The DOI matches its Crossref record; 15 of the 15 references it cites were found in a registry or an index.
The Exoplanet Orbit Database
Open accessAbstract
We present a database of well-determined orbital parameters of exoplanets, and their host stars' properties. This database comprises spectroscopic orbital elements measured for 427 planets orbiting 363 stars from radial velocity and transit measurements as reported in the literature. We have also compiled fundamental transit parameters, stellar parameters, and the method used for the planets discovery. This Exoplanet Orbit Database includes all planets with robust, well measured orbital parameters reported in peer-reviewed articles. The database is available in a searchable, filterable, and sortable form online through the Exoplanets Data Explorer table, and the data can be plotted and explored through the Exoplanet Data Explorer plotter. We use the Data Explorer to generate publication-ready plots, giving three examples of the signatures of exoplanet migration and dynamical evolution: We illustrate the character of the apparent correlation between mass and period in exoplanet orbits, the different selection biases between radial velocity and transit surveys, and that the multiplanet systems show a distinct semimajor-axis distribution from apparently singleton systems.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
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
A Jupiter-mass companion to a solar-type star
Mayor, M., & Queloz, D. (1995) · Nature · doi:10.1038/378355a0 · Cited by 4,111
The Planet‐Metallicity Correlation
Fischer, D. A., & Valenti, J. (2005) · The Astrophysical Journal · doi:10.1086/428383 · Cited by 1,654
Self-citationValenti, J. A., & Fischer, D. A. (2005) · The Astrophysical Journal Supplement Series · doi:10.1086/430500 · Cited by 1,460
Self-citationAccurate masses and radii of normal stars: modern results and applications
Torres, G., Andersen, J., & Giménez, A. (2010) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-009-0025-1 · Cited by 1,418
Butler, R. P., Wright, J. T., Marcy, G. W., Fischer, D. A., Vogt, S. S., Tinney, C. G., Jones, H. R. A., Carter, B. D., Johnson, J. A., McCarthy, C., et al. (2006) · The Astrophysical Journal · doi:10.1086/504701 · Cited by 914
Self-citationParallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue
van Leeuwen, F. (2009) · Astronomy & Astrophysics · doi:10.1051/0004-6361/200811382 · Cited by 535
The unseen companion of HD114762: a probable brown dwarf
Latham, D. W., Mazeh, T., Stefanik, R. P., Mayor, M., & Burki, G. (1989) · Nature · doi:10.1038/339038a0 · Cited by 406
TEN NEW AND UPDATED MULTIPLANET SYSTEMS AND A SURVEY OF EXOPLANETARY SYSTEMS
Wright, J. T., Upadhyay, S., Marcy, G. W., Fischer, D. A., Ford, E. B., & Johnson, J. A. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/693/2/1084 · Cited by 378
Self-citationTakeda, G., Ford, E. B., Sills, A., Rasio, F. A., Fischer, D. A., & Valenti, J. A. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/509763 · Cited by 355
Self-citation
Cited by
HABITABLE 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
“The orbital parameters of the planets and stellar characteristics were obtained from exoplanets.org (Wright et al. 2011).”
MethodThe Occurrence and Architecture of Exoplanetary Systems
Winn, J. N., & Fabrycky, D. C. (2015) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082214-122246 · Cited by 891
UNDERSTANDING THE MASS-RADIUS RELATION FOR SUB-NEPTUNES: RADIUS AS A PROXY FOR COMPOSITION
Lopez, E. D., & Fortney, J. J. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/792/1/1 · Cited by 722
Defining and cataloging exoplanets: the exoplanet.eu database
Schneider, J., Dedieu, C., Le Sidaner, P., Savalle, R., & Zolotukhin, I. (2011) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201116713 · Cited by 657
Solar System evolution from compositional mapping of the asteroid belt
DeMeo, F. E., & Carry, B. (2014) · Nature · doi:10.1038/nature12908 · Cited by 527
Metadata
- Authors
- Wright, J. T., Fakhouri, O., Marcy, G. W., Han, E., Feng, Y., Johnson, J. A., Howard, A. W., Fischer, D. A., Valenti, J. A., Anderson, J., & Piskunov, N.
- Venue
- Publications of the Astronomical Society of the Pacific
- Publisher
- IOP Publishing
- Published
- 2011-04
- Volume
- 123
- Issue
- 902
- Pages
- 412-422
- ISSN
- 0004-6280 (ISSN-L)
- 1538-3873
- OpenAlex
- W2116249072
- Cited by
- 398
- References
- 15
- FWCI
- 37.51
- Type
- journal article
- Language
- en
- Open access
- bronze
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
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: The Exoplanet Orbit Database. https://app.cochat.ai/papers/10.1086/659427
- The paper
- Wright, J. T., Fakhouri, O., Marcy, G. W., Han, E., Feng, Y., Johnson, J. A., Howard, A. W., Fischer, D. A., Valenti, J. A., Anderson, J., & Piskunov, N. (2011). The Exoplanet Orbit Database. Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/659427
Data sources
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).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.