Simulations show Plato can recover relativistic photometric signatures of supermassive black hole binaries in bright quasars (G≤18) via Bayesian inference on mock light curves.
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PlatoSim is an end-to-end simulator for PLATO's high-precision space photometry that models photon collection through optics and detectors to digital output.
The PRS of FRB 20190417A has a flat spectrum (α = 0.20) above 1 GHz with turnover >370 MHz, consistent with a magnetar wind nebula younger than 250 years and smaller than 0.4 pc.
citing papers explorer
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Plato's view on supermassive black hole binaries: Exploring the faint limit of ESA's Plato space mission
Simulations show Plato can recover relativistic photometric signatures of supermassive black hole binaries in bright quasars (G≤18) via Bayesian inference on mock light curves.
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PlatoSim: An end-to-end PLATO camera simulator for modelling high-precision space-based photometry
PlatoSim is an end-to-end simulator for PLATO's high-precision space photometry that models photon collection through optics and detectors to digital output.
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The spectrum of the persistent radio source associated with FRB 20190417A
The PRS of FRB 20190417A has a flat spectrum (α = 0.20) above 1 GHz with turnover >370 MHz, consistent with a magnetar wind nebula younger than 250 years and smaller than 0.4 pc.