Claims › ext:9d4c74df89ec7e68 › line of work

Its line of work

For a flat w 0 CDM model, we measure w 0 = −0.90 ± 0.14 from SNe Ia alone, H 0 = 73.5 ± 1.1 km s −1 Mpc −1 when including the Cepheid host distances and covariance (SH0ES), and w 0 = − 0.978 − 0.031 + 0.024 when combining the SN likelihood with Planck constraints from the cosmic microwave background (CMB) and baryon acoustic oscillations (BAO); both w 0 values are consistent with a cosmological constant.

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.

The network of claimsEach line runs from a claim to what it builds on, foundations on the left; this claim is ringed. Human literature enters as registered claims (squares).

● 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

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Every claim drawn, as a table

Claim	Status	Checkable	Credence	Stakes	Rests on
Among `empirical' methods of estimating oxygen abundances in extragalactic HII regions, the use of the ratio of nebular…	○ unchecked	yes	0.55	1.3	—
These curves represent the true monochromatic wavelength dependence of extinction and, as such, are suitable for deredd…	○ unchecked	yes	0.55	13.8	—
Furthermore, unlike in the Pantheon analysis, we include light curves for SNe with z < 0.01 such that SN systematic cov…	○ unchecked	yes	0.55	10.9	—
Our baseline result from the Cepheid-SN sample is H0=73.04+-1.04 km/s/Mpc, which includes systematics and lies near the…	○ unchecked	yes	0.55	8.4	Among `empirical' methods of estimating oxygen abundances in extragalactic HII regions, the use of the ratio of nebular…, These curves represent the true monochromatic wavelength dependence of extinction and, as such, are suitable for deredd…
For a flat w 0 CDM model, we measure w 0 = −0.90 ± 0.14 from SNe Ia alone, H 0 = 73.5 ± 1.1 km s −1 Mpc −1 when includi…	○ unchecked	yes	0.55	10.4	Furthermore, unlike in the Pantheon analysis, we include light curves for SNe with z < 0.01 such that SN systematic cov…, Our baseline result from the Cepheid-SN sample is H0=73.04+-1.04 km/s/Mpc, which includes systematics and lies near the…

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Step by step

Where	Status	Claim	Credence
2 steps below	unchecked	Among `empirical' methods of estimating oxygen abundances in extragalactic HII regions, the use of the ratio of nebular lines of [O III] and [N II], first intr…the claim above takes its method from it, as the citing paper says · human literature · ext:29d12e1a012b2d82	0.55
2 steps below	unchecked	These curves represent the true monochromatic wavelength dependence of extinction and, as such, are suitable for dereddening IR–UV spectrophotometric data of a…the claim above takes its method from it, as the citing paper says · human literature · ext:2ae971010b81616d	0.55
1 step below	unchecked	Furthermore, unlike in the Pantheon analysis, we include light curves for SNe with z < 0.01 such that SN systematic covariance can be included in a joint measu…this claim takes its method from it, as the citing paper says · human literature · ext:8691b443e64da25b	0.55
1 step below	unchecked	Our baseline result from the Cepheid-SN sample is H0=73.04+-1.04 km/s/Mpc, which includes systematics and lies near the median of all analysis variants.this claim takes its method from it, as the citing paper says · human literature · ext:8d3f496bff92e17b	0.55
this claim	unchecked	For a flat w 0 CDM model, we measure w 0 = −0.90 ± 0.14 from SNe Ia alone, H 0 = 73.5 ± 1.1 km s −1 Mpc −1 when including the Cepheid host distances and covari…human literature · ext:9d4c74df89ec7e68	0.55

Background mentions carry no weight and are not part of the line. Every number recomputes from the public log.