What next? Discipline: Education Now that you have the basics of photometry down you are ready to try several projects: Observing Open Clusters and Making H-R Diagrams How to Make a Light Curve for an Exoplanet Observing Supernovae Observing Variable Stars Tags: photometrySalsaJ
How to Use SalsaJ for Photometry Discipline: Education SalsaJ (Until further notice, please download version 1.4, not version 2.0, which does not yet have full photometry features.) and APT (Aperture Photometry Tool) are both free java based photometry software packages you can install on your computer to use for this project and any project that uses photometry. SalsaJ is a bit simpler and does more Tags: photometrySalsaJradius
Photometry of an Exoplanet Transit with SalsaJ Discipline: Education Download SalsaJ from the European Hands On Universe Website. (Until further notice, please download version 1.4, not version 2.0, which does not yet have full photometry features.)Launch SalsaJ and download our lightcure plotter spreadsheet ( you will need a spreadsheet application such as Excel, OpenOffice Spreadsheet or Numbers).Download and unzip sample data for one of the extrasolar planets below:Tags: transitexoplanetsphotometrySalsaJ
How to Make a Light Curve for an Exoplanet Transit Discipline: Education This guide describes how to create a light curve for an exoplanet transit by measuring the brightness of the target star and a comparison star in several frames. You can do this with sample data available from the Faulkes Telescopes, or with data from your own observation if you have an account. After doing this activity you should be able to: Tags: exoplanetsphotometrySalsaJ
Photometry of Star Clusters with SalsaJ Discipline: Education Download SalsaJ from the Hands On Universe Website. Launch SalsaJ. Tags: open clustersphotometrySalsaJ
Photometry to Find the Color of a Star Discipline: Education Photometry is the measurement of the intensity or brightness of an astronomical object, such as a star or galaxy by adding up all of the light from the object. For example, a star looks like a point of light when you look at it just with your eyes but the Earth’s atmosphere smears it out into something that looks like a round blob when you use a telescope to look at it. In order to measure the total light coming from the star, we must add up all of the light from the smeared out star. Photometry is generally used to generate light curves of objects such as variable stars andTags: photometrySalsaJ