JWST observations confirm a constant-slope mass-metallicity relation for high-redshift dwarf galaxies down to 10^6.3 solar masses with no clear fundamental metallicity relation.
eprint arXiv:1909.11681 , year =
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Cosmographic constraints from 106 FRBs on H0, q0, j0 depend sensitively on whether a Gaussian or quasi-Gaussian PDF is assumed for DM_IGM and on whether the baryon mass fraction is fixed or free.
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Revisiting the mass metallicity relation and the fundamental metallicity relation of dwarf galaxies at cosmic noon with NIRISS
JWST observations confirm a constant-slope mass-metallicity relation for high-redshift dwarf galaxies down to 10^6.3 solar masses with no clear fundamental metallicity relation.
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The impact of FRB dispersion measure probability distribution functions on cosmographic estimates
Cosmographic constraints from 106 FRBs on H0, q0, j0 depend sensitively on whether a Gaussian or quasi-Gaussian PDF is assumed for DM_IGM and on whether the baryon mass fraction is fixed or free.