The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
ARCHITECTURE OF KEPLER'S MULTI-TRANSITING SYSTEMS. II. NEW INVESTIGATIONS WITH TWICE AS MANY CANDIDATES
Open accessAbstract
We report on the orbital architectures of Kepler systems having multiple-planet candidates identified in the analysis of data from the first six quarters of Kepler data and reported by Batalha et al. (2013). These data show 899 transiting planet candidates in 365 multiple-planet systems and provide a powerful means to study the statistical properties of planetary systems. Using a generic mass–radius relationship, we find that only two pairs of planets in these candidate systems (out of 761 pairs total) appear to be on Hill-unstable orbits, indicating ∼96% of the candidate planetary systems are correctly interpreted as true systems. We find that planet pairs show little statistical preference to be near mean-motion resonances. We identify an asymmetry in the distribution of period ratios near first-order resonances (e.g., 2:1, 3:2), with an excess of planet pairs lying wide of resonance and relatively few lying narrow of resonance. Finally, based upon the transit duration ratios of adjacent planets in each system, we find that the interior planet tends to have a smaller transit impact parameter than the exterior planet does. This finding suggests that the mode of the mutual inclinations of planetary orbital planes is in the range 1 0–2 2, for the packed systems of small planets probed by these observations.
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Cites
A hybrid symplectic integrator that permits close encounters between massive bodies
Chambers, J. E. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02379.x · Cited by 1,820
Borucki, W. J., Koch, D. G., Basri, G., Batalha, N., Brown, T. M., Bryson, S. T., Caldwell, D., Christensen-Dalsgaard, J., Cochran, W. D., DeVore, E., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/736/1/19 · Cited by 1,042
Self-citationA FIRST COMPARISON OF KEPLER PLANET CANDIDATES IN SINGLE AND MULTIPLE SYSTEMS
Latham, D. W., Rowe, J. F., Quinn, S. N., Batalha, N. M., Borucki, W. J., Brown, T. M., Bryson, S. T., Buchhave, L. A., Caldwell, D. A., Carter, J. A., et al. (2011) · The Astrophysical Journal · doi:10.1088/2041-8205/732/2/l24 · Cited by 188
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Cited by
OBLIQUITIES OF HOT JUPITER HOST STARS: EVIDENCE FOR TIDAL INTERACTIONS AND PRIMORDIAL MISALIGNMENTS
Albrecht, S., Winn, J. N., Johnson, J. A., Howard, A. W., Marcy, G. W., Butler, R. P., Arriagada, P., Crane, J. D., Shectman, S. A., Thompson, I. B., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/757/1/18 · Cited by 664
Thompson, S. E., Coughlin, J. L., Hoffman, K., Mullally, F., Christiansen, J. L., Burke, C. J., Bryson, S., Batalha, N., Haas, M. R., Catanzarite, J., et al. (2018) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/aab4f9 · Cited by 429
Self-citationA seven-planet resonant chain in TRAPPIST-1
Luger, R., Sestovic, M., Kruse, E., Grimm, S. L., Demory, B.-O., Agol, E., Bolmont, E., Fabrycky, D., Fernandes, C. S., Van Grootel, V., et al. (2017) · Nature Astronomy · doi:10.1038/s41550-017-0129 · Cited by 365
Self-citationWeiss, L. M., Marcy, G. W., Petigura, E. A., Fulton, B. J., Howard, A. W., Winn, J. N., Isaacson, H. T., Morton, T. D., Hirsch, L. A., Sinukoff, E. J., et al. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aa9ff6 · Cited by 328
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
Metadata
- Authors
- Fabrycky, D. C., Lissauer, J. J., Ragozzine, D., Rowe, J. F., Steffen, J. H., Agol, E., Barclay, T., Batalha, N., Borucki, W., Ciardi, D. R., Ford, E. B., Gautier, T. N., Geary, J. C., Holman, M. J., Jenkins, J. M., Li, J., Morehead, R. C., Morris, R. L., Shporer, A., Smith, J. C., Still, M., & Van Cleve, J.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2014-07-16
- Volume
- 790
- Issue
- 2
- Pages
- 146
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2039484433
- Cited by
- 723
- References
- 3
- FWCI
- 33.65
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: ARCHITECTURE OF KEPLER'S MULTI-TRANSITING SYSTEMS. II. NEW INVESTIGATIONS WITH TWICE AS MANY CANDIDATES. https://app.cochat.ai/papers/10.1088/0004-637x/790/2/146
- The paper
- Fabrycky, D. C., Lissauer, J. J., Ragozzine, D., Rowe, J. F., Steffen, J. H., Agol, E., Barclay, T., Batalha, N., Borucki, W., Ciardi, D. R., Ford, E. B., Gautier, T. N., Geary, J. C., Holman, M. J., Jenkins, J. M., Li, J., Morehead, R. C., Morris, R. L., Shporer, A., . . . Van Cleve, J. (2014). ARCHITECTURE OF KEPLER'S MULTI-TRANSITING SYSTEMS. II. NEW INVESTIGATIONS WITH TWICE AS MANY CANDIDATES. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/790/2/146
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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