An anonymous reader writes “Have access to a telescope with a CCD? Now you can make your very own exoplanet transit curves. Brett Morris, a student from the University of Maryland, has written an open source photometry application known as Oscaar. In a recent NASA Press Release, Morris writes: “The purpose of a differential photometry code – the differential part – is to compare the changes in brightness of one star to another nearby. That way you can remove changes in stellar brightness due to the Earth’s atmosphere. Our program measures the brightness change of all the stars in the telescope’s field of view simultaneously, so you can pull out the change in brightness that you see from the planet-hosting star due to the transit event.” The program opens up exoplanet-observing to amateur astronomers and undergraduate students across the globe.”… An anonymous reader writes “Have access to a telescope with a CCD? Now you can make your very own exoplanet transit curves. Brett Morris, a student from the University of Maryland, has written an open source photometry application known as Oscaar. In a recent NASA Press Release, Morris writes: “The purpose of a differential photometry code – the differential part – is to compare the changes in brightness of one star to another nearby. That way you can remove changes in stellar brightness due to the Earth’s atmosphere. Our program measures the brightness change of all the stars in the telescope’s field of view simultaneously, so you can pull out the change in brightness that you see from the planet-hosting star due to the transit event.” The program opens up exoplanet-observing to amateur astronomers and undergraduate students across the globe.”

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