To: Dr. Brandon Wright IRG | From: Dr. Evan Chandler

[Morosz]

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Greetings. Here are the data you requested. If you have any questions this channel will remain open to you.
I took the freedom of marking the places where the anomaly appeared. Maybe you'Ll have more luck with it and will notice somekind of tendency or pattern. I might also remind you that theese are only the ones that the ship's scanners detected and logged. So we don't know if the anomaly only appears in theese systems or it appears in other ones as well. Since so far i was not able to predict where and when will the anomaly form. As i said i managed to get confirmation about the anomaly "syphoning" matter from the area where it forms. This evidence was collected in orbit of Planet Topeka when the anomaly formed deep within it's atmosphere. This was the only incident we managed to observe it from closer but still the interference caused by the planet's atmosphere left us once again with only a very little ammount of data but this confirmed my theory. The attachment will contain the data.


3D reconstruction extrapolated from the scannner data.
Link
The gravitational waves left behind by the anomaly.


Gravitational waves registered by the scanner in omicron Lost when we detected the anomaly.


Leftover radiation.


ATTACHMENT=:::::::::::::

If you have any questions this channel will remain open to you.

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[Stoner_Steve]

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-_-_-_-_-: Sender: Brandon Wright :-_-_-_-_-

Good Afternoon,

The data you have provided is certainly interesting but with only one object successfully identified within Planet Topeka I'm inclined to believe that these anomalies don't represent as large of a risk. However with the rise in appearance of the objects within Omicron Lost I'll authorize you funds for up to 25 million credits should you find, and successfully identify an object while it is formed and stable within the system. However Ingenuus lacks the resources at this time to dedicate its own science team to the project.

I look forward to hearing from you.

Brandon Wright
Ingenuus Research Group