Citation notice #1318 · 2026-07-11 03:18:54.902493+00:00
Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts
cites 2025, The Astrophysical Journal, 991, 205, doi: 10.3847/1538-4357/adfdd6 Dav´ e, R., Angl´ es-Alc´ azar, D., Narayanan, D., et al, which carries a correction notice dated 2026-06-30. One-hop deterministic notice: the citation edge exists in the Pith bibliography graph; no model judged whether the citation was load-bearing.
Citing paper Event page Original DOI Notice DOI File a formal challenge All reference changes
01Evidence
Raw extraction · citation context · bibliography index 40
Journal of Cosmology and Astroparticle Physics2021, 046, DOI: https://dx. doi.org/10.1088/1475-7516/2021/12/046 (2021). 2108.08863. [39] Kravtsov, A. V ., Vikhlinin, A. A. & Meshcheryakov, A. V . Stellar Mass-Halo Mass Relation and Star Formation Efficiency in High-Mass Halos. Astronomy Letters44, 8-34, DOI: https://dx.doi.org/ 10.1134/S1063773717120015 (2018). 1401.7329. [40] Das, S., Truong, N., Chiang, Y .-K. & Mathur, S. Thermal Sunyaev-Zel'dovich Effect in the Cir- cumgalactic Medium. II. Dependence on Star Formation. The Astrophysical Journal991, 205, DOI: https://dx.doi.org/10.3847/1538-4357/adfdd6 (2025). 2508.09514. [41] Leung, C. et al. Stellar Mass-Dispersion Measure Correlations Constrain Baryonic Feedback in Fast
02Event
- Type
- Correction
- Source
- Crossref
- Original DOI
- 10.3847/1538-4357/adfdd6
- Notice DOI
- 10.3847/1538-4357/ae7a5b
- Date
- 2026-06-30
- Title
- Erratum: “Thermal Sunyaev–Zel’dovich Effect in the Circumgalactic Medium. II. Dependence on Star Formation” (2025, ApJ, 991, 205)
- Reasons
- ['Correction']
- Work
- 2025, The Astrophysical Journal, 991, 205, doi: 10.3847/1538-4357/adfdd6 Dav´ e, R., Angl´ es-Alc´ azar, D., Narayanan, D., et al (2025) The Astrophysical Journal
03Dispute this notice
If this citation does not depend on the flagged claim, or the event is wrong, say so. Disputes are public. For a signed challenge against the paper itself, use the formal challenge form.