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| en:praktikum:versuche_bachelor [2022/06/03 16:28] – [C1: Deep Sky Imaging] fruenger | en:praktikum:versuche_bachelor [2024/09/19 10:12] (current) – [C7: Light curve of an eclipsing binary star] rhainich |
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| \begin{equation*} | \begin{equation*} |
| I(\mu) = \frac{3}{5}\left(\cos{(\mu)}+\frac{2}{3}\right)\qquad | I(\mu) = \frac{3}{5}\left(\mu+\frac{2}{3}\right)\qquad |
| \end{equation*} | \end{equation*} |
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| ++++ Data reduction | | ++++ Data reduction | |
| | Please ask a lab course instructor for help. |
| | /* |
| Use the prepared [[en:praktikum:gdl|GDL]] scripts, which can be found at the [[en:praktikum:zugang |laboratory course computer]] (also see details of the [[en:praktikum:namenskonvention |name convention for files]]), to reduce the data photometrically. There are two scripts that do the principal data reduction (1_reduce_images.pro), the read-out, and the plotting of the photometry (2_obtain_flux.pro). Copy them to your local directory and adjust the names of the paths and the date of the current minimum. Compile and run the scripts with [[en:praktikum:gdl |GDL]] to obtain the light curve of the eclipsing binary star, which can be completed using archive data. | Use the prepared [[en:praktikum:gdl|GDL]] scripts, which can be found at the [[en:praktikum:zugang |laboratory course computer]] (also see details of the [[en:praktikum:namenskonvention |name convention for files]]), to reduce the data photometrically. There are two scripts that do the principal data reduction (1_reduce_images.pro), the read-out, and the plotting of the photometry (2_obtain_flux.pro). Copy them to your local directory and adjust the names of the paths and the date of the current minimum. Compile and run the scripts with [[en:praktikum:gdl |GDL]] to obtain the light curve of the eclipsing binary star, which can be completed using archive data. |
| | */ |
| ++++ | ++++ |
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