TIME commissioning observations demonstrate a 2D map data processing pipeline achieving less than 3% calibration difference versus the Bolocam Galactic Plane Survey on G49.5.
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2 Pith papers cite this work. Polarity classification is still indexing.
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ALMA survey finds 4 starless cores in Orion B North consistent with turbulent collapse simulations; virial analysis indicates Chamaeleon I cores are less bound with external pressure dominating unlike Orion B North and Ophiuchus.
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An ALMA search for substructure and fragmentation in starless cores in Orion B North
ALMA survey finds 4 starless cores in Orion B North consistent with turbulent collapse simulations; virial analysis indicates Chamaeleon I cores are less bound with external pressure dominating unlike Orion B North and Ophiuchus.