diff --git a/bibliography/pyautomemory.bib b/bibliography/pyautomemory.bib index d14c746..fa4f142 100644 --- a/bibliography/pyautomemory.bib +++ b/bibliography/pyautomemory.bib @@ -16284,3 +16284,45 @@ @article{EuclidQ1DSPL archivePrefix = {arXiv}, eprint = {2503.15327} } + +@misc{Fung2026, + author = {Fung, Leo W. H. and Broadhurst, Tom and Li, Sung Kei and Lim, Jeremy and Manzoni, Giorgio and Smoot, George F.}, + title = {{Model independent lensing sub-structure detection with multiply-imaged star clusters constellations}}, + year = {2026}, + archivePrefix = {arXiv}, + eprint = {2608.21253}, + primaryClass = {astro-ph.CO}, + url = {https://arxiv.org/abs/2608.21253} +} + +@misc{Lovick2025, + author = {Lovick, Toby and Yallup, David and Piras, Davide and Spurio Mancini, Alessio and Handley, Will}, + title = {{High-Dimensional Bayesian Model Comparison in Cosmology with GPU-accelerated Nested Sampling and Neural Emulators}}, + year = {2025}, + archivePrefix = {arXiv}, + eprint = {2509.13307}, + primaryClass = {astro-ph.CO}, + url = {https://arxiv.org/abs/2509.13307} +} + +@misc{Williams2026Shape, + author = {Williams, Liliya L. R. and Perera, Derek C. and Liesenborgs, Jori and Meena, Ashish K. and Limousin, Marceau and Ecker, Leon R.}, + title = {{Shape Degeneracies: the likely culprit for the differences between lens mass models of galaxy clusters}}, + year = {2026}, + archivePrefix = {arXiv}, + eprint = {2609.27147}, + primaryClass = {astro-ph.CO}, + note = {Submitted to OJA}, + url = {https://arxiv.org/abs/2609.27147} +} + +@misc{Roche2026, + author = {Roche, Cian and McDonald, Michael and Natarajan, Priyamvada and Sharon, Keren and Dutra, Isaque and Meneghetti, Massimo and Vogelsberger, Mark}, + title = {{Host Dependence and Line-of-Sight Effects on Galaxy-Galaxy Strong Lensing in Clusters}}, + year = {2026}, + archivePrefix = {arXiv}, + eprint = {2608.30079}, + primaryClass = {astro-ph.CO}, + note = {Submitted to ApJ}, + url = {https://arxiv.org/abs/2608.30079} +} diff --git a/reading-queue.md b/reading-queue.md index 988c39f..8c6a8b8 100644 --- a/reading-queue.md +++ b/reading-queue.md @@ -82,13 +82,13 @@ The Case for Space: Estimating Precise Time Delays from Ground- and Space-Based JWST Discovery of Strong Lensing from a Galaxy Cluster at Cosmic Noon: Giant Arcs and a Highly Concentrated Core of XLSSC 122 — 2508.08356 HOLISMOKES XVIII: Detecting strongly lensed SNe Ia from time series of multi-band LSST-like imaging data The collar of early-type galaxies -- probing evolution by focusing on the inner stellar density profile -High-Dimensional Bayesian Model Comparison in Cosmology with GPU-accelerated Nested Sampling and Neural Emulators — 2509.13307 +DONE 2026-10-21 — High-Dimensional Bayesian Model Comparison in Cosmology with GPU-accelerated Nested Sampling and Neural Emulators — 2509.13307 THE STELLAR AND DARK MATTER DISTRIBUTIONS IN ELLIPTICAL GALAXIES MEASURED BY STACKED WEAK GRAVITATIONAL LENSING -Model independent lensing sub-structure detection with multiply-imaged star clusters constellations — 2608.21253 +DONE 2026-10-21 — Model independent lensing sub-structure detection with multiply-imaged star clusters constellations — 2608.21253 On what scales does strong lensing robustly constrain the mass profile of low-mass perturbers? — 2608.20454 Measuring Extragalactic Microlens Masses and Motions in Strongly Lensed Quasar Systems with Intensity Interferometry — 2608.27577 TDCOSMO XXIX: JWST/NIRSpec IFU Spatially Resolved Kinematics of Three Time-delay Lenses — 2609.03089 -Host Dependence and Line-of-Sight Effects on Galaxy-Galaxy Strong Lensing in Clusters — 2608.30079 +DONE 2026-10-21 — Host Dependence and Line-of-Sight Effects on Galaxy-Galaxy Strong Lensing in Clusters — 2608.30079 DONE 2026-09-11 — TDCOSMO XXVIII. The Hubble constant from the quadruply lensed quasar J1537$-$3010 with precise time delays — 2609.00179 HOLISMOKES -- XVIII. Cosmology with strongly lensed type II supernovae: Effects of instrumental setups on $H_0$ — 2608.26331 DONE 2026-09-01 — Mapping the Information Geometry of an Unresolved Dark Matter Population using a Differentiable Strong Lensing Simulator — 2608.18224 @@ -109,7 +109,7 @@ SN Helios: A Multiply Imaged Type II Supernova Opening Time-Delay Cosmography be Joint Model-independent Constraints on the Post-Newtonian Parameter and Cosmic Curvature from Galaxy-scale Strong Lensing, SNe Ia, BAO, and Cosmic Chronometers — 2609.29377 Wave-Optics Imprints of Warm Dark Matter Subhalos with Prompt Cusps on Strongly Lensed Gravitational Waves — 2609.28626 A sub-100 pc view at z~5 of a Multiply-Imaged Massive Quiescent Galaxy — 2609.28474 -Shape Degeneracies: the likely culprit for the differences between lens mass models of galaxy clusters — 2609.27147 +DONE 2026-10-21 — Shape Degeneracies: the likely culprit for the differences between lens mass models of galaxy clusters — 2609.27147 Reducing False Positives in Strong-Lens Searches with Generalized-Mean Consensus of Machine-Learning Ensembles in the Kilo-Degree Survey — 2609.24891 LATED: JWST integral field spectroscopy of a galaxy caught in chemical infancy at $z=4.8$ behind Abell 2744 — 2609.24589 Probing modified gravity with galaxy-cluster-lensed gravitational-wave time delays: impact of systematic effects — 2609.24351 diff --git a/wiki/lensing/log.md b/wiki/lensing/log.md index 0523552..04b1308 100755 --- a/wiki/lensing/log.md +++ b/wiki/lensing/log.md @@ -251,3 +251,15 @@ were stored in the repository. - Added missing canonical entries `Sahu2025DSPL` (ApJ 991, 72) and `EuclidQ1DSPL` (A&A 711, A29), checking DOI, arXiv ID, and title for duplicates. - Added compact support and scope notes in `sources/gr-cosmology.md`, distinguishing the AGEL cosmography measurement from the Euclid Q1 candidate-discovery and modelling study. - Verified against arXiv:2504.00656, arXiv:2503.15327, and their published records. Author confirmed that “Sheu” meant Sahu and that the Li reference was the Euclid Q1 paper. + +## 2026-10-21 — Catch-up since 2026-10-16 + +**intake:** none. + +**cite** (canonical bib entry + compact stub, verified against arXiv; no journal record yet): +- `Fung2026` (arXiv:2608.21253) — model-independent substructure detection with JWST star-cluster constellations → `sources/dark-matter-substructure.md`. +- `Williams2026Shape` (arXiv:2609.27147) — shape degeneracies behind differing cluster mass maps → `sources/degeneracies-systematics.md`. +- `Roche2026` (arXiv:2608.30079) — host dependence and line-of-sight effects on cluster GGSL → `sources/cluster-lensing.md`. +- `Lovick2025` (arXiv:2509.13307) — GPU-accelerated nested sampling for cosmological model comparison → `../methods/sources/samplers.md` (no lensing home; logged in the methods log too). + +**queue:** none added. The four existing `reading-queue.md` lines were marked `DONE 2026-10-21` in place. diff --git a/wiki/lensing/sources/cluster-lensing.md b/wiki/lensing/sources/cluster-lensing.md index d788517..87f1891 100755 --- a/wiki/lensing/sources/cluster-lensing.md +++ b/wiki/lensing/sources/cluster-lensing.md @@ -150,6 +150,14 @@ status: stub **Do not use for TODO:** - Evidence until the paper identity and canonical key are verified. +## Roche 2026 — host dependence and LOS effects on cluster GGSL + +**Canonical BibTeX key:** `Roche2026` +**Reference:** Host Dependence and Line-of-Sight Effects on Galaxy-Galaxy Strong Lensing in Clusters; arXiv:2608.30079 +**Concepts:** [[cluster-lensing]], [[line-of-sight-effects]] + +**Supports:** +- Revisits the observed-vs-simulated galaxy–galaxy strong-lensing excess in clusters: correlated LOS material raises P_GGSL by a few to ~15%, hydro runs give up to 10x more GGSL than DM-only, P_GGSL scales roughly as θ_E^2, and the residual tension depends on the field-of-view definition. ## See also diff --git a/wiki/lensing/sources/dark-matter-substructure.md b/wiki/lensing/sources/dark-matter-substructure.md index b86f3e9..dab63cc 100755 --- a/wiki/lensing/sources/dark-matter-substructure.md +++ b/wiki/lensing/sources/dark-matter-substructure.md @@ -539,6 +539,15 @@ Per-paper stubs of substructure-detection literature. All marked stub. **Do not use for:** - Claims about how line-of-sight structure, external multipoles, or the mass-sheet transform specifically interact with the radial subhalo signal — the paper does not settle this; it remains an open question to check against the text before citing. +## Fung 2026 — model-independent substructure detection with star-cluster constellations + +**Canonical BibTeX key:** `Fung2026` +**Reference:** Model independent lensing sub-structure detection with multiply-imaged star clusters constellations; arXiv:2608.21253 +**Concepts:** [[dark-matter-substructure]], [[cluster-lensing]] + +**Supports:** +- Proposes a lens-model-free, data-driven "geometrical-duality" test (the optical Liouville theorem applied across scales) for sub-resolution substructure, applied to 11 multiply imaged star clusters in SMACS0723 with JWST; one outlier pair is consistent with CDM subhaloes of 10^8–10^9 M_sun. + ## See also - [[dark-matter-substructure]] diff --git a/wiki/lensing/sources/degeneracies-systematics.md b/wiki/lensing/sources/degeneracies-systematics.md index 9d9dcfd..fd816e0 100755 --- a/wiki/lensing/sources/degeneracies-systematics.md +++ b/wiki/lensing/sources/degeneracies-systematics.md @@ -205,6 +205,14 @@ status: stub **Do not use for:** - More specific quantitative results, modelling assumptions, or interpretation beyond the verified title/reference metadata without checking the paper text. +## Williams 2026 — shape degeneracies in cluster mass models + +**Canonical BibTeX key:** `Williams2026Shape` +**Reference:** Shape Degeneracies: the likely culprit for the differences between lens mass models of galaxy clusters; arXiv:2609.27147 +**Concepts:** [[cluster-lensing]], [[mass-sheet-degeneracy]], [[source-position-transformation]] + +**Supports:** +- Argues analytically that generalized shape degeneracies, not the mass-sheet or source-position transformation, drive <30 kpc differences between cluster mass maps; they are suppressed near tight image groupings and shift time delays by ~1% (up to ~10% for some sources) in MACS J0416. ## See also diff --git a/wiki/methods/log.md b/wiki/methods/log.md index ba726d3..93386f3 100644 --- a/wiki/methods/log.md +++ b/wiki/methods/log.md @@ -152,3 +152,10 @@ and the reusable task-comparability lesson. Earlier benchmark sections remain historical evidence pending a separate destination/provenance audit. The write contract now routes inference campaigns through Insight and profiling through Pulse; permanence alone does not make a campaign record Memory content. + +## 2026-10-21 — Catch-up since 2026-10-16 + +Lensing catch-up filed `Lovick2025` (arXiv:2509.13307, GPU-accelerated nested +sampling with neural emulators for cosmological model comparison) as a cite-tier +stub in `sources/samplers.md`, verified against arXiv. No benchmark verdict was +added. See the lensing log for the rest of the batch. diff --git a/wiki/methods/sources/samplers.md b/wiki/methods/sources/samplers.md index b3f1f6e..c2b600b 100644 --- a/wiki/methods/sources/samplers.md +++ b/wiki/methods/sources/samplers.md @@ -191,3 +191,12 @@ hopping, and the libraries that implement them. **Do not use for:** - An evidence estimator or proof of multimodal coverage. + +## Lovick 2025 — GPU-accelerated nested sampling for cosmological model comparison + +**Canonical BibTeX key:** `Lovick2025` +**Reference:** High-Dimensional Bayesian Model Comparison in Cosmology with GPU-accelerated Nested Sampling and Neural Emulators; arXiv:2509.13307 +**Concepts:** [[gpu-nested-sampling]], [[nested-sampling]] + +**Supports:** +- Demonstrates GPU nested sampling with JAX neural emulators giving evidences and Bayes factors for a 39-dimensional ΛCDM vs w0wa cosmic-shear analysis in ~2 days on one A100, putting nested sampling on equal footing with MCMC-plus-decoupled-evidence methods.