The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
TrES-1: The Transiting Planet of a Bright K0 V Star
Open accessAbstract
We report the detection of a transiting Jupiter-sized planet orbiting a relatively bright ( V = 11.79) K0 V star. We detected the transit light-curve signature in the course of the TrES multisite transiting planet survey and confirmed the planetary nature of the companion via multicolor photometry and precise radial velocity measurements. We designate the planet TrES-1; its inferred mass is M Jup , its radius is 1.08 R Jup , and its orbital period is 3.030065 ± 0.000008 days. This planet has an orbital period similar to that of HD 209458b but about twice as long as those of the OGLE transiting planets. Its mass is indistinguishable from that of HD 209458b, but its radius is significantly smaller and fits the theoretical models without the need for an additional source of heat deep in the atmosphere, as has been invoked by some investigators for HD 209458b.
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
Detection of Planetary Transits Across a Sun-like Star
Charbonneau, D., Brown, T. M., Latham, D. W., & Mayor, M. (2000) · The Astrophysical Journal · doi:10.1086/312457 · Cited by 1,415
Self-citation
Cited by
The WASP Project and the SuperWASP Cameras
Pollacco, D. L., Skillen, I., Cameron, A. C., Christian, D. J., Hellier, C., Irwin, J., Lister, T. A., Street, R. A., West, R. G., Anderson, D., et al. (2006) · Publications of the Astronomical Society of the Pacific · doi:10.1086/508556 · Cited by 1,244
“More recent surveys have had more success, with published transit detections reported by the Optical Gravitational Lensing Experiment (OGLE) survey (Udalski et al. 2002a, 2002b), TrES-1 (Alonso et al. 2004), HD 189733 (Bouchy et al. 2005), and, most recently, XO-1 (McCullough et al. 2006).”
BackgroundSelf-citationButler, 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
Statistical Properties of Exoplanets
Udry, S., & Santos, N. C. (2007) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.45.051806.110529 · Cited by 622
Infrared radiation from an extrasolar planet
Deming, D., Seager, S., Richardson, L. J., & Harrington, J. (2005) · Nature · doi:10.1038/nature03507 · Cited by 614
The interiors of giant planets: Models and outstanding questions.
Guillot, T. (2005) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev.earth.32.101802.120325 · Cited by 524
Metadata
- Authors
- Alonso, R., Brown, T. M., Torres, G., Latham, D. W., Sozzetti, A., Mandushev, G., Belmonte, J. A., Charbonneau, D., Deeg, H. J., Dunham, E. W., O'Donovan, F. T., & Stefanik, R. P.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2004-09-01
- Volume
- 613
- Issue
- 2
- Pages
- L153-L156
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2041932094
- Cited by
- 456
- References
- 1
- FWCI
- 33.87
- 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: TrES-1: The Transiting Planet of a Bright K0 V Star. https://app.cochat.ai/papers/10.1086/425256
- The paper
- Alonso, R., Brown, T. M., Torres, G., Latham, D. W., Sozzetti, A., Mandushev, G., Belmonte, J. A., Charbonneau, D., Deeg, H. J., Dunham, E. W., O'Donovan, F. T., & Stefanik, R. P. (2004). TrES-1: The Transiting Planet of a Bright K0 V Star. The Astrophysical Journal. https://doi.org/10.1086/425256
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.
