Towards understanding of low-amplitude variability of classical Cepheids
| project | OPUS, 2024/53/B/ST9/02630 |
| funding | Polish National Science Center, NCN |
| PI | Radosław Smolec |
| Co-Is | Rajeev Singh Rathour |
| Igor Soszyński | |
| Oliwia Ziółkowska | |
| dates | 01.2025 - 01.2027 |
Jump to project highlights, refereed publications, conference contributions, and presentations.
Project Highlights
- Software for time–frequency analysis of astronomical time series coming soon
A key element of the project is the software developed by the team for time–frequency analysis of astronomical time series. Our software enables fast, versatile, and interactive data analysis. In addition to standard functionalities, such as computing the discrete Fourier transform and fitting models to data, the software allows for time-dependent prewhitening, segmentation of the data, trend modeling, and advanced comparison with observations for classical pulsating stars.
Interactive interface for frequency spectrum analysis.
Refereed Publications
Conference Publications
