Hipparcos Positioning of Geminga : How and Why . ♠ , ♣

Accuracy in the absolute position in the sky is one of the limiting factors for pulsar timing, and timing parameters have a direct impact on the understanding of the physics of Isolated Neutron Stars (INS). We report here on a high-accuracy measurement of the optical position of Geminga (mv = 25.5), the only known radioquiet INS. The procedure combines the Hipparcos and Tycho catalogues, ground-based astrometric data,and Hubble Space Telescope (HST) Wide Field Planetary Camera (WFPC2) images, to yield Geminga’s absolute position to within ∼ 40 mas (per coordinate). Such a positional accuracy, unprecedented for the optical position of a pulsar or an object this faint, is needed to combine in phase γray photons collected over more than 20 years, i.e. over 2.5 billions of star’ revolutions. Although quite a difficult task, this is the only way to improve our knowledge of the timing parameters of this radio silent INS.