zenodoopen
Swift/UVOT observation of NGC 1566 in 2012 and 2018
<p>This figure shows the brightening of the central active galactic nucleus of NGC 1566 as observed by the Neil Gehrels Swift observatory UVOT instrument between 2018-06-24 (left) and 2012-10-09 (right). A brightening in the UW2 magnitude from 15.35 in 2012 to 12.48 in 018 is measured (ucertainties of 0.01- 0.02 magnitudes). </p>
ShareScore
44/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 8
- Harmonization
- 4
- Access
- 20
- Reuse readiness
- 8
- Engagement
- 4
Topics
Dataset details
- Repository
- zenodo
- Published
- June 26, 2018
- License
- cc-by-4.0
- DOI
- 10.5281/zenodo.1298991
Scored with release 0.9.0
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