The DOI matches its Crossref record; 14 of the 14 references it cites were found in a registry or an index.
Detection of Planetary Transits Across a Sun-like Star
Open accessAbstract
We report high-precision, high-cadence photometric measurements of the star HD 209458, which is known from radial velocity measurements to have a planetary-mass companion in a close orbit. We detect two separate transit events at times that are consistent with the radial velocity measurements. In both cases, the detailed shape of the transit curve due to both the limb darkening of the star and the finite size of the planet is clearly evident. Assuming stellar parameters of 1.1 R middle dot in circle and 1.1 M middle dot in circle, we find that the data are best interpreted as a gas giant with a radius of 1.27+/-0.02 RJup in an orbit with an inclination of 87&fdg;1+/-0&fdg;2. We present values for the planetary surface gravity, escape velocity, and average density and discuss the numerous observations that are warranted now that a planet is known to transit the disk of its parent star.
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.
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?
The cited source says what the claim attributes to it.
In the citing paper
“A number of hot Jupiters-including HD 209458b, the first hot Jupiter to be discovered to transit (Charbonneau et al. 2000, Henry et al. 2000)-have radii larger than expected from internal structure models.”
From Origins of Hot Jupiters (2018) · cites this paper as Charbonneau et al. 2000
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
A Jupiter-mass companion to a solar-type star
Mayor, M., & Queloz, D. (1995) · Nature · doi:10.1038/378355a0 · Cited by 4,111
Self-citationHIRES: the high-resolution echelle spectrometer on the Keck 10-m Telescope
Vogt, S. S., Allen, S. L., Bigelow, B. C., Bresee, L., Brown, W. E., Cantrall, T., Conrad, A. R., Couture, M. D., Delaney, C., Epps, H. W., et al. (1994) · Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · doi:10.1117/12.176725 · Cited by 1,606
ELODIE: A spectrograph for accurate radial velocity measurements
Baranne, A., Queloz, D., Mayor, M., Adrianzyk, G., Knispel, G., Kohler, D., Lacroix, D., Meunier, J., Rimbaud, G., & Vin, A. (1996) · Astronomy & Astrophysics Supplement Series · doi:10.1051/aas:1996251 · Cited by 986
Self-citationTHE CENTER OF THE CORE-CUSP GLOBULAR CLUSTER M15: CFHT AND HST OBSERVATIONS, ALLFRAME REDUCTIONS
Stetson, P. (1994) · Publications of the Astronomical Society of the Pacific · doi:10.1086/133378 · Cited by 945
Three New “51 Pegasi–Type” Planets
Butler, R. P., Marcy, G. W., Williams, E. C., Hauser, H. M., & Shirts, P. (1997) · The Astrophysical Journal · doi:10.1086/310444 · Cited by 459
Giant Planets at Small Orbital Distances
Guillot, T., A. Burrows, W. B. Hubbard, Lunine, J. I., & Saumon, D. (1996) · The Astrophysical Journal · doi:10.1086/309935 · Cited by 413
On the detection of satellites of extrasolar planets with the method of transits
Sartoretti, P., & Schneider, J. (1999) · Astronomy & Astrophysics Supplement Series · doi:10.1051/aas:1999148 · Cited by 228
An Upper Limit on the Reflected Light from the Planet Orbiting the Star τ Bootis
Charbonneau, D., Noyes, R. W., Korzennik, S. G., Nisenson, P., Jha, S. W., Vogt, S. S., & Kibrick, R. I. (1999) · The Astrophysical Journal · doi:10.1086/312234 · Cited by 188
Self-citationPlanetary Companions around Two Solar‐Type Stars: HD 195019 and HD 217107
Fischer, D. A., Marcy, G. W., Butler, R. P., Vogt, S. S., & Apps, K. (1999) · Publications of the Astronomical Society of the Pacific · doi:10.1086/316304 · Cited by 136
A Planet with a 3.1 Day Period around a Solar Twin
Butler, R. P., Marcy, G. W., Vogt, S. S., & Apps, K. (1998) · Publications of the Astronomical Society of the Pacific · doi:10.1086/316287 · Cited by 99
Flagged first, then by citations
Research works printed but not linked: 4
- Borucki, W. J., Koch, D. G., Dunham, E. W. & Jenkins, J. M. 1997, in ASP Conf. Ser. 119, Planets beyond Our Solar System and Next-Generation Space Telescope, ed. D. Soderblom (San Francisco: ASP), 153
- Cameron, A., Horne, K., Penny, A. & James, D. 1999, Nature, in press (astro-ph/9911314) · arXiv
- Queloz, D., etal 1999, A&A, in press (astro-ph/9910223) · arXiv
- Rouan, D., etal 1999, Phys. Chem. Earth, in press
Cited by
Sorted by citations
Items 801–900 of 1,000
TTV-determined Masses for Warm Jupiters and Their Close Planetary Companions
Wu, D.-H., Wang, S., Zhou, J., Steffen, J. H., & Laughlin, G. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aad22b · Cited by 15
Deeg, H. J., Alonso, R., Belmonte, J. A., Alsubai, K. A., Horne, K., & Doyle, L. R. (2004) · Publications of the Astronomical Society of the Pacific · doi:10.1086/425151 · Cited by 17
PLANETARY TRANSITS TOWARD THE GALACTIC BULGE
Gaudi, B. S. (2000) · Cited by 17
Robinson, S. E., Strader, J., Ammons, S. M., Laughlin, G., & Fischer, D. (2006) · The Astrophysical Journal · doi:10.1086/498565 · Cited by 16
Lanza, A. F., & Mathis, S. (2016) · Celestial Mechanics and Dynamical Astronomy · doi:10.1007/s10569-016-9714-z · Cited by 16
WASP-4b Transit Observations With GROND
Nikolov, N., Henning, T. K., Koppenhoefer, J., Lendl, M., Maciejewski, G., & Greiner, J. (2012) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201118336/pdf · Cited by 16
Shallowness of circulation in hot Jupiters
Knierim, H., Batygin, K., & Bitsch, B. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202142588 · Cited by 19
Signs of Similar Stellar Obliquity Distributions for Hot and Warm Jupiters Orbiting Cool Stars
Morgan, M., Bowler, B. P., Tran, Q. H., Petigura, E. A., Nagpal, V., & Blunt, S. C. (2024) · The Astronomical Journal · doi:10.3847/1538-3881/ad0728 · Cited by 17
Malsky, I., Rauscher, E., Roman, M. T., Lee, E. K. H., Beltz, H., Savel, A. B., Kempton, E. M.-R., & Cinque, L. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad0b70 · Cited by 16
Methods for Incorporating Model Uncertainty into Exoplanet Atmospheric Analysis
Nixon, M. C., Welbanks, L., McGill, P., & Kempton, E. M.-R. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad354e · Cited by 16
Southworth, J. H., Mancini, L., Tregloan-Reed, J., Novati, S. C., Ciceri, S., D’Ago, G., Delrez, L., Dominik, M., Evans, D. F., Gillon, M., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2183 · Cited by 16
High energy astrophysics – an introduction
Longair, M. S. (2011) · Cambridge University Press eBooks · doi:10.1017/cbo9780511778346.002 · Cited by 16
Exoplanets: Past, Present, and Future
Lee, C. (2018) · Galaxies · doi:10.3390/galaxies6020051 · Cited by 16
Kosso, P. (2006) · Studies in History and Philosophy of Science Part A · doi:10.1016/j.shpsa.2005.05.001 · Cited by 16
The Search for Worlds Like Our Own
Fridlund, M. C., Eiroa, C., Henning, T. K., Herbst, T. M., Lammer, H., Leger, A. M., Liseau, R., Paresce, F., Penny, A. J., Quirrenbach, A., et al. (2010) · Astrobiology · doi:10.1089/ast.2009.0380 · Cited by 16
Coronal Mass Ejection Effect on Envelopes of Hot Jupiters
Zhilkin, A. G., Бисикало, Д. В., & Kaygorodov, P. V. (2020) · Astronomy Reports · doi:10.1134/s1063772920020055 · Cited by 16
The formation of planetary systems
Oxley, S., & Woolfson, M. M. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.07417.x · Cited by 16
SuperWASP-North extrasolar planet candidates: candidates from fields 17 h < RA < 18 h
Lister, T. A., West, R. G., Wilson, D. M., Cameron, A. C., Clarkson, W. I., Street, R. A., Enoch, B., Parley, N. R., Christian, D. J., Kane, S. R., et al. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11948.x · Cited by 16
Transit origami: a method to coherently fold exomoon transits in time series photometry
Kipping, D. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab2013 · Cited by 15
Day and night side core cooling of a strongly irradiated giant planet
Budaj, J., Hubeny, I., & Burrows, A. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201117975 · Cited by 15
Nielsen, L. D., Bouchy, F., Turner, O., Anderson, D. R., Barkaoui, K., Benkhaldoun, Z., Burdanov, A., Cameron, A. C., Delrez, L., Gillon, M., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2351 · Cited by 15
A Photometric Search for Planets in the Open Cluster NGC 7086
Rosvick, J. M., & Robb, R. M. (2006) · The Astronomical Journal · doi:10.1086/508517 · Cited by 15
The thermal emission of the exoplanet WASP-3b
Rostron, J. W., Wheatley, P. J., Anderson, D. R., Cameron, A. C., Fortney, J. J., Harrington, J., Knutson, H. A., & Pollacco, D. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu814 · Cited by 15
Magnetospheres of hot Jupiters: hydrodynamic models and ultraviolet absorption
Alexander, R. D., Wynn, G. A., Mohammed, H. O., Nichols, J. D., & Ercolano, B. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2867 · Cited by 15
KELT-18b: Puffy Planet, Hot Host, Probably Perturbed
McLeod, K. K., Rodriguez, J. E., Oelkers, R. J., Collins, K. A., Bieryla, A., Fulton, B. J., Stassun, K. G., Gaudi, B. S., Penev, K., Stevens, D. J., et al. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa6d5d · Cited by 15
Self-citationInfrared absorption spectra of hot ammonia
Beale, C. A., Hargreaves, R. J., Coles, P. A., Tennyson, J., & Bernath, P. F. (2017) · Journal of Quantitative Spectroscopy and Radiative Transfer · doi:10.1016/j.jqsrt.2017.02.012 · Cited by 15
A system of three transiting super-Earths in a cool dwarf star
Díez-Alonso, E., Gómez, S. L. S., Hernández, J. I. G., Mascareño, A. S., González-Gutiérrez, C., Velasco, S., Toledo-Padrón, B., Juez, F. J. D. C., & Rebolo, R. (2018) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/sly040 · Cited by 15
Using HARPS-N to characterize the long-period planets in the PH-2 and Kepler-103 systems
Dubber, S., Mortier, A., Rice, K., Nava, C., Malavolta, L., Giles, H., Coffinet, A., Charbonneau, D., Vanderburg, A. M., Bonomo, A. S., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2856 · Cited by 15
Self-citationNon-local thermodynamic equilibrium transmission spectrum modelling of HD 209458b
Young, M. E., Fossati, L., Koskinen, T. T., Salz, M., Cubillos, P. E., & France, K. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202037672 · Cited by 15
ELODIE metallicity-biased search for transiting Hot Jupiters
Santos, N. C., Udry, S., Bouchy, F., da Silva, R., Loeillet, B., Mayor, M., Moutou, C., Pont, F. J., Queloz, D. P., Zucker, S., et al. (2008) · Astronomy and Astrophysics · doi:10.1051/0004-6361:200809402 · Cited by 15
Self-citationStellar Analogs of Solar Activity: The Sun in A Stellar Context
Giampapa, M. S. (2005) · Springer eBooks · doi:10.1007/3-540-27510-x_3 · Cited by 15
The Brave New World of Binary Star Studies
Guinan, E. F., & Engle, S. G. (2006) · Astrophysics and Space Science · doi:10.1007/s10509-006-9069-0 · Cited by 15
Fortney, J. J., Lupu, R. E., Morley, C. V., Freedman, R. S., & Hood, C. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab2a10 · Cited by 15
On the Effects of Planetary Oblateness on Exoplanet Studies
Berardo, D., & de Wit, J. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac82b2 · Cited by 14
Detection and characterization of giant planets with Gaia astrometry
Wallace, A. L., Casey, A. R., Brown, A. G. A., & Castro-Ginard, A. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae2769 · Cited by 14
Debris disc candidates in systems with transiting planets
Krivov, A. V., Reidemeister, M., Fiedler, S., Löhne, T., & Neuhäuser, R. (2011) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2011.01133.x · Cited by 14
Possible New Envelope Types of Hot Jupiters
Zhilkin, A. G., & Бисикало, Д. В. (2020) · Astronomy Reports · doi:10.1134/s1063772920080090 · Cited by 14
Phase-curve Pollution of Exoplanet Transit Depths
Martin-Lagarde, M., Morello, G., Lagage, P.-O., Gastaud, R., & Cossou, C. (2020) · The Astronomical Journal · doi:10.3847/1538-3881/abac09 · Cited by 14
Tidal Response and Shape of Hot Jupiters
Wahl, S. M., Thorngren, D., Lu, T., & Militzer, B. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac1a72 · Cited by 14
Detection of TiO and VO in the Atmosphere of WASP-121b and Evidence For its Temporal Variation
Ouyang, Q., Wang, W., Zhai, M., Chen, G., Rojo, P., Liu, Y., Zhao, F., Huang, J., & Zhao, G. (2023) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/accbb2 · Cited by 14
NON-AXISYMMETRIC FLOWS ON HOT JUPITERS WITH OBLIQUE MAGNETIC FIELDS
Batygin, K., & Stanley, S. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/794/1/10 · Cited by 17
Atmospheric mass-loss of extrasolar planets orbiting magnetically active host stars
Lalitha, S., Schmitt, J. H. M. M., & Dash, S. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty732 · Cited by 14
Zhilkin, A. G., Бисикало, Д. В., & Kaygorodov, P. V. (2020) · Astronomy Reports · doi:10.1134/s1063772920030063 · Cited by 14
Terminus: A Versatile Simulator for Space-based Telescopes
Edwards, B., & Stotesbury, I. (2021) · The Astronomical Journal · doi:10.3847/1538-3881/abdf4d · Cited by 13
Structure and Evolution of Giant Planets
Baraffe, I. (2005) · Space Science Reviews · doi:10.1007/s11214-005-1948-0 · Cited by 14
Fressin, F., Guillot, T., & Nesta, L. J. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200810097 · Cited by 14
CYCLIC TRANSIT PROBABILITIES OF LONG-PERIOD ECCENTRIC PLANETS DUE TO PERIASTRON PRECESSION
Kane, S. R., Horner, J., & von Braun, K. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/757/1/105 · Cited by 14
Kane, S. R., Cameron, A. C., Horne, K., James, D., Lister, T. A., Pollacco, D. L., Street, R. A., & Tsapras, Y. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09656.x · Cited by 14
Prospects for spectroscopic reflected-light planet searches
Leigh, C. J., Cameron, A. C., & Guillot, T. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2003.07139.x · Cited by 14
Beta Pictoris and Other Solar Systems
Artymowicz, P. (2000) · Space Science Reviews · doi:10.1023/a:1005297300878 · Cited by 14
A Binary Shaped Mask Coronagraph for a Segmented PupilPreprint
Enya, K., & Abe, L. (2010) · Cited by 14
Detectability of Exoplanetary Transits from Radial Velocity SurveysPreprint
Kane, S. R. (2008) · Cited by 14
The Chemistry of Extra-solar Materials from White Dwarf Planetary Systems
Xu, S., Rogers, L. K., & Blouin, S. (2024) · Reviews in Mineralogy and Geochemistry · doi:10.2138/rmg.2024.90.06 · Cited by 13
From Tides to Currents: Unraveling the Mechanism that Powers WASP-107b’s Internal Heat Flux
Batygin, K. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adccc4 · Cited by 17
Ground-based detection of the near-infrared emission from the dayside of WASP-5b
Chen, G., van Boekel, R., Madhusudhan, N., Wang, H., Nikolov, N., Seemann, U., & Henning, T. K. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321804 · Cited by 13
Cameron, A. C. (2016) · Astrophysics and space science library · doi:10.1007/978-3-319-27458-4_2 · Cited by 14
MOA-bin-29b: A Microlensing Gas-giant Planet Orbiting a Low-mass Host Star
Kondo, I., Sumi, T., Bennett, D. P., Udalski, A., Bond, I. A., Rattenbury, N. J., Bozza, V., Hirao, Y., Suzuki, D., Koshimoto, N., et al. (2019) · The Astronomical Journal · doi:10.3847/1538-3881/ab4e9e · Cited by 14
Theory of a rotationally shearing interferometer.
González-Romero, R., Strojnik, M., & Garcia-Torales, G. (2021) · Journal of The Optical Society of America A-optics Image Science and Vision · doi:10.1364/josaa.406186 · Cited by 11
Five Methods of Exoplanet Detection
Dai, Z., Ni, D., Pan, L., & Zhu, Y. (2021) · Journal of Physics Conference Series · doi:10.1088/1742-6596/2012/1/012135 · Cited by 13
Gaidos, E. J., Anderson, D. R., Lépine, S., Colón, K. D., Maravelias, G., Narita, N., Chang, E., Beyer, J., Fukui, A., Armstrong, J. D., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2078 · Cited by 13
SONG – getting ready for the prototype
Grundahl, F., Christensen-Dalsgaard, J., Jørgensen, U. G., Frandsen, S., Kjeldsen, H., & Rasmussen, P. K. (2011) · Journal of Physics Conference Series · doi:10.1088/1742-6596/271/1/012083 · Cited by 13
Pepper, J., Stassun, K. G., & Gaudi, B. S. (2018) · Springer eBooks · doi:10.1007/978-3-319-55333-7_128 · Cited by 13
Johns, D., Reed, P. A., Rodriguez, J. E., Pepper, J. A., Stassun, K. G., Penev, K., Gaudi, B. S., Labadie-Bartz, J. M., Fulton, B. J., Quinn, S. N., et al. (2019) · The Astronomical Journal · doi:10.3847/1538-3881/ab24c7 · Cited by 13
Self-citationMarov, M. Y., & Shevchenko, I. I. (2019) · Physics-Uspekhi · doi:10.3367/ufne.2019.10.038673 · Cited by 17
Strojnik, M., & Bravo-Medina, B. (2020) · Optics Express · doi:10.1364/oe.398649 · Cited by 10
Non-local thermodynamic equilibrium transmission spectrum modelling of HD 209458b
Young, M. E., Fossati, L., Koskinen, T., Salz, M., Cubillos, P. E., & France, K. C. (2020) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/202037672/pdf · Cited by 13
Ксанфомалити, Л. В. (2000) · Solar System Research · doi:10.1023/a:1005218112981 · Cited by 13
The Interior Structure, Composition, and Evolution of Giant Planets
Fortney, J. J., & Nettelmann, N. (2009) · Space sciences series of ISSI · doi:10.1007/978-1-4419-5901-0_13 · Cited by 15
Binaries at the Bottom of the Main Sequence and below
Mayor, M., Udry, S., Halbwachs, J. L., & Arenou, F. (2001) · Symposium - International Astronomical Union · doi:10.1017/s0074180900225047 · Cited by 13
Self-citationCoronal X-ray emission and planetary irradiation in HD 209458
Czesla, S., Salz, M., Schneider, P. C., Mittag, M., & Schmitt, J. H. M. M. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201731408 · Cited by 12
Implicit Biases in Transit Models Using Stellar Pseudo Density
Gilbert, G. J., MacDougall, M. G., & Petigura, E. A. (2022) · The Astronomical Journal · doi:10.3847/1538-3881/ac7f2f · Cited by 12
The Impact of Cometary “Impacts” on the Chemistry, Climate, and Spectra of Hot Jupiter Atmospheres
Sainsbury-Martinez, F., & Walsh, C. M. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad28b3 · Cited by 12
TWENTY-ONE NEW LIGHT CURVES OF OGLE-TR-56b: NEW SYSTEM PARAMETERS AND LIMITS ON TIMING VARIATIONS
Adams, E. R., López‐Morales, M., Elliot, J. L., Seager, S., Osip, D. J., Holman, M. J., Winn, J. N., Hoyer, S., & Rojo, P. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/741/2/102 · Cited by 12
Garai, Z., Pribulla, T., Hambálek, Ľ., Kundra, E., Vaňko, M., Raetz, S., Seeliger, M., Marka, C., & Gilbert, H. (2017) · Astronomische Nachrichten · doi:10.1002/asna.201613208 · Cited by 12
Out-of-transit Refracted Light in the Atmospheres of Transiting and Non-transiting Exoplanets
Dalba, P. A. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa8e47 · Cited by 12
Borra, E. F., & Deschatelets, D. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2593 · Cited by 12
Efficient and Precise Transit Light Curves for Rapidly Rotating, Oblate Stars
Dholakia, S., Luger, R., & Dholakia, S. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac33aa · Cited by 12
Detecting transits from Earth-sized planets around Sun-like stars
Carpano, S., & Fridlund, M. (2008) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20079268 · Cited by 12
Using near-infrared spectroscopy for characterization of transiting exoplanets
Aronson, E., Waldén, P., & Piskunov, N. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201424058 · Cited by 9
Ksanfomality, L. V. (2004) · Solar System Research · doi:10.1023/b:sols.0000043813.80362.1a · Cited by 12
Moldovan, R., Matthews, J. M., Gladman, B., Bottke, W. F., & Vokrouhlický, D. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/716/1/315 · Cited by 12
Ricci, D., Sada, P. V., Navarro-Meza, S., López–Valdivia, R., Michel, R., Machado, L. F., Ramón-Fox, F. G., Ayala-Loera, C., Sevilla, S. B., Reyes-Ruiz, M., et al. (2017) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/aa6b54 · Cited by 12
The Habitability of Our Evolving Galaxy
Gowanlock, M., & Morrison, I. S. (2018) · Elsevier eBooks · doi:10.1016/b978-0-12-811940-2.00007-1 · Cited by 16
Design Considerations for a Ground-based Search for Transiting Planets around L and T Dwarfs
Tamburo, P., & Muirhead, P. S. (2019) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/ab3a1e · Cited by 12
Data Mining and Machine Learning in Time-Domain Discovery and Classification
Bloom, J. S., & RICHARDS, J. (2012) · Chapman & Hall/CRC data mining and knowledge discovery series · doi:10.1201/b11822-10 · Cited by 12
Formation of the Outer Planets
Lissauer, J. J. (2005) · Springer eBooks · doi:10.1007/1-4020-4038-5_2 · Cited by 12
Ксанфомалити, Л. В. (2004) · Solar System Research · doi:10.1023/b:sols.0000037465.72898.27 · Cited by 12
Formation of the Outer Planets
Lissauer, J. J. (2005) · Space Science Reviews · doi:10.1007/s11214-005-1945-3 · Cited by 13
Díaz, R. F., Ramírez, S., Fernández, J. M., Gallardo, J., Gieren, W., Ivanov, V. D., Mauas, P. J. D., Minniti, D., Pietrzyński, G., Perez, F., et al. (2007) · LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) · Cited by 12
Measuring accurate transit parameters
Winn, J. N. (2015) · Cited by 12
A search for the infrared spectroscopic signature of hot Jupiter planets
Lucas, P. W., & Roche, P. F. (2002) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2002.05786.x · Cited by 12
Fressin, F., Guillot, T., & Nesta, L. J. (2009) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200810097/pdf · Cited by 12
Rauer, H., & Erikson, A. (2007) · doi:10.1002/9783527621361.ch9 · Cited by 12
Forbrich, J., Berger, E., & Reid, M. J. (2016) · Cited by 12
Ephemeris refinement of 21 Hot Jupiter exoplanets with high timing uncertainties
Mallonn, M., von Essen, C., Herrero, E., Alexoudi, X., Granzer, T., Sosa, M. S., Strassmeier, K. G., Bakos, G. Á., Bayliss, D., Brahm, R., et al. (2019) · Open Research Online (The Open University) · doi:10.1051/0004-6361/201834194/pdf · Cited by 11
The bright star survey telescope for the planetary transit survey in Antarctica
Tian, Q., Jiang, P., Du, F., Wang, J., Li, Z., Li, X., Zhang, Z., Lu, H., Yuan, X., Liu, H.-G., et al. (2016) · 中国科学通报:英文版 · doi:10.1007/s11434-016-1015-0 · Cited by 11
Day and night side core cooling of a strongly irradiated giant planet
Budaj, J., Hubený, I., & Burrows, A. S. (2012) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201117975/pdf · Cited by 11
HOST STAR PROPERTIES AND TRANSIT EXCLUSION FOR THE HD 38529 PLANETARY SYSTEM
Henry, G. W., Kane, S. R., Wang, S. X., Boyajian, T. S., Braun, K., Henry, G. W., Kane, S. R., Wang, S. X., Wright, J. T., Boyajian, T. S., et al. (2013) · University of Southern Queensland ePrints (University of Southern Queensland) · Cited by 11
A hot Saturn on an eccentric orbit around the giant star K2-132
Jones, M. I., Brahm, R., Espinoza, N., Jordán, A., Rojas, F., Rabus, M., Drass, H., Zapata, A., Soto, M. G., Jenkins, J. S., et al. (2018) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201731478/pdf · Cited by 11
Gledhill, T. M., Sparks, W. B., Ulanowski, Z., Hough, J. H., & DasSarma, S. (2007) · Springer eBooks · doi:10.1007/978-1-4020-5502-7_6 · Cited by 11
Metadata
- Authors
- Charbonneau, D., Brown, T. M., Latham, D. W., & Mayor, M.
- Affiliations
- NSF National Center for Atmospheric Research (US)
- Center for Astrophysics Harvard & Smithsonian (US)
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2000-01-20
- Volume
- 529
- Issue
- 1
- Pages
- L45-L48
- ISSN
- 0004-637X (ISSN-L)
- OpenAlex
- W2151864661
- Cited by
- 1,415
- References
- 14
- Citations by year
- 2026: 25 · 2025: 44 · 2024: 48 · 2023: 50 · 2022: 42 · 2021: 36 · 2020: 60 · 2019: 50 · 2018: 60 · 2017: 54 · 2016: 55 · 2015: 42 · 2014: 39 · 2013: 56 · 2012: 49
- FWCI
- 48.04
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › History and Developments in Astronomy
- Keywords
- HD 209458, planetary transits, exoplanets, hot Jupiters, transit photometry, limb darkening, transit timing, orbital inclination, planetary radius, surface gravity, escape velocity, planet density, solar-type stars
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