Volume 621, January 2019
|Number of page(s)||7|
|Section||Cosmology (including clusters of galaxies)|
|Published online||08 January 2019|
Impact of the 3D source geometry on time-delay measurements of lensed type-Ia supernovae
Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
2 Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str.1, 85740 Garching, Germany
3 Physik-Department, Technische Universität München, James-Franck-Straße 1, 85748 Garching, Germany
Accepted: 7 November 2018
It has recently been proposed that gravitationally lensed type-Ia supernovae can provide microlensing-free time-delay measurements provided that the measurement is taken during the achromatic expansion phase of the explosion and that color light curves are used rather than single-band light curves. If verified, this would provide both precise and accurate time-delay measurements, making lensed type-Ia supernovae a new golden standard for time-delay cosmography. However, the 3D geometry of the expanding shell can introduce an additional bias that has not yet been fully explored. In this work, we present and discuss the impact of this effect on time-delay cosmography with lensed supernovae and find that on average it leads to a bias of a few tenths of a day for individual lensed systems. This is negligible in view of the cosmological time delays predicted for typical lensed type-Ia supernovae but not for the specific case of the recently discovered type-Ia supernova iPTF16geu, whose time delays are expected to be smaller than a day.
Key words: gravitational lensing: strong / supernovae: general / cosmological parameters
© ESO 2019
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