https://doi.org/10.1051/epjconf/201715203008
Spectro-Photo-Interferometry of Stellar Pulsation (SPIPS)
A more precise and more accurate implementation of the parallax of pulsation method
1 European Southern Observatory, Alonso de Córdova 3107, Casilla 19001, Santiago 19, Chile
2 LESIA (UMR 8109), Observatoire de Paris, PSL, CNRS, UPMC, Univ. Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France
3 Unidad Mixta Internacional Franco-Chilena de Astronomía, CNRS/INSU, France (UMI 3386), Departamento de Astronomía, Universidad de Chile, Camino El Observatorio 1515, Las Condes, Santiago, Chile
4 Universidad de Concepción, Departamento de Astronomía, Casilla 160-C, Concepción, Chile
5 Institut Supérieur de l’Aéronautique et de l’Espace, Toulouse, France
Published online: 8 September 2017
We present our implementation of the parallax of pulsation method which integrates all observables and physical modelling of the photosphere to get the best statistical precision and controlled biases. This method has been validated on well known stars and used to estimate observationally the projection factor of the HST-FGS sample. Our future developments include application to the Gaia Cepheids and modelling of the spectrum.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
