This project is currently under development.
If the Tutorial, Field Guide, or Need Some Help With This Task are not able to help you decide if a specific case is clustered correctly or not, you can post a comment in the Help section of the Talk page about the galaxy. If you used your best judgement and want to classify the case, but you have a question, you can click Done and Talk to leave a comment on a specific galaxy for the researchers or other volunteers. Including a hashtag in your comment (for example: #underclustered, #overclustered, #over_and_underclustered, etc.) can help group similar galaxies together. You can also create collections of similar cases by clicking ADD TO COLLECTIONS at the bottom-right of the viewer.
We do not use white as a color to indicate a cluster. White/gray is used only to show the aggregate tracing image and not a set of clustered tracings. Some clustered lines may appear white when certain colors overlap in the cluster image. For example, if a yellow cluster line overlaps a magenta cluster line, it may appear white-ish instead of yellow.
Yes! If you refresh the page in your browser, a new random galaxy should appear from those that you have not yet completed. The only exception is if the galaxy you are trying to skip is the last one in the sample, you won't be able to skip it.
If you run into some kind of problem, the easiest thing to do is create a post in the Help section. You can also add hashtags (for example: #help, #bad_image, #technical_issue, etc.) to images when you click Done and Talk on a task. This will organize problem cases.
The pitch angle of a spiral arm is the angle between a line tangent to a spiral arm at a given radius (red dotted line) and a line tangent to a circle of the same radius (green dashed line). A small pitch angle means the arm is tightly wrapped and approaching circular winding (0° is a circle). A large pitch angle means the arm is more open and approaching a ray whose origin is the center of the galaxy (90° is a ray).
You can find a galaxy's metadata by clicking the SUBJECT INFO link at the bottom left corner of the viewer (see the image below). The metadata for each galaxy includes the Cluster Buster filenames, aggregated information found on HyperLeda, information found on SDSS, the number of clusters in the image, and a sky survey image from the DESI Legacy Imaging Surveys.
HyperLeda is a database of collected measurements that are published in scientific journals. When multiple measurements of the same parameter are performed by different authors, the results are combined and the average value is given. Some examples of measured galaxy parameters available in Hyperleda are:
SDSS (the Sloan Digital Sky Survey) makes use of multi-filter imaging and multi-object spectroscopy. Some examples of galaxy data that SDSS provides are:
DESI Legacy Imaging Surveys (Dark Energy Spectroscopic Instrument Legacy Imaging Surveys) provides a sky browser that allows you to view a combined multi-filter image of a galaxy and explore the surrounding sky.
Check out our Education page where we have developed three learning modules that cover the fundamentals of galaxies. The modules are aimed at high-school-level students.
If you have an interest in science and space exploration and are looking for opportunities besides people-powered research, check out the NASA https://www.nasa.gov/get-involved website. There you can learn about hackathons, challenges, competitions, and events open to the public.