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.
Title resolution pending
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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Small and Complex I: The Three Component Structure of $z \sim 0$ Massive Compact Quiescent Galaxies
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.
- Toward Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions