Intermediate-redshift galaxies show systematically higher dust attenuation at fixed star formation rate surface density than local galaxies, with the excess strongest for galaxies below the star-forming main sequence.
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8 Pith papers cite this work. Polarity classification is still indexing.
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2026 8representative citing papers
Cosmological zoom-in simulation of a 10^9.7 solar mass dwarf galaxy shows AGN outflows create >10^6 K bubbles accelerating gas to 600 km/s that recycle within 10 kpc, tracing observed BPT loci over time.
Stellar surface density independently modulates MgII outflow equivalent width in massive star-forming galaxies at 0.35<z<1.0 observed by DESI.
JWST auroral-line selected galaxies at high redshift show an MZR slope of 0.38 with selection biases favoring high-SFR low-metallicity systems, while stacked non-detections lie closer to the fundamental metallicity relation.
Spatially resolved SED fitting shows AGN contributes 34% of nuclear IR luminosity in GN20 but only 9% galaxy-wide, with the black hole on the local M_BH-M_bulge relation.
Higher-resolution spectra reveal outflow signatures in ~30% of low-mass galaxies (rising to ~60% at higher SFR), with ionized mass outflow rates of 0.1-50 x 10^-3 solar masses per year.
NGC 1427A shows a complex star formation history with young (~10 Myr) and intermediate-age (100-300 Myr) clusters that trace environmental processing during its orbit in the Fornax cluster.
AGN activity correlates independently with bar strength and bulge prominence in z≤0.1 galaxies after controlling for mass and color.
citing papers explorer
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The MAGPI Survey: Evidence for Non-Universal Resolved Dust Attenuation Relations Beyond the Local Universe
Intermediate-redshift galaxies show systematically higher dust attenuation at fixed star formation rate surface density than local galaxies, with the excess strongest for galaxies below the star-forming main sequence.
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AGN-driven outflows in dwarf galaxies from cosmological simulations: Internal properties and observational signatures
Cosmological zoom-in simulation of a 10^9.7 solar mass dwarf galaxy shows AGN outflows create >10^6 K bubbles accelerating gas to 600 km/s that recycle within 10 kpc, tracing observed BPT loci over time.
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Stellar Surface Density Modulates MgII Cool-gas Outflow Absorption in DESI Star-forming Galaxies
Stellar surface density independently modulates MgII outflow equivalent width in massive star-forming galaxies at 0.35<z<1.0 observed by DESI.
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Shape of Direct-Method Mass-Metallicity Relation with JWST: Fast-Track Nitrogen and Helium Enrichment
JWST auroral-line selected galaxies at high redshift show an MZR slope of 0.38 with selection biases favoring high-SFR low-metallicity systems, while stacked non-detections lie closer to the fundamental metallicity relation.
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Dissecting the Obscured Core of GN20: an Active Galactic Nucleus Outshone by Young Stars
Spatially resolved SED fitting shows AGN contributes 34% of nuclear IR luminosity in GN20 but only 9% galaxy-wide, with the black hole on the local M_BH-M_bulge relation.
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Higher resolution optical spectra of $M_*<10^{10}~M_{\odot}$ galaxies reveal outflow signatures unresolved by the SDSS
Higher-resolution spectra reveal outflow signatures in ~30% of low-mass galaxies (rising to ~60% at higher SFR), with ionized mass outflow rates of 0.1-50 x 10^-3 solar masses per year.
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The complex history of NGC 1427A revealed by its star clusters and star formation history
NGC 1427A shows a complex star formation history with young (~10 Myr) and intermediate-age (100-300 Myr) clusters that trace environmental processing during its orbit in the Fornax cluster.
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The complex relationships between AGN, bars and bulges
AGN activity correlates independently with bar strength and bulge prominence in z≤0.1 galaxies after controlling for mass and color.