Papers waiting to be read and filed. Format:
## <Section>headers group papers by domain (matchingwiki/<domain>/where one exists).- One paper per line — a bare title, optionally followed by
— <arXiv id or URL>. - Add the ref whenever you know it. It is what lets the Dashboard link the
paper's arXiv abstract page and put a 📄 one-tap PDF button beside it; without
one the board can only offer an arXiv title search, which costs a results
page and a squint per paper.
scripts/backfill_arxiv_refs.py(nightly, via.github/workflows/arxiv_refs.yml) fills in the ones nobody wrote by hand, and only when exactly one arXiv paper's title matches. - A read/consumed paper is never deleted: prefix its line with
DONE <YYYY-MM-DD> —and leave it in place (the reading history). - Not every line is a paper. Two kinds are not, and marking them keeps the
Dashboard from offering a download button for a heading and stops the nightly
ref backfill spending an arXiv lookup on one:
__Bold Text__on its own line is a sub-heading grouping the papers below it. Rendered as a heading, never counted, never looked up.NOTE <text>is an annotation — a remark, a link that is not a paper, a stray line of pasted prose. Sibling of theDONEprefix: same shape, same never-delete rule. A bare non-arXiv link counts as one automatically.scripts/backfill_arxiv_refs.py --mark-unresolvedapplies the prefix in bulk to lines it could not identify — run it after reading a dry run, since an unresolved title is more often a real paper whose line lost something (a LaTeX redshift, a wrapped subtitle) than a genuine non-paper.- A line that is only an arXiv link is still a paper — the title was just
never written, so the board labels it
arXiv:<id>.
- Filing a read paper: add its canonical entry to
bibliography/, stub it in the matchingwiki/<domain>/sources/*.mdpage perwiki/AGENTS.md, then mark the line DONE and runmake validate.
(Moved from admin_jammy/papers.md on 2026-05-22, when this repo — then
PyAutoPaper, now PyAutoMemory — became the unified knowledge repo.)
DONE 2026-08-21 — The X-Ray Continuum Emission Region in the Lensed Quasar SDSS J133907.23+131038.6 is Much Smaller than the Accretion Disk Confirmation of the Finch Flatter-Fainter Relation for the Quadruple Images of Lensed Point Sources — 2608.17116 The Koi Pond: A Strongly Lensed Protocluster Core hosting a Diverse Population of DSFGs — 2608.15997 DONE 2026-10-07 — Addressing position anomalies in the Strong Gravitational Lensing System HS~0810+2554 through Dark Matter Subhalos — 2608.15554 The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc — 2608.02730 Galaxy-LRD Strong Lenses: A Missing Population? — 2608.02739 Cosmic CORALS: Timing the Universe with high-z star clusters — 2607.19472 Polar coordinate transformations for machine learning based dark matter subhalo detection in strong gravitational lenses — 2607.02663 XShooter DESI Lens Program: Sample characterization — 2607.08562 Strong-lensing effects in high-redshift massive black-hole binary population inference — 2607.03345
LEGGOS III: Mapping Star Formation and Dust in Gravitationally Lensed Galaxies with SUMAC, a UMAP and Clustering Framework LEGGOS II: A Strong Lens Model and Source-Plane Projection of the Clumpy Star-Forming Galaxy SGASJ111020.0+645950.8 at z=2.48 — 2606.20804
Dynamical models of cluster members to probe the total mass properties of cluster subhalos. I. A comparison with parametric strong lensing models — 2606.05298
COOL-LAMPS IX: A Rare Duo of Quasars Each Lensed by a Single Massive Galaxy Cluster — 2605.13514
Beyond collective fluctuations: probing micro-image swarms in lensed quasars with intensity interferometry — 2605.02181
Constraining Axion-like Particles through Multi-epoch Monitoring of Strong Gravitational Lenses — 2602.12863
Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy — 2601.22245
Detecting Strongly-Lensed Supernovae in Wide-field Space Telescope Imaging via Deep Learning — 2512.19886
Microlensing Black Hole Shadows-II: Constraining Primordial Black Hole Dark Matter using the photon rings of M87 and Sgr A* — 2512.20037
SLICE -- Combining Strong Lensing and X-ray in AC,114. Insights into the Merger Scenario
Tracing Structure: Shape and Centroid Deviations in 39 Strong Lensing Clusters as a Test of Cluster Formation Predictions — 2511.22661
A Super-Eddington, Lensing-Magnified Quasar at observed with JWST
Caustic crossings in giant arcs with extended dark matter objects — 2511.20761
Kinematic Mapping of Giant Arcs: A New Method to Locate Lensing Critical Curves — 2511.18479
VENUS: A Strongly Lensed Clumpy Galaxy at behind the Galaxy Cluster MACS J0257.1-2325
Investigating the Dark Energy Constraint from Strongly Lensed AGN at LSST-Scale — 2511.13669
The Chandra Strong Lens Sample: Measuring the Dynamical States and Relaxation Fraction of a Sample of 28 Strong Lensing Selected Galaxy Clusters — 2511.12707
The Impact of Orbital Anisotropy Assumptions in Lensing-Dynamics Modeling — 2511.12013
SourceREACH (Source REconstruction of Arcs behind Cluster Halos): A New Source Reconstruction Algorithm Optimized for Giant Arcs and Galaxy Cluster Lenses
JWST Lensed Quasar Dark Matter Survey III: Dark Matter Sensitive Flux Ratios and Warm Dark Matter Constraint from the Full Sample. — 2511.07765
A Strong Gravitational Lensing Model of PSZ2 G118.46+39.32 — 2511.08300
CSST Strong Lensing Preparation: Cosmological Constraints Forecast from CSST Galaxy-Scale Strong Lensing — 2511.08030
The complicated nature of the X-ray emission from the field of the strongly lensed hyperluminous infrared galaxy PJ1053+60 at z=3.54
A cosmographic analysis using DESI-DR2 and strong lensing: I. Time-Delay measurements — 2511.00788
A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements — 2511.00789
Detecting dark matter substructure with lensed quasars in optical bands — 2510.09148
CURLING -- II. Improvement on the Inference from Pixelized Cluster Strong Lens Modeling
iPTF16geu through the lens of thermonuclear explosion models — 2510.01160
Forecasting the Observable Rates of Gravitationally Lensed Supernovae for the PASSAGES Dusty Starbursts — 2510.00923
The Case for Space: Estimating Precise Time Delays from Ground- and Space-Based Observations of Lensed Supernovae with Glimpse — 2509.25350
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
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
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 2026-09-11 — 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
Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils — 2603.02811 Core Scouring Dynamics and Gravitational Wave Consequences: Constraints on Supermassive Black Hole Binary Hardening — 2601.07762 Stellar cores live long and prosper in cuspy dark matter halos — 2512.05719 Recoiling Black Hole Candidates from Spatially Offset Broad Emission Lines in MaNGA — 2512.00174 Accretion, Jets, and Recoil in Merging Supermassive Binary Black Holes — 2510.05883 Off-center black hole seed formation? Implications for high and low redshift massive black holes — 2509.12306 Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA — 2509.01674 Identifying massive black hole binaries via light curve variability in optical time-domain surveys — 2508.21510 A Large Systematic Search for Close Supermassive Binary and Rapidly Recoiling Black Holes -- IV. Ultraviolet spectroscopy — 2501.10574 Elliptical (E) and ellicular (ES) galaxies in the M_bh-M_*,sph diagram, and a merger-driven explanation for the origin of ES galaxies, anti-truncated stellar discs in lenticular galaxies, and the Sersicification of E galaxy light profiles — 2501.09953 HST Observations within the Sphere of Influence of the Powerful Supermassive Black Hole in PKS0745-191 — 2501.03339 Primordial Black Hole stellar microlensing constraints: understanding their dependence on the density and velocity distributions — 2501.02610 Probing the Merger Rates of Supermassive Black Holes and Galaxies with Gravitational Waves — 2501.02748 Two radio cores in GPS J1543-0757: a new dual supermassive black hole system? — 2408.06187 Can quasars, triggered by mergers, account for NANOGrav's stochastic gravitational wave background? Is your stochastic signal really detectable? — 2412.10468 Beyond the Goldilocks Zone: Identifying Critical Features in Massive Black Hole Formation — 2412.08829 Massive black holes or stars first: the key is the residual cosmic electron fraction — 2412.02763 Wandering and escaping: recoiling massive black holes in cosmological simulations — 2412.02374 Large-scale dual AGN in large-scale cosmological hydrodynamical simulations — 2411.15297 Super-Size Me: The Big Multi-AGN Catalog (The Big MAC), Data Release 1: The Source Catalog — 2411.12799 A Recent Supermassive Black Hole Binary in the Galactic Center Unveiled by the Hypervelocity Stars — 2411.09278 Primordial black holes as supermassive black holes seeds — 2411.03448 Connecting Inflation to the NANOGrav 15-year Data Set via Massive Gravity — 2410.09658 Active Galactic Nuclei and Host Galaxies in COSMOS-Web. II. First Look at the Kpc-scale Dual and Offset AGN Population — 2405.14980 Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations II: Unique Stellar Kinematics in Integral Field Unit Spectroscopy — 2407.14061 The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling — 2407.09949 PKS 2131-021 -- Discovery of Strong Coherent Sinusoidal Variations from Radio to Optical Frequencies: Compelling Evidence for a Blazar Supermassive Black Hole Binary — 2407.09647 Dynamics around supermassive black holes: Extreme mass-ratio inspirals as gravitational-wave sources — 2406.19443 Supermassive black hole mass measurement in the spiral galaxy NGC 4736 Using JWST/NIRSpec stellar kinematics — 2505.09941
The Host Galaxies of PTA Sources: Converting Supermassive BH Binary Parameters into EM Observables — 2505.11598 First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence — 2505.12591 Accretion onto supermassive black hole binaries — 2405.14843 Astrometric Jitter as a Detection Diagnostic for Recoiling and Slingshot Supermassive Black Hole Candidates — 2405.11026 Detection and Prediction of Future Massive Black Hole Mergers with Machine Learning and Truncated Waveforms — 2405.11340 How do Primordial Black Holes change the Halo Mass Function and Structure? — 2405.11381 Tip of the iceberg: overmassive black holes at 4<z<7 found by JWST are not inconsistent with the local MBH-M⋆ relation
https://arxiv.org/pdf/2103.16254.pdf https://arxiv.org/pdf/2112.03576.pdf
NOTE as several triplet SMBHs have NOTE been observed in the local Universe (Deane et al. 2014; NOTE Pfeifle et al. 2019; Liu et al. 2019; Kollatschny et al. NOTE 2020).
NOTE , shrink the orbits further (see NOTE e.g. Amaro-Seoane et al. 2022, for a review).
The Redshift Difference in Gravitational Lensed Systems: A Novel Probe of Cosmology — 2308.07529 Evidence for a milli-parsec separation Supermassive Black Hole Binary with quasar microlensing The Black Hole Mass Function Across Cosmic Times II. Heavy Seeds and (Super)Massive Black Holes — 2206.07357 Black Hole Mass Measurements of Early-Type Galaxies NGC 1380 and NGC 6861 Through ALMA and HST Observations and Gas-Dynamical Modeling — 2206.09043 A Bayesian Approach To The Halo-Galaxy-SMBH Connection Through Cosmic Time Detection of an X-ray quasar in a gravitationally-lensed z=10.3 galaxy suggests that early supermassive black holes originate from heavy seeds Mass-redshift dependency of Supermassive Black Hole Binaries for the Gravitational Wave Background — 2305.18293 SLICK: Strong Lensing Identification of Candidates Kindred in gravitational wave data — 2403.02994 A Population Study for Searching Supermassive Binary Black Holes in Active Galactic Nuclei: Continuum Spectral Features and Periodic Variabilities — 2608.25507
The heartbeat of stellar halos: Insights from the stellar halo mass-metallicity relation — 2512.07780 Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations — 2504.18042 The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations — 2412.03406 Tracing the origins of galaxy lopsidedness across cosmic time — 2411.19426 Photometric properties of classical bulge and pseudo-bulge galaxies at 0.5≤z<1.0 — 2407.21527 ALESS-JWST: Joint (sub-)kiloparsec JWST and ALMA imaging of z∼3 submillimeter galaxies reveals heavily obscured bulge formation events — 2407.15846 Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows — 2407.10760 Characterising Tidal Features Around Galaxies in Cosmological Simulations — 2404.12436 A forward-modelling approach to overcome PSF smearing and fit flexible models to the chemical structure of galaxies — 2403.08175 A two-phase model of galaxy formation: I. The growth of galaxies and supermassive black holes — 2311.05030 Galaxy quenching at the high redshift frontier: A fundamental test of cosmological models in the early universe with JWST-CEERS — 2311.02526 Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects — 2310.15234 A JWST investigation into the bar fraction at redshifts 1 < z < 3 — 2309.10038 Identifying the disc, bulge, and intra-halo light of simulated galaxies through structural decomposition Exploring the Angular Momentum - Atomic Gas Content Connection with EAGLE and IllustrisTNG — 2307.02722 Bulgeless disks, dark galaxies, inverted color gradients, and other expected phenomena at higher z. The chromatic surface brightness modulation (CMOD) effect — 2303.12845 Has JWST already falsified dark-matter-driven galaxy formation? — 2210.14915 A shot in the Dark (Ages): a faint galaxy at z=9.76 confirmed with JWST CEERS Key Paper IV: The Diversity of Galaxy Structure and Morphology at z=3-9 with JWST NOTE The MillenniumTNG Project: Many papers 2022 The MASSIVE Survey. XVIII. Deep Wide-Field K-band Photometry and Local Scaling Relations for Massive Early-Type Galaxies — 2210.08043 Sizes and mass profiles of candidate massive galaxies discovered by JWST at 7<z<9: evidence for very early formation of the central ∼100 pc of present-day ellipticals — 2305.17162
The AIDA-TNG project: 3D halo shapes — 2512.15856 The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models — 2512.15869 Connection between galaxy morphology and dark-matter halo structure II: predicting disk structure from dark-matter halo properties — 2512.13822 Buried but not destroyed: the evolution from prompt cusps to NFW haloes — 2512.13804 Forecasting Dark Matter Subhalo Constraints from Stellar Streams using Implicit Likelihood Inference — 2512.07960 Probing the Nature of Dark Matter Self-Interactions Through Observations of Massive Black Hole Mergers — 2511.13220 Reaching for the Edge II: Stellar Halos out to Large Radii as a Tracer of Dark Matter Halo Mass — 2511.10723 Detecting dark matter sub-halos in the Galactic plane with the Cherenkov Telescope Array Observatory — 2501.09789 Implications of the intriguing constant inner mass surface density observed in dark matter halos — 2501.03761 Dwarf galaxies imply dark matter is heavier than 2.2×10−21eV — 2405.20374 Effectiveness of halo and galaxy properties in reducing the scatter in the stellar-to-halo mass relation — 2405.15191 Hydrodynamical simulations of merging galaxy clusters: giant dark matter particle colliders, powered by gravity — 2405.00140 The Influence of Baryons on Low-mass Haloes — 2403.17044 Predicting the Scaling Relations between the Dark Matter Halo Mass and Observables from Generalised Profiles I: Kinematic Tracers — 2403.07352 Brightest Cluster Galaxy Offsets in Cold Dark Matter — 2402.00928 Micro galaxies as a falsifiable prediction of LCDM cosmology No Catch-22 for Fuzzy Dark Matter: testing substructure counts and core sizes via high-resolution cosmological simulations — 2311.03591 Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties — 2311.03491 Beyond Best-Fits and Model Selection -- Introducing "Reliability" of cusp-core inference of dark matter halos — 2310.20272 Can prompt cusps of WIMP dark matter be detected as individual gamma-ray sources? — 2310.15214 The formation of cores in galaxies across cosmic time -- the existence of cores is not in tension with the LCDM paradigm — 2310.13055 Till the core collapses: the evolution and properties of self-interacting dark matter subhalos — 2310.09910 The abundance of core--collapsed subhalos in SIDM: insights from structure formation in ΛCDM Tracking the evolution of satellite galaxies: mass stripping and dark-matter deficient galaxies — 2212.12090 New Constraints on Warm Dark Matter from the Lyman-α Forest Power Spectrum — 2209.14220 Review of solutions to the Cusp-core problem of the ΛCDM Model Matching the mass function of Milky Way satellites in competing dark matter model The shape of dark matter haloes: results from weak lensing in the Ultraviolet Near-Infrared Optical Northern Survey (UNIONS) — 2209.09088 A lensing multi-messenger channel: Combining LIGO-Virgo-Kagra lensed gravitational-wave measurements with Euclid observations Chandra Observations of Spikey: A Possible Self-lensing Supermassive Black Hole Binary System The massive relic galaxy NGC 1277 is dark matter deficient. From dynamical models of integral-field stellar kinematics out to five effective radii — 2303.11360 The impact of baryonic potentials on the gravothermal evolution of self-interacting dark matter haloes — 2306.08028 Is the mysterious {\it Punctum} a primordial black hole? — 2608.25423
AstroAlertBench: Evaluating the Accuracy, Reasoning, and Honesty of Multimodal LLMs in Astronomical Classification — 2605.05573 ALABI: Active Learning for Accelerated Bayesian Inference — 2603.18259 Probabilistic Graphical Models in Astronomy — 2601.16959 How to embed any likelihood into SBI: Application to Planck + Stage IV galaxy surveys and Dynamical Dark Energy — 2507.22990 IRIS: A Bayesian Approach for Image Reconstruction in Radio Interferometry with expressive Score-Based priors — 2501.02473 SIDE-real: Truncated marginal neural ratio estimation for Supernova Ia Dust Extinction with real data LtU-ILI: An All-in-One Framework for Implicit Inference in Astrophysics and Cosmology — 2402.05137 nbi: the Astronomer's Package for Neural Posterior Estimation Bayesian Computation in Astronomy: Novel methods for parallel and gradient-free inference — 2303.16134 Finding reproducible cluster partitions for the k-means algorithm Scalable hierarchical BayeSN inference: Investigating dependence of SN Ia host galaxy dust properties on stellar mass and redshift — 2401.08755
NOTE Where an arxiv-interests.md paper lands when its [Topic] names no
NOTE section above — the fallback, not a domain. Re-file from here.
Imagining the Alien: Human Projections and Cognitive Limitations — 2602.07284 Results of ten years of UCLA SETI searches with the Green Bank Telescope — 2605.05408 OmniCosmos: Transferring Particle Physics Knowledge Across the Cosmos — 2512.24422 From Extraterrestrial Microbes to Alien Intelligence: Rebalancing Astronomical Research Priorities — 2507.17790 Microlensing Signatures of Dyson Sphere-like Structures around Primordial Black Holes as Technosignatures of Extraterrestrial Advanced Civilizations — 2512.07924
NOTE postprocessing (Kelley et al. 2017a; NOTE Katz et al. 2020; Volonteri et al. 2020) find that many NOTE binaries stall and fail to merge within a Hubble time. NOTE For example, the fiducial model in Kelley et al. (2017a) NOTE sees a peak of MBHB lifetimes at a median value is 29 NOTE Gyr, with only ∼ 7 % binaries have lifetime less than 1 NOTE Gyr.
SMBH
Massive black holes in galactic nuclei: Theory and Simulations — 2304.11541
NOTE Cant remember
Massive Black Holes summary — https://arxiv.org/pdf/2304.10233.pdf
NOTE Thorough summary of black hole binarys
SMBH Binaries
Hierarchical Bayesian inference on an analytical model of the LISA massive black hole binary population — 2409.06527
NOTE Incredible Bayes Model of SMBH mergers for GW astronomy, INCLUING MERGER TIME DELAYS
Dual AGNs: Precursors of Binary Supermassive Black Hole Formation and Mergers: — 2403.17076
NOTE Shows rates of SMBHs around AGNs, implies that galaxies should have many 10^8MSun SMBHs wandering around.
Active Galactic Nuclei and Host Galaxies in COSMOS-Web. II. First Look at the Kpc-scale Dual and Offset AGN Population — 2405.14980
NOTE High rate of dual AGN in redshift 1-3 galaxies, now possible due to JWST.
Einstein vs Hawking: Black hole binaries and cosmological expansion: — 2308.15117
NOTE Cant remember
Observational Signatures of Supermassive Black Hole Binaries — 2310.16896
NOTE CONTAINS SMBHB EVOLUTION EQUATIONS
https://arxiv.org/pdf/2310.16896.pdf
NOTE RABBITS Simulations which show that SMBH binaries are driven to coalescence by central nuclear star formation
https://arxiv.org/abs/2311.01499
https://arxiv.org/abs/2311.01493
Compact object mergers: Observations of supermassive binary black holes and stellar tidal disruption events — 1502.05720
NOTE Run through of observational signatures of SMBHBs, most of which are x-ray or AGN based.
The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background — 2306.16220
NOTE The link between gravitational wave background and > 10^7MSun SMBHB's.
Premature supermassive black hole mergers in cosmological simulations of structure formation — 2504.17549
NOTE Brilliant example of how numerical effects in simulations can lead to delays on SMBH mergers which impact SWGB PTA results.
https://arxiv.org/pdf/2211.11788.pdf
Big Galaxies and Big Black Holes: The Massive Ends of the Local Stellar and Black Hole Mass Functions and the Implications for Nanohertz Gravitational Waves — 2407.14595
NOTE Examples of how to make and plot SMBH mass functions and relating them to GWB.
Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): A Mix of Singles, Lenses, and True Duals at Cosmic Noon — 2409.16363
NOTE Good overview of dual AGN and looking for them
Identifying supermassive black hole recoil in elliptical galaxies — 2410.13942
NOTE All the stuff SMBH binary recoils do to the Sersic core and galaxy around them.
SMBH Scouring
The supermassive black hole merger driven evolution of high-redshift red nuggets into present-day cored early-type galaxies — 2407.18303
NOTE Great KetJU simulation study of how scouring SMBHs can create cored galaxies and impact the galaxies around them.
Analysis
Characterization of JWST NIRCam PSFs and Implications for AGN+Host Image Decomposition: — 2304.13776
NOTE Detailed discussion of the JWST PSF and how to model it, reference for PyAutoGalaxy.
Dark Matter
THESAN-HR: Galaxies in the Epoch of Reionization in warm dark matter, fuzzy dark matter and interacting dark matter: — 2304.06742
NOTE Good description of how alternative DM models (Warm, Fuzzy, Interacting) impact high-z galaxy formation / reionization.
The shape of dark matter halos: a new fundamental cosmological invariance — 2406.15947
NOTE Could be a Cosmology motivation for COMSOSO SL+WL study
Galaxies
Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales — 2210.09320
NOTE Description of how a mass threshold surpresses stellar feedback to make BH's efficient and quency galaxie,s similar to Bower 2017
Software
Setting SAIL: Leveraging Scientist-AI-Loops for Rigorous Visualization Tools — 2603.18145
https://github.com/patrick-kidger/optimistix?tab=readme-ov-file:
NOTE LOADS of JAX githubs including lineaer solvers, BlackJAX
Eryn: A multi-purpose sampler for Bayesian inference — 2303.02164
NOTE Another cool sampler for autofit.