Introduction
An astronomer wants to ascertain whether a supernova candidate is Type Ia or Type II. Determining galaxy redshift and morphology of the environment in which the supernova candidate was discovered will aid classification.
Flow of Events
First, the astronomer searches the resource catalogue for optical or IR image data catalogues covering known supernova positions. The astronomer selects a catalogue from the returned list and requests images from the catalogue, based on position. The astronomer then acquires recent observations of the same location (in the same wavelength) from a telescope resource. The new observation image is uploaded onto Astrogrid; it is subtracted from the old image, creating a new subtracted image. The astronomer then uploads an algorithm to check the new image for objects that have moved between the first and second observation; these objects are eliminated as near Earth objects. Finally, a catalogue is generated of the remaining supernova candidates.
Sequence Diagram
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