Download and installation

The latest version (1.2) can be downloaded from PyPI – the Python Package index

The package includes the source code, a configuration file, and a document (PDF).

PSLS requires the following python packages: numpy, scipy, matplotlib, and yaml
To install the program in your home directory for you own use, type:

 python install --home=$HOME/

It is also possible to install the code for all the users:

 sudo python install

Edit the configuration file, an example is given in psls.yaml. Then, execute PSLS: -P -V psls.yaml

To make the code working with ADIPLS, you will also need to provide as input  a set of theoretical frequencies (the .gsm files generated by ADIPLS).

The package provides the code and various files storing the parameters describing the PLATO systematic errors:

  • PLATO_systematics_[BOL/EOL]_V1.npy: Begining Of Life (BOL) and End Of Life (EOL) systematic errors for the P5 sample (aperture mask photometry with mask updates operating) ;
  • PLATO_systematics_[EOL/BOL]_FixedMask_V1.npy: fixed aperture mask  photometry ;
  •  PLATO_systematics_[EOL/BOL]_P1_V1.npy: systematic errors representative for the P1
    sample (based on the PSF fitting method)

Old systematic errors tables (version 0) are given for compatibility and consistency with Samadi et al (2019) results.

The package also provides two working examples:
– a main sequence star (0012069449.yaml) with its associated theoretical frequencies (0012069449.gsm) generated by ADIPLS pulsation code
– a red giant star (0009882316.yaml), which does not require as input theoretical frequencies.

The grid of models have to be downloaded from this website.

We provide two grids of theoretical frequencies (credit: Takafumi Sonoi):

  • m+0y27l.tar.gz: stellar models with masses ranging between 0.75 and 1.15 with an initial Helium abundance Y_0=0.27 ; microscopic diffusion (no radiative accelerations) was included using the simplified equations from Michaud & Proffitt (1993). Overshoot is not included and the mixing-length parameter is fixed to 1.9.
  • m+0y24h.tar.gz: stellar models with masses ranging between 1.20 and 2.00 with an Helium abundance Y=0.24 ; diffusion was not included as this depletes heavy elements from the upper layers of the star, due to the neglect of radiative accelerations. An overshoot of 0.2 is assumed and the mixing-length parameter is fixed to 1.6.

Note that, for RGB and clump stars, the program relies on the Universal Pattern, accordingly sets of theoretical frequencies are not required for those stars. To install the grids proceed as follows:

mkdir models
cd models
tar zxf m+0y24h.tar.gz
tar zxf m+0y27l.tar.gz
cd ..

This simulator is not an official product of the Plato Mission Consortium (PMC), it  is distributed under the terms of the GNU General Public License  in the hope that it will be useful, but WITHOUT ANY WARRANTY.

(c) 2017 by Réza SAMADI, LESIA – Observatoire de Paris.

Main contributors: Alexi Deru (LESIA), Emmanuel Grolleau (LESIA), Daniel Reese (LESIA)

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