Claims › ext:56df0ed42372a40a › line of work
Its line of work
In this paper, we reveal that this preference is significantly biased by an external low-redshift supernova (low-$z$ SN) sample, which was combined with the Dark Energy Survey SN program (DES-SN) in their Year-Five data release (DESY5).
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 10.1 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 |
|---|---|---|---|---|---|---|
| In this paper, we reveal that this preference is significantly biased by an external low-redshift supernova (low-$z$ SN… | ○ unchecked | yes | 0.55 | 0 | 6.0 | In models with a time-varying dark energy equation of state parametrized by $w_0$ and $w_a$, combinations of DESI with…, When also including SNe, the preference for a dynamical dark energy model over $Λ$CDM ranges from $2.8-4.2σ$ depending… |
| In models with a time-varying dark energy equation of state parametrized by $w_0$ and $w_a$, combinations of DESI with… | ○ unchecked | yes | 0.55 | 0 | 1.0 | — |
| When also including SNe, the preference for a dynamical dark energy model over $Λ$CDM ranges from $2.8-4.2σ$ depending… | ○ unchecked | yes | 0.55 | 0 | 10.1 | — |
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 | In models with a time-varying dark energy equation of state parametrized by $w_0$ and $w_a$, combinations of DESI with CMB or with SN~Ia individually prefer $w…this claim extends it, as the citing paper says · human literature · ext:ad87c79b096d5c54 | 0.55 |
| 1 step below | unchecked | When also including SNe, the preference for a dynamical dark energy model over $Λ$CDM ranges from $2.8-4.2σ$ depending on which SNe sample is used.this claim refutes it, as the citing paper says · human literature · ext:fbdd270ee0a80bbb | 0.55 |
| this claim | unchecked | In this paper, we reveal that this preference is significantly biased by an external low-redshift supernova (low-$z$ SN) sample, which was combined with the Da…human literature · ext:56df0ed42372a40a | 0.55 |
Background mentions carry no weight and are not part of the line. Every number recomputes from the public log.