NGC 5927Ā is aĀ globular clusterĀ in theĀ constellationĀ Lupus.
The globular cluster was discovered by James Dunlop in 1826 and was also observed in 1834 by John Herschel. NGC 5927 has a diameter of about 12 arc mins and an apparent magnitude of +8.86.
Observation
I collected 15 images from Skynet, of this cluster using telescopes PROMPT-MO-1, Prompt5, and Prompt6. The pictures were taken with the B filter using an exposure time of 141.73s, with the V filter using a length of 94.49s, and the R filter using a length of 70.87s. The picture below is the pictures using the three filters via Afterglow Workbench. This is an apparent tri-color image of NGC 5927.
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To form an apparent image of my cluster:
And now I reddened it.
Primary Results via Astronomicon
Using the Astronomicon website I could find the following primary observations about my cluster:
Analysis
Analyzing this Cluster was very tough, but I did find some interesting stuff looking into the nature of NGC 5927. I noticed a lot of blue stragglers, and more while analyzing this cluster. It is a very very old cluster, a ancient one, and was very hard for me to figure out during this stage. During Isochrone matching, it was very difficult for me to find something that worked, the data was almost impossible to use for me, so I believe I made an error, but this is the best I got:
Via Kharchenko et. al, I believe I found his values within sheet number 2425:
Conclusion:
In conclusion, I am not very happy with the results of my studies/research. The cluster was very difficult for me, and almost everything went wrong while analyzing this cluster. I learned a lot about blue stragglers though, and applied that on my exam as well. I believe with more time, I could figure out every error with this blog post, but other than that I did the best I could.