-divergence be- tween the true and variational posterior distributions,"},{"citing_arxiv_id":"2604.18598","ref_index":28,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Bathymetry Reconstruction by Bayesian Inference","primary_cat":"stat.AP","submitted_at":"2026-04-09T08:47:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Bayesian inference reconstructs bathymetry from point water height measurements, improving NRMSE over adjoint optimization on real wave flume data while quantifying uncertainty.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"We use the Metropolis-Hastings (MH) algorithm [24, 25] for sampling, because of its simplicity. Tests comparing the MH algorithm with the pre- conditioned Crank-Nicolson algorithm (pCN) [26] algorithm showed that 6 the MH algorithm achieves similar accuracy in our case. More advanced MCMC methods exist, such as Hamiltonian Monte Carlo [27], No-U-Turn sampler [28] or the Metropolis-adjusted Langevin algorithm [29], but require gradient information of the forward model. Including gradient information in the sampling process is possible but would require a computationally costly backward evaluation of the forward model in every iteration, similar to ad- joint optimization methods. This is also left for future work."},{"citing_arxiv_id":"2604.06388","ref_index":26,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Determining the Host Stars of Planets in Binary Star Systems with Asterodensity Profiling: Investigating the Canonical Radius Gap","primary_cat":"astro-ph.EP","submitted_at":"2026-04-07T19:19:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Probabilistic host-star assignments via asterodensity profiling suggest the exoplanet radius gap is less empty in binary systems once possible circumsecondary planets are included.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2603.13053","ref_index":110,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A unified harmonic framework for dark siren cosmology","primary_cat":"astro-ph.CO","submitted_at":"2026-03-13T15:03:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The GW-galaxy cross-correlation method, unified with spectral sirens in a harmonic framework, can measure H0 to 1% and Omega_m to 5% precision with 2 years of data from next-generation detectors like Einstein Telescope and Cosmic Explorer.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"017. [108] A. Amon and G. Efstathiou, A non-linear solu- tion to the S 8 tension?, MNRAS516, 5355 (2022), arXiv:2206.11794 [astro-ph.CO]. [109] H. A. Winther, S. Casas, M. Baldi, K. Koyama, B. Li, L. Lombriser, and G.-B. Zhao, Emulators for the non- linear matter power spectrum beyond Λ CDM, PhRvD 100, 123540 (2019), arXiv:1903.08798 [astro-ph.CO]. [110] M. P. van Daalen, J. Schaye, C. M. Booth, and C. Dalla Vecchia, The effects of galaxy formation on the mat- ter power spectrum: a challenge for precision cosmol- ogy, MNRAS415, 3649 (2011), arXiv:1104.1174 [astro- ph.CO]. [111] N. E. Chisari, A. J. Mead, S. Joudaki, P. G. Ferreira, A. Schneider, J. Mohr, T. Tr¨ oster, D. Alonso, I. G. McCarthy, S."},{"citing_arxiv_id":"2601.21125","ref_index":32,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects","primary_cat":"astro-ph.SR","submitted_at":"2026-01-28T23:46:32+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A new compact hierarchical triple main-sequence star system G1010 was discovered through combined low- and high-SNR spectroscopy, Gaia DR3 data, and TESS light curve analysis, showing an inner eclipsing binary rather than a compact object companion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.08666","ref_index":54,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Stochastic gravitational-wave background search using data from five pulsar timing arrays","primary_cat":"astro-ph.CO","submitted_at":"2025-12-09T14:52:04+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Combined five-PTA dataset yields posterior on SGWB power-law amplitude and index consistent with nonzero signal but below 5-sigma significance, with reconstructed angular correlations matching the Hellings-Downs prediction.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.15352","ref_index":42,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"People readily follow personal advice from AI but it does not improve their well-being","primary_cat":"cs.HC","submitted_at":"2025-11-19T11:22:48+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Large longitudinal RCT finds high rates of following AI personal advice but no sustained well-being gains versus a hobbies control condition.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.18749","ref_index":54,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Symbolic Emulators for Cosmology: Accelerating Cosmological Analyses Without Sacrificing Precision","primary_cat":"astro-ph.CO","submitted_at":"2025-10-21T15:57:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Symbolic emulators approximate key Lambda CDM functions to 0.001-0.05% accuracy across relevant redshifts and Omega_m values, enabling faster 3x2pt inference with consistent results.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.05219","ref_index":5,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Conversational AI increases political knowledge as effectively as self-directed internet search","primary_cat":"cs.HC","submitted_at":"2025-09-05T16:26:55+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Conversational AI matches self-directed internet search in increasing belief in true political information and decreasing belief in misinformation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.21410","ref_index":52,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Sifting for a Stream: The Morphology of the $300S$ Stellar Stream","primary_cat":"astro-ph.GA","submitted_at":"2025-06-26T15:57:54+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"300S stellar stream exhibits three density peaks, smooth width variations, a possible 4.7 degree gap, and a kink modeled as resulting from Large Magellanic Cloud interaction across its full known footprint.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.03969","ref_index":38,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Differentiable Fuzzy Cosmic-Web for Field Level Inference","primary_cat":"astro-ph.CO","submitted_at":"2025-06-04T14:01:32+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Introduces HICOBIAN, a differentiable fuzzy hierarchical cosmic-web bias model using sigmoid gradients for smooth region transitions, enabling accurate Bayesian field-level reconstruction of primordial density fields validated by Fourier-space statistics.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2411.12021","ref_index":166,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","primary_cat":"astro-ph.CO","submitted_at":"2024-11-18T20:03:34+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"DESI DR1 full-shape galaxy clustering constrains Omega_m = 0.296 ± 0.010, H0 = 68.63 ± 0.79 km/s/Mpc, and sigma_8 = 0.841 ± 0.034, consistent with LambdaCDM and Planck.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"not employ the emulator, or validate chains run with an emulator by recalculating the likelihood with the model without an emulator at each point of the chain. Although this is slower, it means the results obtained from DESI data are robust against possible emulator inaccuracies. MCMC chains presented in this paper are either run with the No U-Turn Sampler (NUTS [166], as implemented in blackjax [167]14), when emulating the galaxy power spectrum model or with the MCMC sampler [168, 169] implemented inCobaya 15 when running without an emulator 10.Fiducial cosmology. We must choose a fiducial cosmology to create the 3D galaxy catalogues. This is the cosmology used to transform the redshifts into comoving dis- tances expressed inh −1Mpc."},{"citing_arxiv_id":"1906.11199","ref_index":20,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Deployable probabilistic programming","primary_cat":"cs.PL","submitted_at":"2019-06-20T15:17:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Design guidelines and a Go library (Infergo) for deploying probabilistic programming in production systems, with benchmark comparisons.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1904.02180","ref_index":41,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences","primary_cat":"astro-ph.IM","submitted_at":"2019-04-03T18:04:57+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"dynesty is an open-source Python package for dynamic nested sampling that improves efficiency in Bayesian posterior and evidence estimation compared to MCMC on certain problems.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}