PHANGS-Hα provides new narrow-band Hα imaging and derived star formation products for 65 nearby galaxies, validated against MUSE spectroscopy and serving as calibration reference for the PHANGS collaboration.
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J-PLUS DR3 yields Schechter-function stellar mass functions for quiescent and star-forming galaxies at 0.05 <= z <= 0.2 that match prior work, with quiescent galaxies showing higher characteristic mass and flatter faint-end slope.
citing papers explorer
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The PHANGS-H{\alpha} survey. Ground-based narrow-band imaging of nearby star-forming galaxies
PHANGS-Hα provides new narrow-band Hα imaging and derived star formation products for 65 nearby galaxies, validated against MUSE spectroscopy and serving as calibration reference for the PHANGS collaboration.
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J-PLUS: The stellar mass function of quiescent and star-forming galaxies at 0.05 <= z <= 0.2
J-PLUS DR3 yields Schechter-function stellar mass functions for quiescent and star-forming galaxies at 0.05 <= z <= 0.2 that match prior work, with quiescent galaxies showing higher characteristic mass and flatter faint-end slope.