The DOI matches its Crossref record; 111 of the 111 references it cites were found in a registry or an index.
A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone
Open accessAbstract
Context. Since low-mass stars have low luminosities, orbits at which liquid water can exist on Earth-sized planets are relatively close-in, which produces Doppler signals that are detectable using state-of-the-art Doppler spectroscopy.
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Citations
Cites
The Two Micron All Sky Survey (2MASS)
Skrutskie, M. F., Cutri, R. M., Stiening, R., Weinberg, M. D., Schneider, S., Carpenter, J. M., Beichman, C., Capps, R., Chester, T., Elias, J., et al. (2006) · The Astronomical Journal · doi:10.1086/498708 · Cited by 12,019
Validation of the new Hipparcos reduction
van Leeuwen, F. (2007) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20078357 · Cited by 3,736
Murray, C. D., & Dermott, S. F. (2000) · Cambridge University Press eBooks · doi:10.1017/cbo9781139174817 · Cited by 2,856
An Adaptive Metropolis Algorithm
Haario, H., Saksman, E., & Tamminen, J. (2001) · Bernoulli · doi:10.2307/3318737 · Cited by 2,631
Habitable Zones around Main Sequence Stars
Kasting, J. F., Whitmire, D. P., & Reynolds, R. T. (1993) · Icarus · doi:10.1006/icar.1993.1010 · Cited by 2,501 · cited 4×
“Traditionally, analyses of planetary habitability begin with determining if a planet is in the habitable zone (Dole 1964; Hart 1979; Kasting et al. 1993; Selsis et al. 2007; Kopparapu et al. 2013), but many factors are relevant.”
BackgroundInfluentialA new extensive library of PHOENIX stellar atmospheres and synthetic spectra
Husser, T.-O., Wende-von Berg, S., Dreizler, S., Homeier, D., Reiners, A., Barman, T., & Hauschildt, P. H. (2013) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201219058 · Cited by 1,943
Self-citationHABITABLE ZONES AROUND MAIN-SEQUENCE STARS: NEW ESTIMATES
Kopparapu, R. K., Ramirez, R., Kasting, J. F., Eymet, V., Robinson, T. D., Mahadevan, S., Terrien, R. C., Domagal-Goldman, S., Meadows, V., & Deshpande, R. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/765/2/131 · Cited by 1,615 · cited 3×
“Traditionally, analyses of planetary habitability begin with determining if a planet is in the habitable zone (Dole 1964; Hart 1979; Kasting et al. 1993; Selsis et al. 2007; Kopparapu et al. 2013), but many factors are relevant.”
BackgroundMethodInfluentialOrbital migration of the planetary companion of 51 Pegasi to its present location
Lin, D. N. C., Bodenheimer, P., & Richardson, D. C. (1996) · Nature · doi:10.1038/380606a0 · Cited by 1,235
The chaotic motion of the solar system: A numerical estimate of the size of the chaotic zones
Laskar, J. (1990) · Icarus · doi:10.1016/0019-1035(90)90084-m · Cited by 1,123
Chromospheric variations in main-sequence stars
Baliunas, S. L., Donahue, R. A., Soon, W. H., Horne, J. H., Frazer, J., Woodard-Eklund, L., Bradford, M., Rao, L. M., Wilson, O. C., Zhang, Q., et al. (1995) · The Astrophysical Journal · doi:10.1086/175072 · Cited by 1,054
Cited by
Extreme Water Loss and Abiotic O 2 Buildup on Planets Throughout the Habitable Zones of M Dwarfs
Luger, R., & Barnes, R. (2015) · Astrobiology · doi:10.1089/ast.2014.1231 · Cited by 585
Self-citationPerryman, M. (2018) · Cambridge University Press eBooks · doi:10.1017/9781108304160 · Cited by 340
The habitability of planets orbiting M-dwarf stars
Shields, A. L., Ballard, S., & Johnson, J. A. (2016) · Physics Reports · doi:10.1016/j.physrep.2016.10.003 · Cited by 319
High stellar FUV/NUV ratio and oxygen contents in the atmospheres of potentially habitable planets
Tian, F., France, K., Linsky, J. L., Mauas, P. J. D., & Vieytes, M. C. (2014) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2013.10.024 · Cited by 183
New planetary systems from the Calan–Hertfordshire Extrasolar Planet Search
Jenkins, J. S., Jones, H. R. A., Tuomi, M., Díaz, M., Cordero, J. P., Aguayo, A., Pantoja, B., Arriagada, P., Mahu, R., Brahm, R., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2811 · Cited by 66
Self-citation
Metadata
- Authors
- Anglada-Escudé, G., Tuomi, M., Gerlach, E., Barnes, R., Heller, R., Jenkins, J. S., Wende, S., Vogt, S. S., Paul Butler, R., Reiners, A., & Jones, H. R. A.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2013-08
- Volume
- 556
- Pages
- A126
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2033005444
- Cited by
- 381
- References
- 111
- FWCI
- 11.30
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Anglada-Escudé, G., Tuomi, M., Gerlach, E., Barnes, R., Heller, R., Jenkins, J. S., Wende, S., Vogt, S. S., Paul Butler, R., Reiners, A., & Jones, H. R. A. (2013). A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201321331
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