Stacked DESI-LRG spectra yield a cosmographic H(z) curve from z=0.36 to 0.80 and two direct cosmic-chronometer measurements, including H(z≈0.61)=88.5^{+6.7}_{-12.6}±8.1 km/s/Mpc.
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6 Pith papers cite this work. Polarity classification is still indexing.
6
Pith papers citing it
representative citing papers
75% of massive compact quiescent galaxies at z~0 require three-component photometric models (bulge + disk + envelope), versus only 7% of mass-matched control quiescent galaxies.
Interstellar calcium and sodium absorption in MaStar is modeled and removed, yielding corrected spectra and simple stellar population templates that reduce a systematic bias in galaxy stellar population analyses.
A KDE-based MDF reconstruction from CALIFA IFU data reveals that MDF width decreases with galaxy mass and that radial metallicity profiles can obscure multi-modal chemical structures.
Molecular gas discs in six low-excitation radio galaxies rotate in an ordered manner but show ubiquitous low-level distortions, with NGC 3557 yielding a black hole mass of 7.1e8 solar masses and NGC 3100 showing evidence of inflowing gas.
citing papers explorer
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Cosmography with DESI-DR1 Cosmic Chronometers: Direct H(z) measurements from Luminous Red Galaxy ages
Stacked DESI-LRG spectra yield a cosmographic H(z) curve from z=0.36 to 0.80 and two direct cosmic-chronometer measurements, including H(z≈0.61)=88.5^{+6.7}_{-12.6}±8.1 km/s/Mpc.
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SDSS-IV MaStar: Quantification and Abatement of Interstellar Absorption in the Largest Empirical Stellar Spectral Library
Interstellar calcium and sodium absorption in MaStar is modeled and removed, yielding corrected spectra and simple stellar population templates that reduce a systematic bias in galaxy stellar population analyses.
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The stellar metallicity distribution function of galaxies in the CALIFA survey
A KDE-based MDF reconstruction from CALIFA IFU data reveals that MDF width decreases with galaxy mass and that radial metallicity profiles can obscure multi-modal chemical structures.
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The AGN fuelling/feedback cycle in nearby radio galaxies II. Kinematics of the molecular gas
Molecular gas discs in six low-excitation radio galaxies rotate in an ordered manner but show ubiquitous low-level distortions, with NGC 3557 yielding a black hole mass of 7.1e8 solar masses and NGC 3100 showing evidence of inflowing gas.