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VIM is a tool for researching multiple sky positions simultaneously. Each source becomes a row in a table, with catalog, image cutouts, and spectral information. This information is drawn from all the published surveys of the astronomical literature. |
Example 1: Looking at existing workbenchs
Example 2: Finding out who is observing a given set of targets
Example 3: Checking what photometry NED has for a set of sources.
Example 4: A color-color-color plot from the join of GSC and USNO-B
6 Bright Galaxies and its script
90 Bright Arp galaxies and its script
51 Xray binaries and its script
148 matched SDSS and 2MASS and its script
47 rich Abell clusters and its script
Developed with the support of the National Science Foundation This NVO Application is hosted by Caltech |
Meet the Developers![]() |