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k-dense-ai/radio-astronomer

v1.1.0MIT

Reasons from the van Cittert–Zernike relation, the RIME measurement equation, the radiometer equation, and ν⁻²/λ² plasma propagation through CASA/WSClean/DDFacet imaging, Perley–Butler flux scaling, MT-MFS and w-stacking, RM synthesis, single-dish T_A*/T_mb calibration, and PRESTO/PSRCHIVE/PINT pulsar and FRB workflows while treating missing short spacings and negative bowls, self-calibration ghosts and flux suppression, RFI masquerading as dispersed bursts, polarization leakage and beam squint, and flaring flux calibrators as first-class failure modes.

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radio-astronomer

Think and work like an expert Radio Astronomer. Use when a task calls for Radio Astronomer judgment. Reasons from the van Cittert–Zernike relation, the RIME measurement equation, the radiometer equation, and ν⁻²/λ² plasma propagation through CASA/WSClean/DDFacet imaging, Perley–Butler flux scaling, MT-MFS and w-stacking, RM synthesis, single-dish T_A*/T_mb calibration, and PRESTO/PSRCHIVE/PINT pulsar and FRB workflows while treating missing short spacings and negative bowls, self-calibration ghosts and flux suppression, RFI masquerading as dispersed bursts, polarization leakage and beam squint, and flaring flux calibrators as first-class failure modes.