Oxygen Appendix

• quarantine · O · I · red-optical · iag_fts_solar_atlas · solar_iag · ALL · SET-AGSS21 · SYNTH · 1D-LTE
  RYA-1097 gated re-run precedence: this product does NOT pass the RYA-1092 eligibility gate, so it was published into quarantine and did not supersede anything. [NOT_YET_DEFENSIBLE] O I is outside the ratified real set {Fe I, Fe II, Al}. It is a pilot measurement, not a product.
• quarantine · O · I · red-optical · iag_fts_solar_atlas · solar_iag · ALL · SYNTH · 1D-LTE
  RYA-1097 gated re-run precedence: this product does NOT pass the RYA-1092 eligibility gate, so it was published into quarantine and did not supersede anything. [NOT_YET_DEFENSIBLE] O I is outside the ratified real set {Fe I, Fe II, Al}. It is a pilot measurement, not a product.
• quarantine · O · I · red-optical · kpno_solar_atlas · solar_kpno_kurucz2005_corrected · ALL · SET-AGSS21 · SYNTH · 1D-LTE
  RYA-1097 gated re-run precedence: this product does NOT pass the RYA-1092 eligibility gate, so it was published into quarantine and did not supersede anything. [NOT_YET_DEFENSIBLE] O I is outside the ratified real set {Fe I, Fe II, Al}. It is a pilot measurement, not a product.
• quarantine · O · I · red-optical · kpno_solar_atlas · solar_kpno_kurucz2005_corrected · ALL · SYNTH · 1D-LTE
  RYA-1097 gated re-run precedence: this product does NOT pass the RYA-1092 eligibility gate, so it was published into quarantine and did not supersede anything. [NOT_YET_DEFENSIBLE] O I is outside the ratified real set {Fe I, Fe II, Al}. It is a pilot measurement, not a product.
• quarantine · O · I · red-optical · kpno_solar_atlas · solar_kpno_molecfit_corrected · ALL · SET-AGSS21 · SYNTH · 1D-LTE
  RYA-1097 gated re-run precedence: this product does NOT pass the RYA-1092 eligibility gate, so it was published into quarantine and did not supersede anything. [NOT_YET_DEFENSIBLE] O I is outside the ratified real set {Fe I, Fe II, Al}. It is a pilot measurement, not a product.
• quarantine · O · I · red-optical · kpno_solar_atlas · solar_kpno_molecfit_corrected · ALL · SYNTH · 1D-LTE
  RYA-1097 gated re-run precedence: this product does NOT pass the RYA-1092 eligibility gate, so it was published into quarantine and did not supersede anything. [NOT_YET_DEFENSIBLE] O I is outside the ratified real set {Fe I, Fe II, Al}. It is a pilot measurement, not a product.
• quarantine · O · I · VIS · harps · solar_harps_molecfit_corrected · ALL · FORB-OI_6300 · SYNTH · 1D-LTE
  RYA-1097 gated re-run precedence: this product does NOT pass the RYA-1092 eligibility gate, so it was published into quarantine and did not supersede anything. [STAT_BASIS_MISMATCH] sigma_stat here is a 'curvature_sigma' (SYNTH route, band_products.py:506) while the rest of the feed publishes a 'standard_error' (error_budget.py:609). The feed carries no stat_basis field, so `A +/- sigma_stat` renders as comparable when it is not -- this product's bar reads ~sqrt(n) times worse than it is. [NOT_YET_DEFENSIBLE] O I is outside the ratified real set {Fe I, Fe II, Al}. It is a pilot measurement, not a product.

Solar abundance and indicator analyses. Solar O atomic/molecular indicator lineage and atmospheric sensitivity; comparison literature, not an adopted Codex abundance. Sources: [1], [2].

Atomic data and gf authorities. The recorded O I/O II base pedigree is Wiese–Fuhr–Deters / Opacity Project theory. Per-transition exceptions and the open O I source decisions remain explicit. Sources: [3], [4], [5].

Atomic data and gf authorities. O I triplet source record: NIST (this script) — Tachiev NOT adopted; OPEN — referred to Ryan (RYA-1214 EOS) Sources: [3], [6].

Model and grid sources. Registered O I line/grid lineage: Amarsi, Nissen & Skuladottir 2019, A&A 630, A104 — line-by-line 3D-NLTE grids built on the Amarsi+2018 O I model atom. The current feed treatment remains authoritative; a grid reference does not imply a correction was applied. Sources: [7], [8].

Atomic data and gf authorities. Atomic O I entry; source-family pedigree only, not a substitute for a per-transition gf join. Sources: [3], [4], [5].

Model and grid sources. Feed treatment: 1D-LTE; no NLTE/3D correction is claimed for this entry. Turbospectrum is the synthesis implementation. Sources: [9].

Special diagnostics. The synthesis sidecar names Johansson’s Ni I blend data, Storey & Zeippen’s forbidden-line gf lineage and Caffau’s CO5BOLD comparison anchor. The feed entry remains 1D-LTE and quarantined; the sidecar’s cited anchor is not promoted to a measured abundance. Sources: [10], [11], [12].

• O-quarantine-361df42bd1f9 · quarantine · red-optical · solar_iag · SET-AGSS21 · 1D-LTE · not supplied · [1], [3], [4], [5], [9]
• O-quarantine-945c945b31da · quarantine · red-optical · solar_iag · not supplied · 1D-LTE · not supplied · [1], [3], [4], [5], [9]
• O-quarantine-e2dedb7ba833 · quarantine · red-optical · solar_kpno_kurucz2005_corrected · SET-AGSS21 · 1D-LTE · not supplied · [1], [3], [4], [5], [9]
• O-quarantine-eadb1d33ffa2 · quarantine · red-optical · solar_kpno_kurucz2005_corrected · not supplied · 1D-LTE · not supplied · [1], [3], [4], [5], [9]
• O-quarantine-da700d54e88d · quarantine · red-optical · solar_kpno_molecfit_corrected · SET-AGSS21 · 1D-LTE · not supplied · [1], [3], [4], [5], [9]
• O-quarantine-255dd9842275 · quarantine · red-optical · solar_kpno_molecfit_corrected · not supplied · 1D-LTE · not supplied · [1], [3], [4], [5], [9]
• O-quarantine-a69ed2a177ae · quarantine · VIS · solar_harps_molecfit_corrected · FORB-OI_6300 · 1D-LTE · not supplied · [1], [3], [4], [5], [9], [10], [11], [12]

Solar abundance and indicator analyses

• [1] — Asplund, M.; Amarsi, A. M.; Grevesse, N. (2021). The chemical make-up of the Sun: A 2020 vision. A&A 653, A141 DOI: 10.1051/0004-6361/202140445. source record
• [2] — Amarsi et al. 2021, A&A 656 A113 DOI: 10.1051/0004-6361/202141384. source record

Atomic data and gf authorities

• [3] — Kramida, A.; Ralchenko, Yu.; Reader, J.; NIST ASD Team (2024). NIST Atomic Spectra Database (version 5.11/5.12). National Institute of Standards and Technology, Gaithersburg, MD DOI: 10.18434/T4W30F. source record
• [4] — Wiese, W. L.; Fuhr, J. R. (2006). New Critical Compilations of Atomic Transition Probabilities for Neutral and Singly Ionized Carbon, Nitrogen, and Iron. Proceedings of the NASA Laboratory Astrophysics Workshop (14-16 February 2006, UNLV, Las Vegas) source record
• [5] — Wiese, W. L.; Fuhr, J. R.; Deters, T. M. (1996). Atomic Transition Probabilities of Carbon, Nitrogen, and Oxygen: A Critical Data Compilation. JPCRD Monograph 7. source record
• [6] — Tachiev & Froese Fischer 2002, A&A 385, 716 DOI: 10.1051/0004-6361:20011816. source record

Model and grid sources

• [7] — Amarsi, A. M.; Nissen, P. E.; Skuladottir, A. (2019). Carbon, oxygen, and iron abundances in disk and halo stars. A&A 630, A104 DOI: 10.1051/0004-6361/201936265. source record
• [8] — Amarsi, Barklem, Asplund, Collet & Zatsarinny 2018, A&A 616, A89 DOI: 10.1051/0004-6361/201832770. source record
• [9] — Gerber, J. M.; Magg, E.; Plez, B.; Bergemann, M.; Heiter, U.; Olander, T.; Hoppe, R. (2023). Non-LTE radiative transfer with Turbospectrum. A&A 669, A43 DOI: 10.1051/0004-6361/202243673. source record

Special diagnostics

• [10] — Johansson, S.; Litzen, U.; Lundberg, H.; Zhang, Z. (2003). Experimental f-Value and Isotopic Structure for the Ni I Line Blended with [O I] at 6300 A. ApJ 584, L107 DOI: 10.1086/374037. source record
• [11] — Storey, P. J.; Zeippen, C. J. (2000). Theoretical values for the [O III] 5007/4959 line-intensity ratio and homologous cases. MNRAS 312, 813 DOI: 10.1046/j.1365-8711.2000.03184.x. source record
• [12] — Caffau, E.; Ludwig, H.-G.; Steffen, M.; Livingston, W.; Bonifacio, P.; Malherbe, J.-M.; Doerr, H.-P.; Schmidt, W. (2015). The photospheric solar oxygen project. III. Investigation of the centre-to-limb variation of the 630 nm [O I]–Ni I blend. A&A 579, A88. source record