Prompt 1
Please update cmb_derivation.md
Prompt 2
Starting a new session can be mildly frustrating as the new instantiation of you gets up to speed. I want to make sure YOU will be able to spin up quickly with the perspective needed to continue this work.
When this session began, there was lots of targeted detail to get you up to speed and familiar with our cmb work, in the handoff and startup files. It’s probably mostly still useful and just needs to have the work in this session included.
There should be continuing information on how to update the manuscript, the location of the project public git repo with the manuscript and support files and instructions that should allow for updating and script auditing. Those are important. Leave or update them.
Please make sure that just the parts of CG and VR that needed to be read to bring the next session up to speed are noted, instead of it having to inefficiently read the whole documents.
Make sure startup, handoff, and vr, accurately capture the state of the project after this and previous sessions. Can you audit and look for legacy, obsolete, or contradictory information that should probably be moved to investigation history?
Prompt 3
Please doublecheck handoff and startup for legacy, obsolete, contradictory, or other errors.
Prompt 4
Please doublecheck vr for legacy, obsolete, contradictory, or other errors.
Prompt 5
The global CMB operator we determined this session, and its subsequently derived channel operators is probably at or near the geometric floor of matching to Planck data. It is important that the derivation of this operator is captured in VR, and as appropriate in CG, and of course in cmb_derivation.md
Prompt 6
In our next session we will be comparing to other datasets besides Planck, such as SPT or ACT. These datasets may only have binned data available. If that’s the case, we need to adapt the operators accordingly for each dataset compared. We may also continue to see if we can find any components the current Global Operator is missing, so full development theory via links to documents to read needs to be passed on to session 11.
We also will soon be preparing to download TOD data from the ESA Planck Legacy servers and create a non LCDM processed Planck dataset to then compare UDT to LCDM and if our previous results become even stronger with perhaps UDT replacing LCDM with the better fit. That may or may not happen during session 11. Session 11 may also include tightening up the BAO, and SNe operators to update the manuscript.
Prompt 7
There is a file in the root containing the prompt to initiate session 10. Please write a new prompt file for initiating session 11.
Prompt 8
Using the new session 11 prompt from the file, put yourself in the position and mindset of an empty new instance. Follow the prompt through all the instructions and see if there are any contradictions, issues with obsolete material, or any other issues in getting up to speed.
Prompt 9
Repeat the previous dress rehearsal.
Prompt 10
repeat the dress rehearsal.
Prompt 11
/exit
Final
then you can reboot.