This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
This product includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA's Science Mission Directorate. https://doi.org/10.1117/1.JATIS.1.1.014003 Retrieved using pylightkurve tool.
C11EdgeHD SCT, ST8XME, & G11 GEM Rc filter, 2 star ensemble, mostly clear sky. Image exposures 10 sec then data averaged 5x to reduce noise. Hot Jupiter planet with longer 21.2 day period orbit.
SW ED 80/600, Atic 16 IC, AG by MMys na SW 80/400 Hraní si s daty - soubor dat jsem postupně zmergoval snímky po 2, 3, 4, 5, 6, 7 a 8mi, prohnal fitovátkem, výsledek jsem nechal zprůměrovat pomocí fittool a výsledek je překvapivý, ale otázka, nakolik reálný. DQ 3, TminHJD = 2455817.55399 +/- 0.00107
RL200, f/6 + ST8, guider RF80/600+G1-0300 1min binned data, average of 3 different aperture size light curves, decrease et end of original data removed
SW ED 80/600, Atic 16 IC, AG by MMys na SW 80/400 Poměrně čistá obloha, ale hodně rušil Měsíc, FWHM kolem 9, expozice 40 s, průměrná křivka z individuálně detrendovaných křivek s 6 porovnávacími hvězdami s různými aperturami, Při použití mergování klesla přesnost určení délky a hloubky minima, DQ 4, TminHJD = 2455817.556 +/- 0.00226
SW ED 80/600, Atic 16 IC, AG by MMys na SW 80/400 Poměrně čistá obloha, ale hodně rušil Měsíc, FWHM kolem 9, expozice 40 s, průměrná křivka z individuálně detrendovaných křivek s 6 porovnávacími hvězdami s různými aperturami, Při použití mergování klesla přesnost určení délky a hloubky minima, ale byl by menší rozptyl bodů.
