A radio-luminosity-based model of mild q decrease to z~2 from cosmic ray losses mitigates the >3σ discrepancy in MeerKAT source counts near 10 μJy with ≥2σ evidence, while bounding intrinsic scatter.
J., Srinivasan, S., Pudritz, R
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
Stronger radiation environments produce more massive, hotter protostellar discs whose fragments are large and disruptive rather than planetary-mass.
SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.
citing papers explorer
-
The Radio-IR Correlation in the Context of Deep Radio Source Counts
A radio-luminosity-based model of mild q decrease to z~2 from cosmic ray losses mitigates the >3σ discrepancy in MeerKAT source counts near 10 μJy with ≥2σ evidence, while bounding intrinsic scatter.
-
The Impact of Radiation Environment on the Evolution and Fragmentation of Protostellar Discs
Stronger radiation environments produce more massive, hotter protostellar discs whose fragments are large and disruptive rather than planetary-mass.
-
Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect
SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.