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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EP250827b/SN 2025wkm is an X-ray flash supernova at z=0.1194 powered by a long-lived magnetar and disk winds interacting with extended circumstellar medium, without an on-axis relativistic jet.
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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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EP250827b/SN 2025wkm: An X-ray Flash-Supernova Powered by a Central Engine and Circumstellar Interaction
EP250827b/SN 2025wkm is an X-ray flash supernova at z=0.1194 powered by a long-lived magnetar and disk winds interacting with extended circumstellar medium, without an on-axis relativistic jet.