{
  "schemaVersion": "1.0.0",
  "note": "Papers found by arXiv API search (ids and titles returned by arXiv). Status: ingested (an id appears in data/curves provenance), queued, skipped (with reason), candidate. Regenerate from docs/literature-candidates.md with scripts/build-literature-backlog.py; edit status and statusNote here.",
  "entries": [
    {
      "arxiv": "2111.01160",
      "project": "ASTRID",
      "year": 2021,
      "firstAuthor": "Bird",
      "title": "The ASTRID Simulation: Galaxy Formation and Reionization",
      "section": "suite in sim-highline",
      "couldSupply": "overview; box, reionization models, BH dynamics",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2110.14154",
      "project": "ASTRID",
      "year": 2021,
      "firstAuthor": "Ni",
      "title": "The ASTRID simulation: the evolution of Supermassive Black Holes",
      "section": "suite in sim-highline",
      "couldSupply": "supermassive black holes; BH-galaxy relations",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for bh, uvlf; not extractable at this quality."
    },
    {
      "arxiv": "2409.10666",
      "project": "ASTRID",
      "year": 2024,
      "firstAuthor": "Ni",
      "title": "The Astrid Simulation: Evolution of black holes and galaxies to z=0.5 and different evolution pathways for gal",
      "section": "suite in sim-highline",
      "couldSupply": "extension to lower redshift (z=0.5 and beyond); check for relations at z<3",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for bh, gsmf, size, ssfr, uvlf; not extractable at this quality."
    },
    {
      "arxiv": "1504.06619",
      "project": "BlueTides",
      "year": 2015,
      "firstAuthor": "Feng",
      "title": "The BlueTides Simulation: First Galaxies and Reionization",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention sfrd, uvlf in vector figures or tables (8); not yet extracted."
    },
    {
      "arxiv": "1801.04951",
      "project": "BlueTides",
      "year": 2018,
      "firstAuthor": "Huang",
      "title": "BlueTides simulation: establishing black hole-galaxy relations at high-redshift",
      "section": "suite in sim-highline",
      "couldSupply": "BH-galaxy relations at high z (already ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1704.00954",
      "project": "BlueTides",
      "year": 2017,
      "firstAuthor": "Wilkins",
      "title": "The properties of the first galaxies in the BLUETIDES simulation",
      "section": "suite in sim-highline",
      "couldSupply": "galaxy properties of the first galaxies",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2508.21126",
      "project": "COLIBRE",
      "year": 2025,
      "firstAuthor": "Schaye",
      "title": "The COLIBRE project: cosmological hydrodynamical simulations of galaxy formation and evolution",
      "section": "suite in sim-highline",
      "couldSupply": "project overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2509.07960",
      "project": "COLIBRE",
      "year": 2025,
      "firstAuthor": "Chaikin",
      "title": "The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from red",
      "section": "suite in sim-highline",
      "couldSupply": "GSMF and SFR evolution (ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2509.25309",
      "project": "COLIBRE",
      "year": 2025,
      "firstAuthor": "Benítez-Llambay",
      "title": "Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation",
      "section": "suite in sim-highline",
      "couldSupply": "pre-supernova feedback (model paper)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2603.26200",
      "project": "COLIBRE",
      "year": 2026,
      "firstAuthor": "Ludlow",
      "title": "The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "sizes and angular momentum: would feed size and j* relations",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2607.26058",
      "project": "COLIBRE",
      "year": 2026,
      "firstAuthor": "Vijayan",
      "title": "The evolution of galaxy dust scaling relations in the COLIBRE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "dust scaling relations",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention mzr, ssfr in vector figures or tables (6); not yet extracted."
    },
    {
      "arxiv": "2609.11654",
      "project": "COLIBRE",
      "year": 2026,
      "firstAuthor": "Huppenkothen",
      "title": "The atomic multiphase interstellar medium of galaxies in the COLIBRE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "atomic multiphase ISM: HI scaling relations",
      "status": "skipped",
      "statusNote": "Figures are raster PNGs (no vector paths); no data table on the COLIBRE paper-data page."
    },
    {
      "arxiv": "2604.03503",
      "project": "COLIBRE",
      "year": 2026,
      "firstAuthor": "Moreno",
      "title": "The morphologies of present-day galaxies in the COLIBRE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "present-day morphologies",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention jstar in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "2607.27319",
      "project": "COLIBRE",
      "year": 2026,
      "firstAuthor": "Davies",
      "title": "The influence of feedback on the baryonic content of haloes in the COLIBRE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "baryonic content of haloes (feedback)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2608.19007",
      "project": "COLIBRE",
      "year": 2026,
      "firstAuthor": "Chaikin",
      "title": "The progenitors of $z\\gtrsim10$ JWST galaxies in the COLIBRE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "progenitors of z>=10 JWST galaxies",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2608.12132",
      "project": "COLIBRE",
      "year": 2026,
      "firstAuthor": "Zegveld",
      "title": "The effect of galaxy interactions on star formation rates in the COLIBRE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "galaxy interactions and SFR",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gas, sfms in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "2610.25786",
      "project": "DARWIN",
      "year": 2026,
      "firstAuthor": "Lee",
      "title": "The DARWIN Project: Cosmological Simulations of Galaxy Formation down to Dwarf Scales in Diverse Environments",
      "section": "suite in sim-highline",
      "couldSupply": "overview (ingested; five vector figures read, three raster figures not)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1407.7040",
      "project": "EAGLE",
      "year": 2014,
      "firstAuthor": "Schaye",
      "title": "The EAGLE project: Simulating the evolution and assembly of galaxies and their environments",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1501.01311",
      "project": "EAGLE",
      "year": 2015,
      "firstAuthor": "Crain",
      "title": "The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations",
      "section": "suite in sim-highline",
      "couldSupply": "calibration and model variations",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1510.01320",
      "project": "EAGLE",
      "year": 2015,
      "firstAuthor": "McAlpine",
      "title": "The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues",
      "section": "suite in sim-highline",
      "couldSupply": "public catalogue release",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention size in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1706.09899",
      "project": "EAGLE",
      "year": 2017,
      "firstAuthor": "team",
      "title": "The EAGLE simulations of galaxy formation: Public release of particle data",
      "section": "suite in sim-highline",
      "couldSupply": "public particle data release",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1509.05056",
      "project": "EAGLE",
      "year": 2015,
      "firstAuthor": "Schaller",
      "title": "The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme",
      "section": "suite in sim-highline",
      "couldSupply": "hydrodynamics scheme",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gas, sfrd, ssfr in vector figures or tables (3); not yet extracted."
    },
    {
      "arxiv": "1504.04374",
      "project": "EAGLE",
      "year": 2015,
      "firstAuthor": "Trayford",
      "title": "Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "colours and luminosities at z=0.1",
      "status": "ingested",
      "statusNote": "Scanned 2026-10-08: captions mention uvlf in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "1601.07907",
      "project": "EAGLE",
      "year": 2016,
      "firstAuthor": "Trayford",
      "title": "It's not easy being green: The evolution of galaxy colour in the EAGLE simulation",
      "section": "suite in sim-highline",
      "couldSupply": "colour evolution",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for zstar; not extractable at this quality."
    },
    {
      "arxiv": "1704.06283",
      "project": "EAGLE",
      "year": 2017,
      "firstAuthor": "Correa",
      "title": "The relation between galaxy morphology and colour in the EAGLE simulation",
      "section": "suite in sim-highline",
      "couldSupply": "morphology and colour",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1810.07335",
      "project": "EAGLE",
      "year": 2018,
      "firstAuthor": "Wright",
      "title": "Quenching timescales of galaxies in the EAGLE simulations",
      "section": "suite in sim-highline",
      "couldSupply": "quenching timescales: quenched fractions",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for gas, quenched, sfms; not extractable at this quality."
    },
    {
      "arxiv": "1806.11120",
      "project": "EAGLE",
      "year": 2018,
      "firstAuthor": "Cochrane",
      "title": "Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE",
      "section": "suite in sim-highline",
      "couldSupply": "mass and environment quenching",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention shmr in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "2203.16326",
      "project": "EAGLE",
      "year": 2022,
      "firstAuthor": "Zenocratti",
      "title": "The origin of correlations between mass, metallicity and morphology in galaxies from the EAGLE simulation",
      "section": "suite in sim-highline",
      "couldSupply": "correlations among mass, metallicity and morphology: MZR",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for gas, mzr, ssfr; not extractable at this quality."
    },
    {
      "arxiv": "1311.2073",
      "project": "FIRE",
      "year": 2013,
      "firstAuthor": "Hopkins",
      "title": "Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient St",
      "section": "suite in sim-highline",
      "couldSupply": "FIRE-1 (original)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for mzr, sfms, shmr; not extractable at this quality."
    },
    {
      "arxiv": "1702.06148",
      "project": "FIRE",
      "year": 2017,
      "firstAuthor": "Hopkins",
      "title": "FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation",
      "section": "suite in sim-highline",
      "couldSupply": "FIRE-2 (ingested via Ma+18)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention shmr in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "2203.00040",
      "project": "FIRE",
      "year": 2022,
      "firstAuthor": "Hopkins",
      "title": "FIRE-3: Updated Stellar Evolution Models, Yields, &amp; Microphysics and Fitting Functions for Applications in",
      "section": "suite in sim-highline",
      "couldSupply": "FIRE-3 physics update",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1602.05957",
      "project": "FIRE",
      "year": 2016,
      "firstAuthor": "Wetzel",
      "title": "Reconciling dwarf galaxies with LCDM cosmology: Simulating a realistic population of satellites around a Milky",
      "section": "suite in sim-highline",
      "couldSupply": "Wetzel+16 satellites of a Milky Way-mass host",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1706.06605",
      "project": "FIRE",
      "year": 2017,
      "firstAuthor": "Ma",
      "title": "Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and",
      "section": "suite in sim-highline",
      "couldSupply": "Ma+18 scaling relations at z>=5 (ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1710.00008",
      "project": "FIRE",
      "year": 2017,
      "firstAuthor": "Ma",
      "title": "Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes",
      "section": "suite in sim-highline",
      "couldSupply": "Ma+18 sizes and morphologies at high z",
      "status": "skipped",
      "statusNote": "FIRE-2 size-mass at z 6-10 is plotted in arcseconds, not physical units, and per galaxy; would need a cosmology conversion and new definitions."
    },
    {
      "arxiv": "2403.08853",
      "project": "FIRE",
      "year": 2024,
      "firstAuthor": "Marszewski",
      "title": "The High-Redshift Gas-Phase Mass-Metallicity Relation in FIRE-2",
      "section": "suite in sim-highline",
      "couldSupply": "high-z gas-phase MZR in FIRE-2",
      "status": "ingested",
      "statusNote": "FIRE-2 high-z MZR: check against ingested FIRE-2 mzr"
    },
    {
      "arxiv": "1504.02097",
      "project": "FIRE",
      "year": 2015,
      "firstAuthor": "Ma",
      "title": "The Origin and Evolution of the Galaxy Mass-Metallicity Relation",
      "section": "suite in sim-highline",
      "couldSupply": "Ma+16 MZR (used in sim-highline notes)",
      "status": "skipped",
      "statusNote": "FIRE-1 (Ma+16) simulations, not FIRE-2; the tracked FIRE-2 suite should not be mixed with them without a separate run label."
    },
    {
      "arxiv": "2205.15325",
      "project": "FIREbox",
      "year": 2022,
      "firstAuthor": "Feldmann",
      "title": "FIREbox: Simulating galaxies at high dynamic range in a cosmological volume",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2306.04024",
      "project": "FLAMINGO",
      "year": 2023,
      "firstAuthor": "Schaye",
      "title": "The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster sur",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2306.05492",
      "project": "FLAMINGO",
      "year": 2023,
      "firstAuthor": "Kugel",
      "title": "FLAMINGO: Calibrating large cosmological hydrodynamical simulations with machine learning",
      "section": "suite in sim-highline",
      "couldSupply": "ML calibration (variations ingested; ingested: best-fitting calibration runs, stellar mass function and gas fraction)",
      "status": "ingested",
      "statusNote": "Scanned 2026-10-08: captions mention gas, gsmf in vector figures or tables (8); not yet extracted."
    },
    {
      "arxiv": "2410.17109",
      "project": "FLAMINGO",
      "year": 2024,
      "firstAuthor": "Schaller",
      "title": "The FLAMINGO project: Baryon effects on the matter power spectrum",
      "section": "suite in sim-highline",
      "couldSupply": "baryon effects on the matter power spectrum",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention bhsigma, gas, gsmf in vector figures or tables (6); not yet extracted."
    },
    {
      "arxiv": "2312.08277",
      "project": "FLAMINGO",
      "year": 2023,
      "firstAuthor": "Braspenning",
      "title": "The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations",
      "section": "suite in sim-highline",
      "couldSupply": "clusters vs X-ray observations",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gas in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "2410.14773",
      "project": "FLAMINGO",
      "year": 2024,
      "firstAuthor": "Baker",
      "title": "The abundance and nature of high-redshift quiescent galaxies from JADES spectroscopy and the FLAMINGO simulati",
      "section": "suite in sim-highline",
      "couldSupply": "high-z quiescent galaxies vs JADES: quenched fractions and GSMF at z>2",
      "status": "skipped",
      "statusNote": "Its simulation content is the comoving number density of massive quiescent galaxies versus redshift, a quantity sim-highline has no relation for; add one (like sfrd) before extracting."
    },
    {
      "arxiv": "2510.17980",
      "project": "FLAMINGO",
      "year": 2025,
      "firstAuthor": "Costello",
      "title": "FLAMINGO: Tracing the co-evolution of hot gas and black holes in galaxy groups and clusters",
      "section": "suite in sim-highline",
      "couldSupply": "hot gas and black holes in groups and clusters",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gas in vector figures or tables (4); not yet extracted."
    },
    {
      "arxiv": "2004.07283",
      "project": "FLARES",
      "year": 2020,
      "firstAuthor": "Lovell",
      "title": "First Light And Reionisation Epoch Simulations (FLARES) I: Environmental Dependence of High-Redshift Galaxy Ev",
      "section": "suite in sim-highline",
      "couldSupply": "FLARES I (overview, environment dependence)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gsmf in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "2008.06057",
      "project": "FLARES",
      "year": 2020,
      "firstAuthor": "Vijayan",
      "title": "First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxi",
      "section": "suite in sim-highline",
      "couldSupply": "FLARES II (photometric properties)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2108.00830",
      "project": "FLARES",
      "year": 2021,
      "firstAuthor": "Vijayan",
      "title": "First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmi",
      "section": "suite in sim-highline",
      "couldSupply": "FLARES III (massive dusty galaxies)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention sfms, ssfr, uvlf in vector figures or tables (8); not yet extracted."
    },
    {
      "arxiv": "2211.07540",
      "project": "FLARES",
      "year": 2022,
      "firstAuthor": "Lovell",
      "title": "First Light And Reionisation Epoch Simulations (FLARES) VIII. The Emergence of Passive Galaxies at $z \\geqslan",
      "section": "suite in sim-highline",
      "couldSupply": "FLARES VIII (passive galaxies)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention sfms, size in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "2204.09431",
      "project": "FLARES",
      "year": 2022,
      "firstAuthor": "Wilkins",
      "title": "First Light And Reionisation Epoch Simulations (FLARES) V: The redshift frontier",
      "section": "suite in sim-highline",
      "couldSupply": "FLARES V (redshift frontier)",
      "status": "ingested",
      "statusNote": "FLARES V: check for UV luminosity function figure"
    },
    {
      "arxiv": "2301.05228",
      "project": "FLARES",
      "year": 2023,
      "firstAuthor": "Roper",
      "title": "FLARES IX: The Physical Mechanisms Driving Compact Galaxy Formation and Evolution",
      "section": "suite in sim-highline",
      "couldSupply": "FLARES IX (compact galaxies: sizes)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for size, ssfr; not extractable at this quality."
    },
    {
      "arxiv": "1402.1165",
      "project": "Horizon-AGN",
      "year": 2014,
      "firstAuthor": "Dubois",
      "title": "Dancing in the dark: galactic properties trace spin swings along the cosmic web",
      "section": "suite in sim-highline",
      "couldSupply": "overview (spin alignment)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for jstar, sfms; not extractable at this quality."
    },
    {
      "arxiv": "1605.09379",
      "project": "Horizon-AGN",
      "year": 2016,
      "firstAuthor": "Kaviraj",
      "title": "The Horizon-AGN simulation: evolution of galaxy properties over cosmic time",
      "section": "suite in sim-highline",
      "couldSupply": "galaxy properties over cosmic time (ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1602.01941",
      "project": "Horizon-AGN",
      "year": 2016,
      "firstAuthor": "Volonteri",
      "title": "The cosmic evolution of massive black holes in the Horizon-AGN simulation",
      "section": "suite in sim-highline",
      "couldSupply": "Volonteri+16 black holes (ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1606.03086",
      "project": "Horizon-AGN",
      "year": 2016,
      "firstAuthor": "Dubois",
      "title": "The Horizon-AGN simulation: morphological diversity of galaxies promoted by AGN feedback",
      "section": "suite in sim-highline",
      "couldSupply": "Dubois+16 morphological diversity",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2005.04902",
      "project": "Horizon-AGN",
      "year": 2020,
      "firstAuthor": "Volonteri",
      "title": "Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations",
      "section": "suite in sim-highline",
      "couldSupply": "BH mergers, NewHorizon and Horizon-AGN",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1405.2921",
      "project": "Illustris",
      "year": 2014,
      "firstAuthor": "Vogelsberger",
      "title": "Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1405.3749",
      "project": "Illustris",
      "year": 2014,
      "firstAuthor": "Genel",
      "title": "Introducing the Illustris Project: the evolution of galaxy populations across cosmic time",
      "section": "suite in sim-highline",
      "couldSupply": "galaxy populations across cosmic time",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1405.1418",
      "project": "Illustris",
      "year": 2014,
      "firstAuthor": "Vogelsberger",
      "title": "Properties of galaxies reproduced by a hydrodynamic simulation",
      "section": "suite in sim-highline",
      "couldSupply": "Nature paper",
      "status": "candidate",
      "statusNote": "Scan failed (source could not be fetched); not triaged."
    },
    {
      "arxiv": "1408.6842",
      "project": "Illustris",
      "year": 2014,
      "firstAuthor": "Sijacki",
      "title": "The Illustris simulation: the evolving population of black holes across cosmic time",
      "section": "suite in sim-highline",
      "couldSupply": "Sijacki+15 black holes: BH mass function, BH-galaxy relations",
      "status": "skipped",
      "statusNote": "Examined 2026-10-14: the black-hole mass function, SFR and BH accretion densities are vector figures, but the M_BH-sigma and M_BH-M_bulge relations are raster 2D histograms, and the fit table (slope and normalisation at z=0-4 for sigma_1D, z=0-1 for sigma_eff) states no sigma range, so no domain can be set honestly for a fit record."
    },
    {
      "arxiv": "1703.02970",
      "project": "IllustrisTNG",
      "year": 2017,
      "firstAuthor": "Pillepich",
      "title": "Simulating Galaxy Formation with the IllustrisTNG Model",
      "section": "suite in sim-highline",
      "couldSupply": "model description",
      "status": "ingested",
      "statusNote": "Scanned 2026-10-08: captions mention gsmf, size in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "1607.03486",
      "project": "IllustrisTNG",
      "year": 2016,
      "firstAuthor": "Weinberger",
      "title": "Simulating galaxy formation with black hole driven thermal and kinetic feedback",
      "section": "suite in sim-highline",
      "couldSupply": "black-hole feedback model",
      "status": "skipped",
      "statusNote": "SFRD figure is for the test boxes of the model-development paper; the volume is not stated in the caption, so it cannot be labelled as TNG100 without checking the paper body."
    },
    {
      "arxiv": "1710.04659",
      "project": "IllustrisTNG",
      "year": 2017,
      "firstAuthor": "Weinberger",
      "title": "Supermassive black holes and their feedback effects in the IllustrisTNG simulation",
      "section": "suite in sim-highline",
      "couldSupply": "Weinberger+18 black holes and feedback: BH-galaxy relations",
      "status": "skipped",
      "statusNote": "No figure fits an existing relation (quasar luminosity function, feedback rates, merger rates, Eddington ratios); would need new black-hole relations."
    },
    {
      "arxiv": "1707.03395",
      "project": "IllustrisTNG",
      "year": 2017,
      "firstAuthor": "Nelson",
      "title": "First results from the IllustrisTNG simulations: the galaxy color bimodality",
      "section": "suite in sim-highline",
      "couldSupply": "colour bimodality",
      "status": "ingested",
      "statusNote": "Scanned 2026-10-08: captions mention zstar in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1707.03397",
      "project": "IllustrisTNG",
      "year": 2017,
      "firstAuthor": "Springel",
      "title": "First results from the IllustrisTNG simulations: matter and galaxy clustering",
      "section": "suite in sim-highline",
      "couldSupply": "clustering",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1707.03396",
      "project": "IllustrisTNG",
      "year": 2017,
      "firstAuthor": "Marinacci",
      "title": "First results from the IllustrisTNG simulations: radio haloes and magnetic fields",
      "section": "suite in sim-highline",
      "couldSupply": "magnetic fields",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1707.03401",
      "project": "IllustrisTNG",
      "year": 2017,
      "firstAuthor": "Naiman",
      "title": "First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and",
      "section": "suite in sim-highline",
      "couldSupply": "chemical enrichment",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1812.05609",
      "project": "IllustrisTNG",
      "year": 2018,
      "firstAuthor": "Nelson",
      "title": "The IllustrisTNG Simulations: Public Data Release",
      "section": "suite in sim-highline",
      "couldSupply": "public data release",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention mzr, smd in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1902.05553",
      "project": "IllustrisTNG",
      "year": 2019,
      "firstAuthor": "Pillepich",
      "title": "First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time",
      "section": "suite in sim-highline",
      "couldSupply": "TNG50 discs",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1902.05554",
      "project": "IllustrisTNG",
      "year": 2019,
      "firstAuthor": "Nelson",
      "title": "First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback",
      "section": "suite in sim-highline",
      "couldSupply": "TNG50 outflows",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention sfms, size in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "1707.05327",
      "project": "IllustrisTNG",
      "year": 2017,
      "firstAuthor": "Genel",
      "title": "The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation",
      "section": "suite in sim-highline",
      "couldSupply": "sizes (used in sim-highline notes; figures not yet extracted)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1711.05261",
      "project": "IllustrisTNG",
      "year": 2017,
      "firstAuthor": "Torrey",
      "title": "The evolution of the mass-metallicity relation in IllustrisTNG",
      "section": "suite in sim-highline",
      "couldSupply": "MZR (used in notes; figures not yet extracted)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1906.02747",
      "project": "IllustrisTNG",
      "year": 2019,
      "firstAuthor": "Terrazas",
      "title": "The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG",
      "section": "suite in sim-highline",
      "couldSupply": "BH mass vs galaxy properties",
      "status": "skipped",
      "statusNote": "TNG black hole feedback paper: M_BH-M_star only (already covered by Habouzit+21), no M_BH-sigma."
    },
    {
      "arxiv": "2203.10098",
      "project": "IllustrisTNG",
      "year": 2022,
      "firstAuthor": "Rodriguez-Gomez",
      "title": "Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black ",
      "section": "suite in sim-highline",
      "couldSupply": "Rodriguez-Gomez+22 galactic angular momentum: j*-M*",
      "status": "ingested",
      "statusNote": "j* in TNG: fills jstar"
    },
    {
      "arxiv": "2307.02722",
      "project": "IllustrisTNG",
      "year": 2023,
      "firstAuthor": "Hardwick",
      "title": "Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG",
      "section": "suite in sim-highline",
      "couldSupply": "angular momentum and atomic gas, EAGLE and TNG",
      "status": "skipped",
      "statusNote": "HI fraction versus stellar mass for EAGLE and TNG with an xGASS-like selection; adds another selection definition to relations already covered by Dave+20, Crain+17 and Diemer+19, so left for later."
    },
    {
      "arxiv": "2007.10993",
      "project": "IllustrisTNG",
      "year": 2020,
      "firstAuthor": "Hemler",
      "title": "Gas-phase metallicity gradients of TNG50 star-forming galaxies",
      "section": "suite in sim-highline",
      "couldSupply": "TNG50 metallicity gradients",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention mzr in vector figures or tables (6); not yet extracted."
    },
    {
      "arxiv": "2311.06338",
      "project": "IllustrisTNG",
      "year": 2023,
      "firstAuthor": "Nelson",
      "title": "Introducing the TNG-Cluster Simulation: overview and physical properties of the gaseous intracluster medium",
      "section": "suite in sim-highline",
      "couldSupply": "TNG-Cluster overview",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gas in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "2504.01061",
      "project": "Magneticum",
      "year": 2025,
      "firstAuthor": "Dolag",
      "title": "Encyclopedia Magneticum: Scaling Relations from Cosmic Dawn to Present Day",
      "section": "suite in sim-highline",
      "couldSupply": "Encyclopedia Magneticum (28 relations; box-labelled tables already ingested for eight of them)",
      "status": "skipped",
      "statusNote": "The SFR density figure colours curves by resolution class and two boxes share the 'hr' colour (and two share 'uhr'), so a curve cannot be attributed to one named box; the other figures duplicate the released Magneticum tables."
    },
    {
      "arxiv": "1503.03501",
      "project": "Magneticum",
      "year": 2015,
      "firstAuthor": "Teklu",
      "title": "Connecting Angular Momentum and Galactic Dynamics: The complex Interplay between Spin, Mass, and Morphology",
      "section": "suite in sim-highline",
      "couldSupply": "Teklu+15 angular momentum and morphology",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for gas, jstar; not extractable at this quality."
    },
    {
      "arxiv": "1709.02393",
      "project": "Magneticum",
      "year": 2017,
      "firstAuthor": "Remus",
      "title": "The Outer Halos of Very Massive Galaxies: BCGs and their DSC in the Magneticum Simulations",
      "section": "suite in sim-highline",
      "couldSupply": "BCGs and diffuse stellar component",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1708.00027",
      "project": "Magneticum",
      "year": 2017,
      "firstAuthor": "Dolag",
      "title": "Distribution and Evolution of Metals in the Magneticum simulations",
      "section": "suite in sim-highline",
      "couldSupply": "metals in Magneticum",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for mzr, zstar; not extractable at this quality."
    },
    {
      "arxiv": "2011.06602",
      "project": "Magneticum",
      "year": 2020,
      "firstAuthor": "Lotz",
      "title": "Rise and fall of post-starburst galaxies in Magneticum Pathfinder",
      "section": "suite in sim-highline",
      "couldSupply": "post-starburst galaxies",
      "status": "skipped",
      "statusNote": "Quenched fraction is plotted against halo mass in stellar-mass bins for massive galaxies, not against stellar mass like the quenched-fraction relation here; the Magneticum quenched relation would need that new x axis."
    },
    {
      "arxiv": "2009.10578",
      "project": "NewHorizon",
      "year": 2020,
      "firstAuthor": "Dubois",
      "title": "Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time",
      "section": "suite in sim-highline",
      "couldSupply": "overview (ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1503.04818",
      "project": "NIHAO",
      "year": 2015,
      "firstAuthor": "Wang",
      "title": "NIHAO project I: Reproducing the inefficiency of galaxy formation across cosmic time with a large sample of co",
      "section": "suite in sim-highline",
      "couldSupply": "NIHAO I overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1506.08785",
      "project": "NIHAO",
      "year": 2015,
      "firstAuthor": "Stinson",
      "title": "NIHAO III: The constant disc gas mass conspiracy",
      "section": "suite in sim-highline",
      "couldSupply": "III: constant disc gas mass",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1607.01028",
      "project": "NIHAO",
      "year": 2016,
      "firstAuthor": "Macciò",
      "title": "NIHAO X: Reconciling the local galaxy velocity function with Cold Dark Matter via mock HI observations",
      "section": "suite in sim-highline",
      "couldSupply": "X: mock HI, velocity function",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1610.06375",
      "project": "NIHAO",
      "year": 2016,
      "firstAuthor": "Dutton",
      "title": "NIHAO XII: galactic uniformity in a ΛCDM universe",
      "section": "suite in sim-highline",
      "couldSupply": "XII: scaling relations incl. Tully-Fisher (ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1706.04202",
      "project": "NIHAO",
      "year": 2017,
      "firstAuthor": "Santos-Santos",
      "title": "NIHAO XIV: Reproducing the observed diversity of dwarf galaxy rotation curve shapes in LCDM",
      "section": "suite in sim-highline",
      "couldSupply": "XIV: rotation curve diversity",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention bhsigma in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1807.10518",
      "project": "NIHAO",
      "year": 2018,
      "firstAuthor": "Dutton",
      "title": "NIHAO XVII: The diversity of dwarf galaxy kinematics and implications for the HI velocity function",
      "section": "suite in sim-highline",
      "couldSupply": "XVII: HI velocity function",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1902.06751",
      "project": "NIHAO",
      "year": 2019,
      "firstAuthor": "Dutton",
      "title": "NIHAO XVIII: Origin of the MOND phenomenology of galactic rotation curves in a LCDM universe",
      "section": "suite in sim-highline",
      "couldSupply": "XVIII: MOND phenomenology and radial acceleration relation",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for size; not extractable at this quality."
    },
    {
      "arxiv": "1906.06955",
      "project": "NIHAO",
      "year": 2019,
      "firstAuthor": "Blank",
      "title": "NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite",
      "section": "suite in sim-highline",
      "couldSupply": "XXII: black holes (ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2204.11579",
      "project": "NIHAO",
      "year": 2022,
      "firstAuthor": "Blank",
      "title": "NIHAO XXVII: Crossing the green valley",
      "section": "suite in sim-highline",
      "couldSupply": "XXVII: green valley",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for zstar; not extractable at this quality."
    },
    {
      "arxiv": "1909.05864",
      "project": "NIHAO",
      "year": 2019,
      "firstAuthor": "Buck",
      "title": "NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations",
      "section": "suite in sim-highline",
      "couldSupply": "NIHAO-UHD",
      "status": "ingested",
      "statusNote": "Extracted 2026-10-14: left-panel stellar Tully-Fisher points of the five galaxies (circular velocity at 2.2 R_d and HI line-width velocity). The right panel (flat velocity at the HI radius against SPARC) is not extracted."
    },
    {
      "arxiv": "1607.02151",
      "project": "Romulus25",
      "year": 2016,
      "firstAuthor": "Tremmel",
      "title": "The Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of S",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1904.10116",
      "project": "Romulus25",
      "year": 2019,
      "firstAuthor": "Ricarte",
      "title": "Tracing Black Hole and Galaxy Co-evolution in the Romulus Simulations",
      "section": "suite in sim-highline",
      "couldSupply": "Ricarte+19 BH-galaxy co-evolution (ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2203.00016",
      "project": "Romulus25",
      "year": 2022,
      "firstAuthor": "Jung",
      "title": "Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0",
      "section": "suite in sim-highline",
      "couldSupply": "massive central galaxies of groups",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention bhsigma, sfms, shmr in vector figures or tables (5); not yet extracted."
    },
    {
      "arxiv": "1901.10203",
      "project": "SIMBA",
      "year": 2019,
      "firstAuthor": "Davé",
      "title": "Simba: Cosmological Simulations with Black Hole Growth and Feedback",
      "section": "suite in sim-highline",
      "couldSupply": "overview (GSMF ingested)",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1604.01418",
      "project": "SIMBA",
      "year": 2016,
      "firstAuthor": "Davé",
      "title": "MUFASA: Galaxy Formation Simulations With Meshless Hydrodynamics",
      "section": "suite in sim-highline",
      "couldSupply": "MUFASA predecessor",
      "status": "skipped",
      "statusNote": "MUFASA is the predecessor of SIMBA with a different model; its curves are not SIMBA's."
    },
    {
      "arxiv": "2003.03402",
      "project": "SIMBA",
      "year": 2020,
      "firstAuthor": "Glowacki",
      "title": "The baryonic Tully-Fisher relation in the Simba simulation",
      "section": "suite in sim-highline",
      "couldSupply": "BTFR in Simba",
      "status": "ingested",
      "statusNote": "BTFR in SIMBA: fills btfr"
    },
    {
      "arxiv": "2011.08866",
      "project": "SIMBA",
      "year": 2020,
      "firstAuthor": "Glowacki",
      "title": "The redshift evolution of the baryonic Tully-Fisher relation in Simba",
      "section": "suite in sim-highline",
      "couldSupply": "BTFR evolution to z~2 (fit parameters per redshift): fills btfr epochs",
      "status": "skipped",
      "statusNote": "The fit table (V_flat, W50/2, W20/2 at z 0-1) gives no velocity range for the fits, so a domain cannot be set without reading it from the figure; extract the dashed fit lines from the figure to add it."
    },
    {
      "arxiv": "2002.07226",
      "project": "SIMBA",
      "year": 2020,
      "firstAuthor": "Davé",
      "title": "Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations",
      "section": "suite in sim-highline",
      "couldSupply": "cold gas contents in EAGLE, TNG and Simba (multi-simulation HI and H2 fractions)",
      "status": "ingested",
      "statusNote": "cold gas fractions in EAGLE, TNG and SIMBA: fills gas/hi-fraction/h2-fraction"
    },
    {
      "arxiv": "2512.04582",
      "project": "SIMBA",
      "year": 2025,
      "firstAuthor": "Rabyang",
      "title": "Investigating the H i mass-size relation using the Simba cosmological simulations",
      "section": "suite in sim-highline",
      "couldSupply": "HI mass-size relation in Simba",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for size; not extractable at this quality."
    },
    {
      "arxiv": "2308.03436",
      "project": "SIMBA",
      "year": 2023,
      "firstAuthor": "Hough",
      "title": "SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation",
      "section": "suite in sim-highline",
      "couldSupply": "Simba-C chemical enrichment",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for gsmf, mzr, sfms; not extractable at this quality."
    },
    {
      "arxiv": "2105.12748",
      "project": "SIMBA",
      "year": 2021,
      "firstAuthor": "Akins",
      "title": "Quenching and the UVJ diagram in the SIMBA cosmological simulation",
      "section": "suite in sim-highline",
      "couldSupply": "quenching and UVJ diagram",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention sfms in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "1801.07259",
      "project": "SPHINX",
      "year": 2018,
      "firstAuthor": "Rosdahl",
      "title": "The SPHINX Cosmological Simulations of the First Billion Years: the Impact of Binary Stars on Reionization",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2101.11624",
      "project": "SPHINX",
      "year": 2021,
      "firstAuthor": "Katz",
      "title": "Introducing SPHINX-MHD: The Impact of Primordial Magnetic Fields on the First Galaxies, Reionization, and the ",
      "section": "suite in sim-highline",
      "couldSupply": "SPHINX-MHD",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for bhsigma, sfrd, shmr, size, uvlf, zstar; not extractable at this quality."
    },
    {
      "arxiv": "2309.03269",
      "project": "SPHINX",
      "year": 2023,
      "firstAuthor": "Katz",
      "title": "The Sphinx Public Data Release: Forward Modelling High-Redshift JWST Observations with Cosmological Radiation ",
      "section": "suite in sim-highline",
      "couldSupply": "public data release for JWST forward modelling",
      "status": "ingested",
      "statusNote": "UV luminosity function extracted. Not extracted: the SFR density (progenitors of a galaxy selection at several snapshots, not a volume-wide SFR density)."
    },
    {
      "arxiv": "2207.03232",
      "project": "SPHINX",
      "year": 2022,
      "firstAuthor": "Rosdahl",
      "title": "LyC escape from SPHINX galaxies in the Epoch of Reionization",
      "section": "suite in sim-highline",
      "couldSupply": "LyC escape",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2110.00584",
      "project": "THESAN",
      "year": 2021,
      "firstAuthor": "Kannan",
      "title": "Introducing the THESAN project: radiation-magnetohydrodynamic simulations of the epoch of reionization",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2110.01628",
      "project": "THESAN",
      "year": 2021,
      "firstAuthor": "Garaldi",
      "title": "The THESAN project: properties of the intergalactic medium and its connection to Reionization-era galaxies",
      "section": "suite in sim-highline",
      "couldSupply": "IGM properties",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gsmf, sfrd, shmr in vector figures or tables (3); not yet extracted."
    },
    {
      "arxiv": "2110.02966",
      "project": "THESAN",
      "year": 2021,
      "firstAuthor": "Smith",
      "title": "The THESAN project: Lyman-alpha emission and transmission during the Epoch of Reionization",
      "section": "suite in sim-highline",
      "couldSupply": "Lyman-alpha",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gsmf, uvlf in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "2309.06475",
      "project": "THESAN",
      "year": 2023,
      "firstAuthor": "Garaldi",
      "title": "The thesan project: public data release of radiation-hydrodynamic simulations matching reionization-era JWST o",
      "section": "suite in sim-highline",
      "couldSupply": "public data release",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention mzr, sfms, sfrd in vector figures or tables (4); not yet extracted."
    },
    {
      "arxiv": "2402.08717",
      "project": "THESAN",
      "year": 2024,
      "firstAuthor": "Shen",
      "title": "The THESAN project: galaxy sizes during the epoch of reionization",
      "section": "suite in sim-highline",
      "couldSupply": "Shen+24 galaxy sizes in the epoch of reionization: high-z size relation",
      "status": "skipped",
      "statusNote": "All size-mass figures are raster PNGs (no vector paths); needs tables from the authors."
    },
    {
      "arxiv": "2502.20437",
      "project": "THESAN-zoom",
      "year": 2025,
      "firstAuthor": "Kannan",
      "title": "Introducing the THESAN-ZOOM project: radiation-hydrodynamic simulations of high-redshift galaxies with a multi",
      "section": "suite in sim-highline",
      "couldSupply": "overview",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "2503.01949",
      "project": "THESAN-zoom",
      "year": 2025,
      "firstAuthor": "Shen",
      "title": "The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies",
      "section": "suite in sim-highline",
      "couldSupply": "star-formation efficiencies at high z",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention h2, uvlf in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "2503.02927",
      "project": "THESAN-zoom",
      "year": 2025,
      "firstAuthor": "Zier",
      "title": "The THESAN-ZOOM project: Long-term imprints of external reionization on galaxy evolution",
      "section": "suite in sim-highline",
      "couldSupply": "external reionization imprints",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention size, zstar in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "1602.02155",
      "project": "APOSTLE-EAGLE",
      "year": 2016,
      "firstAuthor": "Sales",
      "title": "The low-mass end of the baryonic Tully-Fisher relation",
      "section": "suite in sim-highline",
      "couldSupply": "BTFR fit parameters (V_max, V_out), APOSTLE and EAGLE galaxies",
      "status": "ingested",
      "statusNote": ""
    },
    {
      "arxiv": "1607.03100",
      "project": "EAGLE",
      "year": 2016,
      "firstAuthor": "Ferrero",
      "title": "Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE",
      "section": "suite in sim-highline",
      "couldSupply": "stellar Tully-Fisher fit parameters z 0-1",
      "status": "skipped",
      "statusNote": "Table of EAGLE stellar TF fit parameters at z 0, 0.25, 0.75, 1 (M0, alpha, gamma), but the fit range is not stated and the figures are raster; extract with a domain from the authors."
    },
    {
      "arxiv": "1905.02741",
      "project": "SIMBA",
      "year": 2019,
      "firstAuthor": "Thomas",
      "title": "Black Hole -- Galaxy Correlations in Simba",
      "section": "suite in sim-highline",
      "couldSupply": "M_BH-sigma and M_BH-M* fits at z=0",
      "status": "skipped",
      "statusNote": "Text quotes SIMBA M_BH-sigma (alpha 8.472, beta 4.45) and M_BH-M* fits, but the figures are raster and no fit range is stated, so a domain cannot be set honestly."
    },
    {
      "arxiv": "2302.05029",
      "project": "IllustrisTNG",
      "year": 2023,
      "firstAuthor": "Deeley",
      "title": "A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG",
      "section": "suite in sim-highline",
      "couldSupply": "BTFR fits (mock-observed)",
      "status": "skipped",
      "statusNote": "BTFR fits of mock-observed TNG and MaNGA; figures are raster and fit ranges are not stated in the text read."
    },
    {
      "arxiv": "2403.09186",
      "project": "TangoSIDM",
      "year": 2024,
      "firstAuthor": "Correa",
      "title": "TangoSIDM Project: Is the Stellar Mass Tully-Fisher relation consistent with SIDM?",
      "section": "suite in sim-highline",
      "couldSupply": "stellar Tully-Fisher medians for SIDM variants",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for bhsigma, gsmf, shmr, size, tf; not extractable at this quality."
    },
    {
      "arxiv": "1511.01098",
      "project": "APOSTLE",
      "year": 2015,
      "firstAuthor": "Sawala",
      "title": "The APOSTLE simulations: solutions to the Local Group's cosmic puzzles",
      "section": "suite not in sim-highline",
      "couldSupply": "Local Group analogues; dwarf-galaxy relations (SHMR, HI, TF) to check",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for gsmf; not extractable at this quality."
    },
    {
      "arxiv": "1507.03643",
      "project": "APOSTLE",
      "year": 2015,
      "firstAuthor": "Fattahi",
      "title": "The APOSTLE project: Local Group kinematic mass constraints and simulation candidate selection",
      "section": "suite not in sim-highline",
      "couldSupply": "selection of simulation candidates",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2408.09784",
      "project": "APOSTLE-Auriga",
      "year": 2024,
      "firstAuthor": "Yang",
      "title": "Apostle--Auriga: Effects of stellar feedback subgrid models on the evolution of angular momentum in disc galax",
      "section": "suite not in sim-highline",
      "couldSupply": "angular momentum evolution, two feedback models",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention jstar in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "1610.01159",
      "project": "Auriga",
      "year": 2016,
      "firstAuthor": "Grand",
      "title": "The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time",
      "section": "suite not in sim-highline",
      "couldSupply": "disc galaxies of Milky Way mass: sizes, SFH, j*, MZR to check",
      "status": "skipped",
      "statusNote": "Auriga is not a tracked suite; adding it needs a simulation profile (code, resolution, team) as well as the baryonic Tully-Fisher points."
    },
    {
      "arxiv": "2004.01914",
      "project": "ARTEMIS",
      "year": 2020,
      "firstAuthor": "Font",
      "title": "The ARTEMIS simulations: stellar haloes of Milky Way-mass galaxies",
      "section": "suite not in sim-highline",
      "couldSupply": "stellar haloes of Milky Way-mass galaxies",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for mzr, smd, zstar; not extractable at this quality."
    },
    {
      "arxiv": "2008.04926",
      "project": "HESTIA",
      "year": 2020,
      "firstAuthor": "Libeskind",
      "title": "The Hestia project: simulations of the Local Group",
      "section": "suite not in sim-highline",
      "couldSupply": "Local Group constrained simulations",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gsmf, size, uvlf in vector figures or tables (3); not yet extracted."
    },
    {
      "arxiv": "1809.04622",
      "project": "The Three Hundred",
      "year": 2018,
      "firstAuthor": "Cui",
      "title": "The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and as",
      "section": "suite not in sim-highline",
      "couldSupply": "cluster regions: group and cluster relations (ingested; gas fraction inside R500 and the Y500-M500 relation with its fits)",
      "status": "ingested",
      "statusNote": "Scanned 2026-10-08: captions mention gas, gsmf, shmr in vector figures or tables (3); not yet extracted."
    },
    {
      "arxiv": "1703.10610",
      "project": "Hydrangea",
      "year": 2017,
      "firstAuthor": "Bahé",
      "title": "The Hydrangea simulations: galaxy formation in and around massive clusters",
      "section": "suite not in sim-highline",
      "couldSupply": "clusters with EAGLE physics: cluster-galaxy relations",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gsmf in vector figures or tables (3); not yet extracted."
    },
    {
      "arxiv": "1603.02702",
      "project": "BAHAMAS",
      "year": 2016,
      "firstAuthor": "McCarthy",
      "title": "The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology",
      "section": "suite not in sim-highline",
      "couldSupply": "calibrated to GSMF and gas fractions; large volumes",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for bhsigma, gsmf, sfrd, smd, uvlf; not extractable at this quality."
    },
    {
      "arxiv": "1607.04569",
      "project": "MACSIS",
      "year": 2016,
      "firstAuthor": "Barnes",
      "title": "The redshift evolution of massive galaxy clusters in the MACSIS simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "massive clusters",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "0909.5196",
      "project": "OWLS",
      "year": 2009,
      "firstAuthor": "Schaye",
      "title": "The physics driving the cosmic star formation history",
      "section": "suite not in sim-highline",
      "couldSupply": "cosmic SFR history; OWLS suite",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for sfrd; not extractable at this quality."
    },
    {
      "arxiv": "2010.00619",
      "project": "CAMELS",
      "year": 2020,
      "firstAuthor": "Villaescusa-Navarro",
      "title": "The CAMELS project: Cosmology and Astrophysics with MachinE Learning Simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "thousands of small boxes, four codes (TNG, Simba, ASTRID, Magneticum variants): envelopes of relations",
      "status": "ingested",
      "statusNote": "Scanned 2026-10-08: captions mention bhsigma, sfrd in vector figures or tables (7); not yet extracted."
    },
    {
      "arxiv": "2304.02096",
      "project": "CAMELS",
      "year": 2023,
      "firstAuthor": "Ni",
      "title": "The CAMELS project: Expanding the galaxy formation model space with new ASTRID and 28-parameter TNG and SIMBA ",
      "section": "suite not in sim-highline",
      "couldSupply": "CAMELS expansion with ASTRID and 28-parameter models",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for gsmf, sfms, sfrd; not extractable at this quality."
    },
    {
      "arxiv": "2109.10915",
      "project": "CAMELS",
      "year": 2021,
      "firstAuthor": "Villaescusa-Navarro",
      "title": "The CAMELS Multifield Dataset: Learning the Universe's Fundamental Parameters with Artificial Intelligence",
      "section": "suite not in sim-highline",
      "couldSupply": "multifield dataset",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2408.07258",
      "project": "Horizon Run 5",
      "year": 2024,
      "firstAuthor": "Lee",
      "title": "Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5",
      "section": "suite not in sim-highline",
      "couldSupply": "cluster and group star formation at z~1 (only a first hit; check the overview paper)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2002.04045",
      "project": "Obelisk",
      "year": 2020,
      "firstAuthor": "Trebitsch",
      "title": "The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters",
      "section": "suite not in sim-highline",
      "couldSupply": "protocluster simulation",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gsmf, sfrd, shmr, uvlf in vector figures or tables (4); not yet extracted."
    },
    {
      "arxiv": "2408.12854",
      "project": "Obelisk",
      "year": 2024,
      "firstAuthor": "Volonteri",
      "title": "Exploring Active Galactic Nuclei and Little Red Dots with the Obelisk simulation",
      "section": "suite not in sim-highline",
      "couldSupply": "AGN and little red dots",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention size, uvlf in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "2402.17635",
      "project": "Obelisk",
      "year": 2024,
      "firstAuthor": "Giovinazzo",
      "title": "Modelling LAEs in the Epoch of Reionization with OBELISK",
      "section": "suite not in sim-highline",
      "couldSupply": "LAEs in reionization",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1402.0888",
      "project": "MassiveBlack-II",
      "year": 2014,
      "firstAuthor": "Khandai",
      "title": "The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0",
      "section": "suite not in sim-highline",
      "couldSupply": "MassiveBlack-II overview (precursor of BlueTides and ASTRID)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for sfrd, uvlf; not extractable at this quality."
    },
    {
      "arxiv": "2006.13951",
      "project": "Dianoga",
      "year": 2020,
      "firstAuthor": "Bassini",
      "title": "The DIANOGA simulations of galaxy clusters: characterizing star formation in proto-clusters",
      "section": "suite not in sim-highline",
      "couldSupply": "proto-clusters",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gas, sfms, sfrd in vector figures or tables (8); not yet extracted."
    },
    {
      "arxiv": "2108.09670",
      "project": "Dianoga",
      "year": 2021,
      "firstAuthor": "Planelles",
      "title": "Exploring the role of cosmological shock waves in the Dianoga simulations of galaxy clusters",
      "section": "suite not in sim-highline",
      "couldSupply": "shock waves in clusters",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2102.12343",
      "project": "FirstLight",
      "year": 2021,
      "firstAuthor": "Ceverino",
      "title": "FirstLight IV: Diversity in sub-L$_*$ galaxies at cosmic dawn",
      "section": "suite not in sim-highline",
      "couldSupply": "FirstLight IV (sub-L* galaxies at cosmic dawn)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention sfms, size, ssfr in vector figures or tables (3); not yet extracted."
    },
    {
      "arxiv": "1910.11729",
      "project": "FirstLight",
      "year": 2019,
      "firstAuthor": "Langan",
      "title": "Weak Evolution of the Mass-metallicity Relation at Cosmic Dawn in the FirstLight Simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "mass-metallicity relation at cosmic dawn: MZR at z>5",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for gas; not extractable at this quality."
    },
    {
      "arxiv": "2404.02537",
      "project": "FirstLight",
      "year": 2024,
      "firstAuthor": "Ceverino",
      "title": "Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "galaxy formation efficiency at z=5-13: SHMR at high z",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention shmr, smd, uvlf in vector figures or tables (4); not yet extracted."
    },
    {
      "arxiv": "2210.15372",
      "project": "VELA",
      "year": 2022,
      "firstAuthor": "Ceverino",
      "title": "Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction",
      "section": "suite not in sim-highline",
      "couldSupply": "feedback effects in VELA",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention gas, size in vector figures or tables (2); not yet extracted."
    },
    {
      "arxiv": "1503.01110",
      "project": "Renaissance",
      "year": 2015,
      "firstAuthor": "O'Shea",
      "title": "Probing The Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "UV luminosity function of the earliest galaxies",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention uvlf in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1701.02749",
      "project": "Renaissance",
      "year": 2017,
      "firstAuthor": "Barrow",
      "title": "First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "spectra of high-z galaxies",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention ssfr in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1804.06477",
      "project": "Renaissance",
      "year": 2018,
      "firstAuthor": "Smith",
      "title": "The Growth of Black Holes from Population III Remnants in the Renaissance Simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "Pop III black-hole growth",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention bh in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1511.00011",
      "project": "CoDa",
      "year": 2015,
      "firstAuthor": "Ocvirk",
      "title": "Cosmic Dawn (CoDa): the First Radiation-Hydrodynamics Simulation of Reionization and Galaxy Formation in the L",
      "section": "suite not in sim-highline",
      "couldSupply": "CoDa I",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for sfms, sfrd, uvlf; not extractable at this quality."
    },
    {
      "arxiv": "1811.11192",
      "project": "CoDa",
      "year": 2018,
      "firstAuthor": "Ocvirk",
      "title": "Cosmic Dawn II (CoDa II): a new radiation-hydrodynamics simulation of the self-consistent coupling of galaxy f",
      "section": "suite not in sim-highline",
      "couldSupply": "CoDa II (ingested; UV luminosity functions from the appendix table, stellar mass function and stellar mass-halo mass relation from the public catalogue)",
      "status": "ingested",
      "statusNote": "Scanned 2026-10-08: captions mention uvlf in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1403.4245",
      "project": "CROC",
      "year": 2014,
      "firstAuthor": "Gnedin",
      "title": "Cosmic Reionization On Computers I. Design and Calibration of Simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "CROC I",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention uvlf in vector figures or tables (3); not yet extracted."
    },
    {
      "arxiv": "1603.00034",
      "project": "Aurora",
      "year": 2016,
      "firstAuthor": "Pawlik",
      "title": "The Aurora radiation-hydrodynamical simulations of reionization: calibration and first results",
      "section": "suite not in sim-highline",
      "couldSupply": "Aurora radiation-hydro reionization simulations",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention sfrd in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1904.02723",
      "project": "EDGE",
      "year": 2019,
      "firstAuthor": "Agertz",
      "title": "EDGE: the mass-metallicity relation as a critical test of galaxy formation physics",
      "section": "suite not in sim-highline",
      "couldSupply": "EDGE: mass-metallicity relation of ultra-faint dwarfs (a critical test)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1909.04664",
      "project": "EDGE",
      "year": 2019,
      "firstAuthor": "Rey",
      "title": "EDGE: The origin of scatter in ultra-faint dwarf stellar masses and surface brightnesses",
      "section": "suite not in sim-highline",
      "couldSupply": "scatter in ultra-faint stellar masses",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention size in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "2004.09530",
      "project": "EDGE",
      "year": 2020,
      "firstAuthor": "Rey",
      "title": "EDGE: From quiescent to gas-rich to star-forming low-mass dwarf galaxies",
      "section": "suite not in sim-highline",
      "couldSupply": "gas-rich to quiescent dwarfs",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention size in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1607.03127",
      "project": "EDGE",
      "year": 2016,
      "firstAuthor": "Read",
      "title": "The stellar mass-halo mass relation of isolated field dwarfs: a critical test of $Λ$CDM at the edge of galaxy ",
      "section": "suite not in sim-highline",
      "couldSupply": "Read+16 SHMR of isolated dwarfs (compares with observations)",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for gsmf, shmr; not extractable at this quality."
    },
    {
      "arxiv": "2010.07311",
      "project": "LYRA",
      "year": 2020,
      "firstAuthor": "Gutcke",
      "title": "LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars",
      "section": "suite not in sim-highline",
      "couldSupply": "LYRA I: multi-phase ISM of a dwarf galaxy with variable-energy supernovae",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2110.06233",
      "project": "LYRA",
      "year": 2021,
      "firstAuthor": "Gutcke",
      "title": "LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment",
      "section": "suite not in sim-highline",
      "couldSupply": "LYRA II: cosmological dwarf galaxy formation with inhomogeneous Pop III enrichment: MZR and SHMR of dwarfs to check",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2209.03366",
      "project": "LYRA",
      "year": 2022,
      "firstAuthor": "Gutcke",
      "title": "LYRA III: The smallest Reionization survivors",
      "section": "suite not in sim-highline",
      "couldSupply": "LYRA III: smallest reionization survivors",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention jstar, mzr, size in vector figures or tables (5); not yet extracted."
    },
    {
      "arxiv": "2511.10582",
      "project": "LYRA",
      "year": 2025,
      "firstAuthor": "Sureda",
      "title": "Co-evolution of baryons and dark matter halos of LYRA dwarf galaxies",
      "section": "suite not in sim-highline",
      "couldSupply": "co-evolution of baryons and dark matter in LYRA dwarfs",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention size, zstar in vector figures or tables (3); not yet extracted."
    },
    {
      "arxiv": "2511.21824",
      "project": "LYRA",
      "year": 2025,
      "firstAuthor": "Brown",
      "title": "LYRA ultra-faints: The emergence of faint dwarf galaxies in the presence of an early Lyman-Werner background",
      "section": "suite not in sim-highline",
      "couldSupply": "LYRA ultra-faints",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for h2, shmr; not extractable at this quality."
    },
    {
      "arxiv": "2609.38179",
      "project": "LYRA",
      "year": 2026,
      "firstAuthor": "Sureda",
      "title": "LYRA: The formation and growth of nuclear star clusters in dwarf galaxies",
      "section": "suite not in sim-highline",
      "couldSupply": "nuclear star clusters in dwarfs",
      "status": "candidate",
      "statusNote": ""
    },
    {
      "arxiv": "2006.06012",
      "project": "VINTERGATAN",
      "year": 2020,
      "firstAuthor": "Renaud",
      "title": "VINTERGATAN III: how to reset the metallicity of the Milky Way",
      "section": "suite not in sim-highline",
      "couldSupply": "VINTERGATAN III",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention jstar in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "2006.06011",
      "project": "VINTERGATAN",
      "year": 2020,
      "firstAuthor": "Renaud",
      "title": "VINTERGATAN II: the history of the Milky Way told by its mergers",
      "section": "suite not in sim-highline",
      "couldSupply": "VINTERGATAN II",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2206.08379",
      "project": "VINTERGATAN",
      "year": 2022,
      "firstAuthor": "Otero",
      "title": "VINTERGATAN IV: Cosmic phases of star formation in Milky Way-like galaxies",
      "section": "suite not in sim-highline",
      "couldSupply": "VINTERGATAN IV",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: captions mention bhsigma in vector figures or tables (1); not yet extracted."
    },
    {
      "arxiv": "1504.06261",
      "project": "GARROTXA",
      "year": 2015,
      "firstAuthor": "Roca-Fàbrega",
      "title": "GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and M",
      "section": "suite not in sim-highline",
      "couldSupply": "Milky Way-sized galaxies",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1208.0002",
      "project": "MaGICC",
      "year": 2012,
      "firstAuthor": "Stinson",
      "title": "Making Galaxies in a Cosmological Context: The Need for Early Stellar Feedback",
      "section": "suite not in sim-highline",
      "couldSupply": "early stellar feedback",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "2008.11207",
      "project": "DC Justice League",
      "year": 2020,
      "firstAuthor": "Applebaum",
      "title": "Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations",
      "section": "suite not in sim-highline",
      "couldSupply": "Mint-condition ultra-faint dwarfs in a Milky Way context",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: only raster figures for size, ssfr, uvlf; not extractable at this quality."
    },
    {
      "arxiv": "2512.04157",
      "project": "DREAMS",
      "year": 2025,
      "firstAuthor": "Lilie",
      "title": "The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark ",
      "section": "suite not in sim-highline",
      "couldSupply": "DREAMS: halo-to-halo variance",
      "status": "candidate",
      "statusNote": "Scanned 2026-10-08: no figure or table caption names a tracked relation."
    },
    {
      "arxiv": "1410.0365",
      "project": "L-Galaxies",
      "year": 2014,
      "firstAuthor": "Henriques",
      "title": "Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours",
      "section": "semi-analytic or empirical model",
      "couldSupply": "Planck-cosmology model: observed SF evolution",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1611.02286",
      "project": "L-Galaxies",
      "year": 2016,
      "firstAuthor": "Henriques",
      "title": "Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering",
      "section": "semi-analytic or empirical model",
      "couldSupply": "mass and environmental quenching",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1601.04709",
      "project": "SAGE",
      "year": 2016,
      "firstAuthor": "Croton",
      "title": "Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results",
      "section": "semi-analytic or empirical model",
      "couldSupply": "SAGE model",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1807.11180",
      "project": "Shark",
      "year": 2018,
      "firstAuthor": "Lagos",
      "title": "Shark: introducing an open source, free and flexible semi-analytic model of galaxy formation",
      "section": "semi-analytic or empirical model",
      "couldSupply": "Shark SAM",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1605.00647",
      "project": "Dark Sage",
      "year": 2016,
      "firstAuthor": "Stevens",
      "title": "Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model",
      "section": "semi-analytic or empirical model",
      "couldSupply": "angular momentum disc structure: j*",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1008.1786",
      "project": "Galacticus",
      "year": 2010,
      "firstAuthor": "Benson",
      "title": "Galacticus: A Semi-Analytic Model of Galaxy Formation",
      "section": "semi-analytic or empirical model",
      "couldSupply": "Galacticus",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1412.2712",
      "project": "Santa Cruz SAM and hydro review",
      "year": 2014,
      "firstAuthor": "Somerville",
      "title": "Physical Models of Galaxy Formation in a Cosmological Framework",
      "section": "semi-analytic or empirical model",
      "couldSupply": "review (cited in sim-highline notes)",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1705.05373",
      "project": "EMERGE",
      "year": 2017,
      "firstAuthor": "Moster",
      "title": "EMERGE - An empirical model for the formation of galaxies since $z\\sim10$",
      "section": "semi-analytic or empirical model",
      "couldSupply": "empirical model",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "2001.02687",
      "project": "EMERGE",
      "year": 2020,
      "firstAuthor": "O'Leary",
      "title": "EMERGE: Empirical predictions of galaxy merger rates since $z\\sim6$",
      "section": "semi-analytic or empirical model",
      "couldSupply": "merger rates",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "0901.4107",
      "project": "AREPO (moving mesh)",
      "year": 2009,
      "firstAuthor": "Springel",
      "title": "E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh",
      "section": "numerical method",
      "couldSupply": "Springel 2010 moving-mesh code",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1804.01987",
      "project": "AREPO-RT",
      "year": 2018,
      "firstAuthor": "Kannan",
      "title": "AREPO-RT: Radiation hydrodynamics on a moving mesh",
      "section": "numerical method",
      "couldSupply": "radiation hydrodynamics on a moving mesh",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1409.7395",
      "project": "GIZMO (meshless)",
      "year": 2014,
      "firstAuthor": "Hopkins",
      "title": "GIZMO: A New Class of Accurate, Mesh-Free Hydrodynamic Simulation Methods",
      "section": "numerical method",
      "couldSupply": "Hopkins 2015",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1304.7126",
      "project": "RAMSES-RT",
      "year": 2013,
      "firstAuthor": "Rosdahl",
      "title": "RAMSES-RT: Radiation hydrodynamics in the cosmological context",
      "section": "numerical method",
      "couldSupply": "radiation hydrodynamics in RAMSES",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "2010.03567",
      "project": "GADGET-4",
      "year": 2020,
      "firstAuthor": "Springel",
      "title": "Simulating cosmic structure formation with the GADGET-4 code",
      "section": "numerical method",
      "couldSupply": "Springel+21",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1707.03824",
      "project": "Gasoline2",
      "year": 2017,
      "firstAuthor": "Wadsley",
      "title": "Gasoline2: A Modern SPH Code",
      "section": "numerical method",
      "couldSupply": "Wadsley+17",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1409.1929",
      "project": "ChaNGa",
      "year": 2014,
      "firstAuthor": "Menon",
      "title": "Adaptive Techniques for Clustered N-Body Cosmological Simulations",
      "section": "numerical method",
      "couldSupply": "Menon+15",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "1707.05333",
      "project": "ChaNGa moving mesh",
      "year": 2017,
      "firstAuthor": "Chang",
      "title": "A Moving Mesh Hydrodynamic Solver for ChaNGa",
      "section": "numerical method",
      "couldSupply": "Chang+17",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    },
    {
      "arxiv": "2305.13380",
      "project": "SWIFT",
      "year": 2023,
      "firstAuthor": "Schaller",
      "title": "SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmo",
      "section": "numerical method",
      "couldSupply": "Schaller+24 code paper",
      "status": "skipped",
      "statusNote": "Out of scope: semi-analytic, empirical or method paper, not a cosmological hydrodynamical simulation suite. Revisit if the scope widens."
    }
  ]
}
