GNU Astronomy Utilities - Tasks: task #14167, Calculating the upper limit...
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task #14167: Calculating the upper limit magnitude for each detection
Submitter: | Mohammad Akhlaghi <makhlaghi> | ||
Submitted: | Thu 29 Sep 2016 01:50:33 PM UTC | ||
Should Start On: | Wed 28 Sep 2016 03:00:00 PM UTC | Should be Finished on: | Wed 28 Sep 2016 03:00:00 PM UTC |
Category: | MakeCatalog | Priority: | 7 - High |
Item Group: | New feature | Status: | Done |
Privacy: | Public | Assigned to: | makhlaghi |
Percent Complete: | 100% | Open/Closed: | Closed |
Effort: | 0.00 |
Sun 02 Oct 2016 10:43:56 PM UTC, comment #1: |
Mohammad Akhlaghi <makhlaghi> |
Thu 29 Sep 2016 01:50:33 PM UTC, original submission:
One very important factor in measuring the magnitude of an object is this: what is the faintest acceptable magnitude for a given object (segmentation map) in an image? This depends on various things like the depth of the image, image correlated noise, or the shape and size of the object.
|
Mohammad Akhlaghi <makhlaghi> |
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Follow 3 latest changes.
Date | Changed by | Updated Field | Previous Value | => | Replaced by |
---|---|---|---|---|---|
2016-10-02 | makhlaghi | Status | In Progress | Done | |
Percent Complete | 70% | 100% | |||
Open/Closed | Open | Closed |
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