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Equation 19 · A Neutron Star Is a Redshift Standard

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z=0.35z=0.35

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Inputs and operations0.35
Result or conditionz
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zz

Symbol z

z is part of the quantity the equation computes from the expression on the right.

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=

=

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The closest anyone came to this measurement, decades before NICER existed, was Jean Cottam, Frits Paerels, and Mariano Mendez’s 2002 analysis of the bursting neutron star EXO 0748-676. Stacking twenty-eight thermonuclear X-ray bursts observed with the Chandra grating spectrometer, they reported narrow absorption features matching iron and oxygen transitions, all consistent with a single redshift of z=0.35 — a clean, quantitative result, and for several years the field’s best evidence that a neutron-star surface line could actually be resolved [ 5 ] . The claim implied a star built from ordinary nuclear matter, in a mass range of roughly 1.3 to 2.0 solar masses, and it was treated for most of…
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The closest anyone came to this measurement, decades before NICER existed, was Jean Cottam, Frits Paerels, and Mariano Mendez’s 2002 analysis of the bursting neutron star EXO 0748-676. Stacking twenty-eight thermonuclear X-ray bursts observed with the Chandra grating spectrometer, they reported narrow absorption features matching iron and oxygen transitions, all consistent with a single redshift of z=0.35 — a clean, quantitative result, and for several years the field’s best evidence that a neutron-star surface line could actually be resolved [ 5 ] . The claim implied a star built from ordinary nuclear matter, in a mass range of roughly 1.3 to 2.0 solar masses, and it was treated for most of a decade as the field’s proof of concept.

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