PCA of H-band IFU pixel spectra decomposes cool stellar populations in NGC 5128 and NGC 5102, identifying M-giant, long-period variable, and carbon star contributions.
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3 Pith papers cite this work. Polarity classification is still indexing.
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2026 3representative citing papers
New SBF distance data confirm a steradian-scale flow converging at ~70 Mpc that matches the direction and amplitude of the CMB dipole and the original Great Attractor model.
SBF distances from HST place the trail dwarfs at ~20 Mpc, inconsistent with the NGC 1035 foreground, while DF2 is revised to 17.7 Mpc matching JWST TRGB at 17.6 Mpc.
citing papers explorer
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Decomposing cool stellar populations with H-band spectral fluctuations: Long-period variable stars in NGC 5128 and carbon stars in NGC 5102
PCA of H-band IFU pixel spectra decomposes cool stellar populations in NGC 5128 and NGC 5102, identifying M-giant, long-period variable, and carbon star contributions.
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New Measurements of Distances to Galaxies in the NGC 1052 Field with the Hubble and James Webb Space Telescopes: Testing the Bullet-Dwarf Origin of the Trail
SBF distances from HST place the trail dwarfs at ~20 Mpc, inconsistent with the NGC 1035 foreground, while DF2 is revised to 17.7 Mpc matching JWST TRGB at 17.6 Mpc.