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TRANSLIENT: Detecting Transients Resulting from Point-source Motion or Astrometric Errors

  • Authors: Ofer Springer, Eran O. Ofek, Barak Zackay, Ruslan Konno, Amir Sharon, Guy Nir, Adam Rubin, Asaf Haddad, Jonathan Friedman, Leora Schein-Lubomirsky, Iakov Aizenberg, Alexander Krassilchtchikov, Avishay Gal-Yam

Ofer Springer et al 2024 The Astronomical Journal 167 .

  • Provider: AAS Journals

Caption: Figure 10.

The likelihood function ﹩P({\widehat{D}}_{T}| {\alpha }_{r}-{\alpha }_{n},({\alpha }_{r}+{\alpha }_{n})| | {\rm{\Delta }}| | ,\theta )﹩, obtained by linearizing Equation (25) in k · Δ. Here evaluation is again for the small translation simulation 8 (as in Figures 8 and 9). One can see that this reduced set of model parameters (in the linearized likelihood) does not show a strong dependence and may therefore be preferable in the small translation limit.

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