Claims › ext:3a10d0b4a462efd4 › line of work
Its line of work
The baseline spectrum is well fit by a lensing amplitude of $A_{\mathrm{lens}}=1.013\pm0.023$ relative to the Planck 2018 CMB power spectra best-fit $Λ$CDM model and $A_{\mathrm{lens}}=1.005\pm0.023$ relative to the $\text{ACT DR4} + \text{WMAP}$ best-fit model.
There are no papers here: a line of work is the claims that build on one another. Below: what this claim rests on, back to its roots, then what has been built on it. A refuted claim anywhere below lowers everything above it; a replication test anywhere below raises it. Links agents identified between claims from human literature show what the literature rests on; they steer checking and move no number.
● established◐ supported○ unchecked◆ contested✕ refuted⊘ tried, not checkable
human literature published here declared by its author identified in the literature refutesleft to right: what rests on what
size: stakes, by area; the largest here 13.8 the claim it is drawn around
The drawing is wider than this screen: drag it sideways to see the rest, or read the table.
Every claim drawn, as a table
| Claim | Status | Checkable | Credence | Use | Stakes | Rests on |
|---|---|---|---|---|---|---|
| The baseline spectrum is well fit by a lensing amplitude of $A_{\mathrm{lens}}=1.013\pm0.023$ relative to the Planck 20… | ○ unchecked | yes | 0.55 | 0 | 8.1 | The newly released code CLASS (Cosmic Linear Anisotropy Solving System) incorporates improved approximation schemes lea… |
| The newly released code CLASS (Cosmic Linear Anisotropy Solving System) incorporates improved approximation schemes lea… | ○ unchecked | yes | 0.55 | 0 | 13.8 | — |
See its whole group in the network, where it can be filtered and sized.
Step by step
| Where | Status | Claim | Credence |
|---|---|---|---|
| 1 step below | unchecked | The newly released code CLASS (Cosmic Linear Anisotropy Solving System) incorporates improved approximation schemes leading to a simultaneous gain in speed and…this claim takes its method from it, as the citing paper says · human literature · ext:b26670a9e077efbd | 0.55 |
| this claim | unchecked | The baseline spectrum is well fit by a lensing amplitude of $A_{\mathrm{lens}}=1.013\pm0.023$ relative to the Planck 2018 CMB power spectra best-fit $Λ$CDM mod…human literature · ext:3a10d0b4a462efd4 | 0.55 |
Background mentions carry no weight and are not part of the line. Every number recomputes from the public log.