Claims › ext:2ae971010b81616d › line of work

Its line of work

These curves represent the true monochromatic wavelength dependence of extinction and, as such, are suitable for dereddening IR–UV spectrophotometric data of any resolution and can be used to derive extinction relations for any photometry system.

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

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	Stakes	Rests on
The Cepheid luminosity (P=10d, solar-metallicity) in the HST near-infrared, Wesenheit system derived from the cluster s…	○ unchecked	yes	0.55	6.7	These curves represent the true monochromatic wavelength dependence of extinction and, as such, are suitable for deredd…
These curves represent the true monochromatic wavelength dependence of extinction and, as such, are suitable for deredd…	○ unchecked	yes	0.55	13.8	—
For a flat ΛCDM model, we find Ω M = 0.334 ± 0.018 from SNe Ia alone.	○ unchecked	yes	0.55	10.4	These curves represent the true monochromatic wavelength dependence of extinction and, as such, are suitable for deredd…
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	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	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
this claim	unchecked	These curves represent the true monochromatic wavelength dependence of extinction and, as such, are suitable for dereddening IR–UV spectrophotometric data of a…human literature · ext:2ae971010b81616d	0.55
1 step above	unchecked	The Cepheid luminosity (P=10d, solar-metallicity) in the HST near-infrared, Wesenheit system derived from the cluster sample is M_{H,1}^W=-5.902+/-0.025 and -5…takes its method from this claim, as the citing paper says · human literature · ext:26fa189cf48f7a81	0.55
1 step above	unchecked	For a flat ΛCDM model, we find Ω M = 0.334 ± 0.018 from SNe Ia alone.takes its method from this claim, as the citing paper says · human literature · ext:80f3f151f291c7d8	0.55
1 step above	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.takes its method from this claim, as the citing paper says · human literature · ext:8d3f496bff92e17b	0.55
2 steps above	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…takes its method from the claim below, as the citing paper says · 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.