High stellar FUV/NUV ratio and oxygen contents in the atmospheres of potentially habitable planets
Open accessIntegrity signals
Registry
Cites
Statistics
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
Several groups have studied the possibility of detectable levels of oxygen and ozone formation in CO2-rich planets orbiting M dwarfs, FGKM stars with low-H2/high-CO2 atmospheres, and pre-main sequence M stars.
“Recently, several groups have studied the possibility of detectable levels of oxygen and ozone formation in CO2-rich planets orbiting M dwarfs (Hu et al., 2012; Tian et al., 2014), FGKM stars with low-H2/high-CO2 atmospheres (Domagal-Goldman et al., 2014), and pre-main sequence M stars (Luger and Barnes, 2015).”
From The Astrobiology Primer v2.0 (2016) · cites this paper as Tian et al., 2014
Cites
A Hydrogen-Rich Early Earth Atmosphere
Tian, F., Toon, O. B., Pavlov, A. A., & De Sterck, H. (2005) · Science · doi:10.1126/science.1106983 · Cited by 390 · see citing works
Self-citationSpectral Evolution of an Earth‐like Planet
Kaltenegger, L., Traub, W. A., & Jucks, K. W. (2007) · The Astrophysical Journal · doi:10.1086/510996 · Cited by 274 · see citing works
Photochemical and climate consequences of sulfur outgassing on early Mars
Tian, F., Claire, M. W., Haqq-Misra, J. D., Smith, M., Crisp, D. C., Catling, D., Zahnle, K., & Kasting, J. F. (2010) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2010.04.016 · Cited by 123 · see citing works
Self-citation
Flagged first, then by citations
Cited by
Sorted by citations
Exoplanet Biosignatures: A Framework for Their Assessment
Catling, D. C., Krissansen-Totton, J., Kiang, N. Y., Crisp, D., Robinson, T. D., DasSarma, S., Rushby, A. J., Del Genio, A., Bains, W., & Domagal-Goldman, S. (2018) · Astrobiology · doi:10.1089/ast.2017.1737 · Cited by 225 · see citing works
Reflections on O <sub>2</sub> as a Biosignature in Exoplanetary Atmospheres
Meadows, V. S. (2017) · Astrobiology · doi:10.1089/ast.2016.1578 · Cited by 173 · see citing works
Krissansen-Totton, J., Garland, R., Irwin, P., & Catling, D. C. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aad564 · Cited by 145 · see citing works
Domagal-Goldman, S. D., Wright, K. E., Domagal-Goldman, S. D., Wright, K. E., Adamala, K., Arina de la Rubia, L., Bond, J., Dartnell, L. R., Goldman, A. D., Lynch, K., et al. (2016) · Astrobiology · doi:10.1089/ast.2015.1460 · Cited by 136 · see citing works
“…groups have studied the possibility of detectable levels of oxygen and ozone formation in CO2rich planets orbiting M dwarfs (Hu et al., 2012; Tian et al., 2014), FGKM stars with low-H2/high-CO2 atmospheres (Domagal-Goldman et al., 2014), and pre-main sequence M stars (Luger and Barnes,…”
Schwieterman, E. W., Meadows, V. S., Domagal-Goldman, S. D., Deming, D., Arney, G. N., Luger, R., Harman, C. E., Misra, A., & Barnes, R. (2016) · The Astrophysical Journal Letters · doi:10.3847/2041-8205/819/1/l13 · Cited by 111 · see citing works
Lammer, H., Sproß, L., Grenfell, J. L., Scherf, M., Fossati, L., Lendl, M., & Cubillos, P. E. (2019) · Astrobiology · doi:10.1089/ast.2018.1914 · Cited by 67 · see citing works
- Authors
- Tian, F., France, K., Linsky, J. L., Mauas, P. J. D., & Vieytes, M. C.
- Affiliations
- National Astronomical Observatories (CN)
- University of Colorado Boulder (US)
- Joint Institute for Laboratory Astrophysics (US)
- Consejo Nacional de Investigaciones Científicas y Técnicas (AR)
- Corresponding author
- Tian, Feng
- Venue
- Earth and Planetary Science Letters
- Publisher
- Elsevier BV
- Published
- 2014-01
- Volume
- 385
- Pages
- 22-27
- ISSN
- 0012-821X (ISSN-L)
- OpenAlex
- W2055437178
- Cited by
- 183
- References
- 3
- Citations by year
- 2026: 3 · 2025: 9 · 2024: 10 · 2023: 8 · 2022: 10 · 2021: 15 · 2020: 15 · 2019: 19 · 2018: 30 · 2017: 16 · 2016: 20 · 2015: 15 · 2014: 11 · 2012: 1
- FWCI
- 8.27
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Earth and Planetary Science Letters (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CONICET Digital (CONICET) (submittedVersion, cc-by-nc-sa)
- arXiv (Cornell University)
- DPS
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Keywords
- M dwarfs, atmospheric oxygen, ozone photolysis, biosignatures, ultraviolet radiation, water photolysis, planetary atmospheres
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
