User:Conci Furiram/Signature bands
Signature bands is an advanced method to speed up scanning a newly entered system. Before Odyssey, the method involved dropping a single Combat probe or a single Deep Space Probe and setting it at maximum range. This way still works, but CCP gave us a new way. This page will discuss both.
Throughout this page, refer to the tables summarized on swiftandbitter:
Probe method
Work-In-Progress
Distance method
When you first enter a system, you will see all the signatures in the system in your probe window. To explain the process, I will go through an example. Below is a screenshot of the signature list upon entering the WHC home system, J211936.
This system is known to have a Hi-sec static and a C3 static hole; we want to find them quickly. The C3 static is an O477 wormhole. Looking at the Wormhole Table, we can see it must be in the 7.33AU band. Since there is only one such signature system in the system, we immediately know ULD-686 is that wormhole. The Hi-sec wormhole, however, is a B274 and has to be in the 6.22AU band. There are two such signatures in system: ZTS-795 and SLE-584. We will have to scan both down to find which is the wormhole.
Also, since this is in wormhole space, the EKE-544 and AKE-140 signatures are most likely a Relic or Data site, or a valuable Vital or Instrumental Gas site. There is a small chance they could be a roaming wormhole, but those are rare.
Especially important for wormhole dwellers is the 6.22AU band: the K162 exit holes are in this band. Since they are such high band, they are easy to scan. When you are mapping a chain, your first signature to scan should be the hole's static, and then everything in the 6.22AU as some may be K162s.
The above image is the signatures in the example scanned to 100%. Note that ULD-686 was the C3 static and ZTS-795 was the Hi-sec static. The 7.33AU signatures were both Relic sites. The other 6.22AU signature was not a K162, but a low-end Minor Gas site.
