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What is a good figure of merit or a key plot (though maybe we need more than one) for dark matter astrophysical probes that we can show in all the conferences we go to? If we do have a money plot, wha…
yymao updated
5 years ago
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Hi there,
I've been using CLASS to calculate linear matter power spectrum for NCDM species. However, for some of my NCDM distribution functions, I got really weird results (see below).
This is the…
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baijin
a super-hazmat suit that uses chalcogenide deca-hydride, which is a compression level of super-hydrides, superconductor materials to reduce radiation penetration
Huhhila
Thought current ha…
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For some of these I have no idea why labs finds a wrong record.
Also listed in https://app.asana.com/0/3003451971699/620773521680386
Each example is given as
recid:[recid] (type of record)
…
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Hi,
I was upgrading class version for some data analysis that requires high accuracy at high ell.
I find significant differences for lensed TT, TE and EE spectra and for lensing potential power …
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### Team Name:
QuantumRing
### Project Description:
Neutrino Oscillation which was first predicted by Bruno Pontecorvo in 1957, has been a great theoretical and experimental i…
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### Team Name:
QuantumRing
### Project Description:
Neutrino Oscillation which was first predicted by Bruno Pontecorvo in 1957, has been a great theoretical and experimental interest, as its…
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# Description
Reporting a weird problem, where sometimes during training/inferring the program throws an error, which is logged to stdout, but does not crash entirely, instead it freezes and can be q…
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Shift antineutrino energy binning by E_thresh for IBD calculations (ES calculations remain unchanged).
Start first bin at E_thresh (Ev_IBD[0] = E_thresh + .005 MeV)
Retain 10 keV bin width (Ev_IBD…
stdye updated
2 years ago
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The following lists the ratio of rates for the two IBD cross sections (SV03 and VB99) for each energy bin. The last two lines give the totals: Web rate, Steve rate, difference(Web-Steve).
The ratio…
stdye updated
3 years ago