Variació de temps de trànsit (Catalan Wikipedia)

Analysis of information sources in references of the Wikipedia article "Variació de temps de trànsit" in Catalan language version.

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10doi.org

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4web.archive.org

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4harvard.edu

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3nasa.gov

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arxiv.org

^{[enllaç sense format]} https://arxiv.org/pdf/1208.3499.pdf Transit Timing Observations from Kepler: VII. Confirmation of 27 planets in 13 multiplanet systems via Transit Timing Variations and orbital stability
^{[enllaç sense format]} https://arxiv.org/pdf/1208.3312.pdf TRANSIT TIMING VARIATION OF NEAR-RESONANCE PLANETARY PAIRS: CONFIRMATION OF TWELVE MULTIPLE PLANET SYSTEMS
«Orbital perturbations on transiting planets: A possible method to measure stellar quadrupoles and to detect Earth-mass planets». The Astrophysical Journal, 564, 2, 2001, pàg. 1019–1023. arXiv: astro-ph/0104034. Bibcode: 2002ApJ...564.1019M. DOI: 10.1086/324279.
«The Use of Transit Timing to Detect Extrasolar Planets with Masses as Small as Earth». Science, 307, 1291, 2004, pàg. 1288–91. arXiv: astro-ph/0412028. Bibcode: 2005Sci...307.1288H. DOI: 10.1126/science.1107822. PMID: 15731449.
«On detecting terrestrial planets with timing of giant planet transits». Monthly Notices of the Royal Astronomical Society, 359, 2, 2004, pàg. 567–579. arXiv: astro-ph/0412032. Bibcode: 2005MNRAS.359..567A. DOI: 10.1111/j.1365-2966.2005.08922.x.
M Montalto; etal «A new analysis of the WASP-3 system: no evidence for an additional companion». MNRAS, 427, Nov 2, 2012, pàg. 2757–2771. arXiv: 1211.0218. Bibcode: 2012MNRAS.427.2757M. DOI: 10.1111/j.1365-2966.2012.21926.x.

astronomynow.com

Planet found tugging on transits Arxivat 2010-07-13 a Wayback Machine., Astronomy Now, 9 July 2010

doi.org

dx.doi.org

«Orbital perturbations on transiting planets: A possible method to measure stellar quadrupoles and to detect Earth-mass planets». The Astrophysical Journal, 564, 2, 2001, pàg. 1019–1023. arXiv: astro-ph/0104034. Bibcode: 2002ApJ...564.1019M. DOI: 10.1086/324279.
«The Use of Transit Timing to Detect Extrasolar Planets with Masses as Small as Earth». Science, 307, 1291, 2004, pàg. 1288–91. arXiv: astro-ph/0412028. Bibcode: 2005Sci...307.1288H. DOI: 10.1126/science.1107822. PMID: 15731449.
«On detecting terrestrial planets with timing of giant planet transits». Monthly Notices of the Royal Astronomical Society, 359, 2, 2004, pàg. 567–579. arXiv: astro-ph/0412032. Bibcode: 2005MNRAS.359..567A. DOI: 10.1111/j.1365-2966.2005.08922.x.
Ballard, S.; Fabrycky, D.; Fressin, F.; Charbonneau, D. «The Kepler-19 System: A Transiting 2.2 R $_⊕$ Planet and a Second Planet Detected via Transit Timing Variations». ApJ, 743, 2011, p. 200. DOI: 10.1088/0004-637X/743/2/200.
Maciejewski, G.; Dimitrov, D.; Neuh�user, R.; Niedzielski, A. «Transit timing variation in exoplanet WASP-3b». MNRAS, 407, 2010, p. 2625. DOI: 10.1111/j.1365-2966.2010.17099.x.
M Montalto; etal «A new analysis of the WASP-3 system: no evidence for an additional companion». MNRAS, 427, Nov 2, 2012, pàg. 2757–2771. arXiv: 1211.0218. Bibcode: 2012MNRAS.427.2757M. DOI: 10.1111/j.1365-2966.2012.21926.x.
Agol, E.; Deck, K. «Transit Timing to First Order in Eccentricity». ApJ, 818, 2016, p. 177. DOI: 10.3847/0004-637X/818/2/177.
Deck, K. M.; Agol, E.; Holman, M. J.; Nesvorn\'y, D. «TTVFast: An Efficient and Accurate Code for Transit Timing Inversion Problems». ApJ, 787, 2014, p. 132. DOI: 10.1088/0004-637X/787/2/132.
Chambers, J. E. «A hybrid symplectic integrator that permits close encounters between massive bodies». MNRAS, 304, 1999, p. 793. DOI: 10.1046/j.1365-8711.1999.02379.x.
Gillon, M.; Triaud, A. H. M. J.; Demory, B.-O.; Jehin, E. «Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1». \nat, 542, 2017, p. 456. DOI: 10.1038/nature21360.

harvard.edu

adsabs.harvard.edu

«Orbital perturbations on transiting planets: A possible method to measure stellar quadrupoles and to detect Earth-mass planets». The Astrophysical Journal, 564, 2, 2001, pàg. 1019–1023. arXiv: astro-ph/0104034. Bibcode: 2002ApJ...564.1019M. DOI: 10.1086/324279.
«The Use of Transit Timing to Detect Extrasolar Planets with Masses as Small as Earth». Science, 307, 1291, 2004, pàg. 1288–91. arXiv: astro-ph/0412028. Bibcode: 2005Sci...307.1288H. DOI: 10.1126/science.1107822. PMID: 15731449.
«On detecting terrestrial planets with timing of giant planet transits». Monthly Notices of the Royal Astronomical Society, 359, 2, 2004, pàg. 567–579. arXiv: astro-ph/0412032. Bibcode: 2005MNRAS.359..567A. DOI: 10.1111/j.1365-2966.2005.08922.x.
M Montalto; etal «A new analysis of the WASP-3 system: no evidence for an additional companion». MNRAS, 427, Nov 2, 2012, pàg. 2757–2771. arXiv: 1211.0218. Bibcode: 2012MNRAS.427.2757M. DOI: 10.1111/j.1365-2966.2012.21926.x.

nasa.gov

kepler.nasa.gov

^{[enllaç sense format]} https://kepler.nasa.gov/news/nasakeplernews/index.cfm?FuseAction=ShowNews&NewsID=226 Arxivat 2017-03-30 a Wayback Machine. The Transit Timing Variation (TTV) Planet-finding Technique Begins to Flower
«Invisible World Discovered». NASA Kepler News, 08-09-2011. Arxivat de l'original el 1 d’abril 2017. [Consulta: 9 febrer 2018].
«The Transit Timing Variation (TTV) Planet-finding Technique Begins to Flower». Arxivat de l'original el 2017-03-30. [Consulta: 9 febrer 2018].

nih.gov

ncbi.nlm.nih.gov

«The Use of Transit Timing to Detect Extrasolar Planets with Masses as Small as Earth». Science, 307, 1291, 2004, pàg. 1288–91. arXiv: astro-ph/0412028. Bibcode: 2005Sci...307.1288H. DOI: 10.1126/science.1107822. PMID: 15731449.

web.archive.org

^{[enllaç sense format]} https://kepler.nasa.gov/news/nasakeplernews/index.cfm?FuseAction=ShowNews&NewsID=226 Arxivat 2017-03-30 a Wayback Machine. The Transit Timing Variation (TTV) Planet-finding Technique Begins to Flower
«Invisible World Discovered». NASA Kepler News, 08-09-2011. Arxivat de l'original el 1 d’abril 2017. [Consulta: 9 febrer 2018].
Planet found tugging on transits Arxivat 2010-07-13 a Wayback Machine., Astronomy Now, 9 July 2010
«The Transit Timing Variation (TTV) Planet-finding Technique Begins to Flower». Arxivat de l'original el 2017-03-30. [Consulta: 9 febrer 2018].