ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

SPIPS: Spectro-Photo-Interferometry of Pulsating Stars

Discussion topics for individual codes
Ada Coda
ASCL Robot
Posts: 1363
Joined: Thu May 08, 2014 5:37 am

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

Site: https://github.com/amerand/SPIPS
http://adsabs.harvard.edu/abs/2015A%26A...584A..80M

Bibcode: 2017ascl.soft10004M

Preferred citation method: http://adsabs.harvard.edu/abs/2015A%26A...584A..80M

ID: ascl:1710.004

Return to “Astrophysics Source Code Library”

Who is online

Users browsing this forum: Bing [Bot] and 7 guests

cron