Reddening maps of the LMC and SMC are produced via SED fitting of RGB stars from SMASH and VMC photometry, yielding mean E(B-V) of 0.076 mag and 0.058 mag with relative spatial structure stable across three stellar atmosphere models but absolute values differing by up to 0.03 mag.
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2 Pith papers cite this work. Polarity classification is still indexing.
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A new sample of young candidate Bridge stars is identified and shown to align with gas structures, with kinematics implying a ~125 Myr crossing time consistent with the last LMC-SMC interaction.
citing papers explorer
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Reddening maps of the Magellanic Clouds using spectral energy distribution fitting of red giants
Reddening maps of the LMC and SMC are produced via SED fitting of RGB stars from SMASH and VMC photometry, yielding mean E(B-V) of 0.076 mag and 0.058 mag with relative spatial structure stable across three stellar atmosphere models but absolute values differing by up to 0.03 mag.
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Characterisation of the Clouds' young stellar Bridge using Gaia DR3
A new sample of young candidate Bridge stars is identified and shown to align with gas structures, with kinematics implying a ~125 Myr crossing time consistent with the last LMC-SMC interaction.