[
 {
  "kind": "sample",
  "name": "TESS 2-minute SPOC light curves (PDCSAP and SAP flux), sectors 1-107",
  "source": "Mikulski Archive for Space Telescopes (MAST), public AWS bucket stpubdata",
  "details": "The 128,042 files data/sample_lcs.csv lists; the SHA-256 of each searched file is in data/run/lcs.csv.gz. Those the audit searches again are pinned in data/external.json."
 },
 {
  "kind": "sample",
  "name": "TESS 2-minute target pixel files of the light curves with counted flares",
  "source": "MAST",
  "details": "The cadences around each counted flare, cut by code/make_cutouts.py, are in data/tpf/; data/tpf/sources.csv gives each source file's SHA-256."
 },
 {
  "kind": "sample",
  "name": "TESS 2-minute target lists, sectors 1-107",
  "source": "TESS Science Office, MIT (tess.mit.edu)",
  "catalog": "all_targets_S001_v1.csv to all_targets_S107_v1.csv",
  "details": "Their TESS magnitudes per target and sector are in data/meta/lc_files_meta.csv.gz."
 },
 {
  "kind": "sample",
  "name": "TESS Input Catalog 8.2",
  "source": "CDS VizieR IV/39/tic82, queried by the CDS cross-match service on 2026-10-24",
  "details": "Rows of the candidate stars in data/meta/parent_bright.csv.gz."
 },
 {
  "kind": "sample",
  "name": "Gaia DR3 gaia_source, astrophysical_parameters, vari_classifier_result, vari_rotation_modulation, dr2_neighbourhood",
  "source": "ESA Gaia Archive TAP service, queried on 2026-10-24",
  "details": "Rows of the candidate stars in data/meta/parent_bright.csv.gz and data/meta/gaia_rotmod.csv."
 },
 {
  "kind": "sample",
  "name": "Gaia DR3 sources near the stars with counted flares and a control sample",
  "source": "CDS cross-match service, VizieR I/355/gaiadr3, queried on 2026-10-24",
  "details": "data/meta/gaia_neighbors.csv.gz and data/meta/neighbor_controls.csv (exploratory)."
 },
 {
  "kind": "sample",
  "name": "TESS eclipsing binaries of Prsa et al. (2022)",
  "source": "CDS VizieR J/ApJS/258/16",
  "details": "data/meta/prsa2022_tessebs.tsv"
 },
 {
  "kind": "sample",
  "name": "TESS spectral response function",
  "source": "AltaiPony repository, commit 7acd5af1210425cb935b359873f29d9303f65e4f (MIT licence)",
  "catalog": "altaipony/static/tess-response-function.csv",
  "details": "Pinned by SHA-256 in data/external.json."
 },
 {
  "kind": "software",
  "name": "Python",
  "source": "python.org, Docker image python:3.13-slim",
  "details": "3.13, image pinned by digest in env/Dockerfile"
 },
 {
  "kind": "software",
  "name": "NumPy",
  "source": "PyPI",
  "details": "2.5.4"
 },
 {
  "kind": "software",
  "name": "SciPy",
  "source": "PyPI",
  "details": "1.18.1 (least-squares template fits, Poisson intervals)"
 },
 {
  "kind": "software",
  "name": "Astropy",
  "source": "PyPI",
  "details": "8.0.2 (FITS reading, Lomb-Scargle periodograms)"
 },
 {
  "kind": "software",
  "name": "pandas",
  "source": "PyPI",
  "details": "3.1.0"
 },
 {
  "kind": "other",
  "name": "Detected fractions of injected flares, the injected profile, and the full sample's flare frequency before and after correction, from three figures of Vasilyev et al. (2024)",
  "source": "Their arXiv source, https://arxiv.org/e-print/2412.12265v1 (sha256:692d23613d85c2ad61d7e5ea39d9df18123e13c99cc6aa379ebe842ee0b09210)",
  "details": "code/read_figures.py, run once with pypdf 5.1.0, reads detectability_of_flares.pdf, mean_flare_profile.pdf, and pdf_flares_for_paper.pdf from the source into data/meta/vasilyev_detectability.csv, vasilyev_profile.csv, and vasilyev_frequency.csv."
 },
 {
  "kind": "software",
  "name": "pypdf 5.1.0",
  "source": "Python Package Index",
  "details": "Reads the figures for code/read_figures.py, outside the analysis's container."
 }
]
