20190329 Large Telescopes Telecon

From CMB-S4 wiki
Revision as of 12:28, 29 March 2019 by Niemack (talk | contribs)
Jump to navigationJump to search

On the call: Steve P, John R, Mike N

Discussion of how to prepare for flowdown and deal with plan of having different frequency distributions between the r survey and the legacy survey.

Agreement that it makes sense to remove 20 GHz optics tube from legacy survey; however, there is concern that anything we make changes to needs to also flow down through the detector array and readout costing.

Question: How are we going to converge on frequency bands?

Need to continue bringing this to the attention of ET and flowdown team. Will bring this up on DSR call this afternoon.