Telecon Notes April 18, 2018
Attendance: Shaul, Dan, Bill, Charles, Nick, Amy
Notes by: Karl
Agenda
Github Repo
Report outline
;
Our Proposal
was arranged by science deliverables;
and so is the S4 science book.
Interesting Figure from Alex Van Engelen
Notes
Github Repo
Report outline, 50 page limit
Our Proposal was arranged by science deliverables; and so is the S4 science book.
Current outline follows working groups, science deliverables might make more sense.
CL: Organizing science around what drives the design. So grouping things slightly differently. Improves flow of science into mission design.
SH: So high frequency channels (galactic science) is one of these drivers.
CL: yes, OK. Make it clear.
CL: Extragalactic science includes some things that are more cosmological than astronomical object. Those could be separate. Minor detail.
CL: Complementarity also needs to be discussed.
SH: Jamie advocated a joint PICO-S4 or space-ground white paper to discuss complementarity.
CL: Attaching such a white paper would be effective for document to decadal.
Decision: Section 3 rearrange to science deliverables. Separate science drivers and non-driving science.
Also add ~0.5 page for complementarity with ground.
Shaul
will rearrange outline, so next week can discuss writing assignments and final those during workshop.
AT: TeamX slides status.
Instrument slides. Gave feedback, TeamX integrating comments.
Probably final iteration, before release to EC.
TeamX probably done in week timescale
Today reviewing Mission slides.
After these to rounds will release to EC.
Interesting Figure from Alex Van Engelen, for APS talk.
lensing potential, for EB estimator we seem to have lower noise. EB is the more effective estimator.
Bill: complementarity/competitiveness with S4 don't need to be mutually exclusive.
General discussion: Why does PICO do better? PICO has better E-mode measurement.
SH: Why S4 better at TT, PICO better at EB?
Dan: PICO beam means lose modes > ell 2000-ish. Lensing connects high ell to low, so those modes are valuable.
SH: Other new from science groups.
Nick estimates 140k SZ clusters; within ~10k of S4.
Nick also estimate 9 meV limit on neutrino mass. using cluster counts. dN/dz
SH: does this make sense?
Dan: If using growth of structure you can avoid the absolute calibration (tau) and potentially do better. Don't know if this is what he did.
SH: dN/dz also requires z, so more further work would be needed.
Nick: not doing that here, still tau limited.
Dan's 14 meV is also tau limited.
may be details in the calculations that account for this difference?
Nick
will look into the details. see if there is additional information being added by PICO.