LStein is a new visualization technique that links data series to display sparse 2.5D information more effectively than traditional methods.
The Thousand-Pulsar-Array programme on MeerKAT – I. Science objectives and first results
3 Pith papers cite this work, alongside 49 external citations. Polarity classification is still indexing.
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Pith papers citing it
49
external citations · Crossref
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2026 3representative citing papers
VLA L-band polarization observations of SNR G7.7-3.7 show cocoon morphology from interaction with pre-existing circumstellar shells, with magnetic fields compressed along filaments and RM variations tracing massive progenitor winds.
Pulsar radio emission beams from the two poles are generally dissimilar in azimuth width and often radius, based on rotating vector model fits to polarization data from eight double-pole interpulse pulsars.
citing papers explorer
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LStein: A new approach to visualizing sparse 2.5-dimensional data
LStein is a new visualization technique that links data series to display sparse 2.5D information more effectively than traditional methods.
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The Cocoon from a Massive Star's Death: VLA Radio Polarization Study of Possible Historical Supernova Remnant G7.7$-$3.7
VLA L-band polarization observations of SNR G7.7-3.7 show cocoon morphology from interaction with pre-existing circumstellar shells, with magnetic fields compressed along filaments and RM variations tracing massive progenitor winds.
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On the Difference Between Pulsar Radio Emission Beams from the Two Poles
Pulsar radio emission beams from the two poles are generally dissimilar in azimuth width and often radius, based on rotating vector model fits to polarization data from eight double-pole interpulse pulsars.