Hou, Goodman, and I discussed spectral fitting in the context of radial-velocity measurement, relevant to our exoplanet work. We feel like we might be able to go the next level down, as it were. In the afternoon, Dmitry Malyshev (NYU) and I discussed how Malyshev is fitting the number-flux relation for gamma-ray sources in the Fermi data below the point-source detection limit. He is finding some nice surprises in there.
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