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The radiance distribution of the star model is found to be of crucial importance, as deviations from a Lambertian radiance distribution can lead to significantly different results.<\/jats:p>","DOI":"10.1088\/1361-6552\/ad4c46","type":"journal-article","created":{"date-parts":[[2024,6,4]],"date-time":"2024-06-04T17:25:17Z","timestamp":1717521917000},"page":"045023","update-policy":"https:\/\/doi.org\/10.1088\/crossmark-policy","source":"Crossref","is-referenced-by-count":0,"title":["A radiometric model for demonstration of exoplanets detection by the transit method"],"prefix":"10.1088","volume":"59","author":[{"given":"T M","family":"Seixas","sequence":"first","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-7611-6056","authenticated-orcid":true,"given":"M A","family":"Salgueiro da Silva","sequence":"additional","affiliation":[]}],"member":"266","published-online":{"date-parts":[[2024,6,4]]},"reference":[{"key":"pedad4c46bib1","doi-asserted-by":"publisher","first-page":"355","DOI":"10.1038\/378355a0","article-title":"A Jupiter-mass companion to a solar-type star","volume":"378","author":"Mayor","year":"1995","journal-title":"Nature"},{"author":"Nasa Exoplanet Archive","key":"pedad4c46bib2"},{"key":"pedad4c46bib3","doi-asserted-by":"publisher","first-page":"296","DOI":"10.3390\/challe5020296","article-title":"The detection and characterization of extrasolar planets","volume":"5","author":"Rice","year":"2014","journal-title":"Challenges"},{"key":"pedad4c46bib4","doi-asserted-by":"publisher","first-page":"46","DOI":"10.1088\/0031-9120\/40\/1\/003","article-title":"An introductory physics exercise using real extrasolar planet data","volume":"40","author":"LoPresto","year":"2005","journal-title":"Phys. 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