Searching for the first stars with the Gaia mission

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

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8 pages, 7 figures

Scientific paper

We construct a theoretical model to predict the number of orphan afterglows (OA) from gamma-ray bursts (GRBs) triggered by primordial metal free (Pop III) stars expected to be observed by the Gaia mission. In particular, we consider primordial metal free stars which were affected by radiation from other stars (Pop III.2) as a possible target. We use a semi-analytical approach, with the inclusion of all relevant feedback effects, to construct the cosmic star formation history and its connection with GRBs cumulative number. The OA events are generated via Monte-Carlo method, and realistic simulations of Gaia's scanning law are performed to derive the observation probability expectation. We show that $\sim 0.4\%$ of all Pop III.2 afterglows should appear in the sky above of Gaia observational flux limit. Combining this result with simulations of Gaia's scanning law, we expect to observe an average of $\sim 13\% \pm 7\%$ of all OA above the observational sensitivity.

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