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SPIPS: Spectro-Photo-Interferometry of Pulsating Stars

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Ada Coda
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SPIPS: Spectro-Photo-Interferometry of Pulsating Stars

Postby Ada Coda » Mon Oct 16, 2017 3:18 pm

SPIPS: Spectro-Photo-Interferometry of Pulsating Stars

Abstract: SPIPS (Spectro-Photo-Interferometry of Pulsating Stars) combines radial velocimetry, interferometry, and photometry to estimate physical parameters of pulsating stars, including presence of infrared excess, color excess, Teff, and ratio distance/p-factor. The global model-based parallax-of-pulsation method is implemented in Python. Derived parameters have a high level of confidence; statistical precision is improved (compared to other methods) due to the large number of data taken into account, accuracy is improved by using consistent physical modeling and reliability of the derived parameters is strengthened by redundancy in the data.

Credit: Mérand, Antoine


Bibcode: 2017ascl.soft10004M

Preferred citation method:

ID: ascl:1710.004

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