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.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
verdicts
UNVERDICTED 3representative citing papers
tPIC2.2 supplies a list of 217,741 stars for PLATO's LOPS2 field, including 202,315 FGK dwarfs/subgiants and 15,037 M dwarfs with uniformly estimated temperatures, radii, and masses.
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.
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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The PLATO Input Catalogue of targets (tPIC) for the first Long Pointing Field
tPIC2.2 supplies a list of 217,741 stars for PLATO's LOPS2 field, including 202,315 FGK dwarfs/subgiants and 15,037 M dwarfs with uniformly estimated temperatures, radii, and masses.
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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.