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Neutral hydrogen mass distributions in galaxies uncovered by three-dimensional stacking
Atomic hydrogen (HI) serves as the raw fuel from which the star-forming molecular hydrogen forms - making it an important tracer of galaxy evolution. Due to the intrinsic faintness of the HI emission line (observed at rest at 21 cm), detecting HI emission in galaxies beyond a z = 0.1 becomes difficu...
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Department of Astronomy
2025
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