15 citations
- Harper CollegeUS5 papers
- Carter ObservatoryNZ4 papers
- University of CanterburyNZ4 papers
- Victoria University of WellingtonNZ4 papers
- Brigham Young UniversityUS3 papers
- Çanakkale Onsekiz Mart ÜniversitesiTR3 papers
- Istanbul UniversityTR2 papers
- Masaryk UniversityCZ2 papers
- Czech Academy of Sciences, Astronomical InstituteCZ1 paper
- Nielsen Engineering & Research (United States)US1 paper
- Provo CollegeUS1 paper
6 papers
V410 Puppis: A useful laboratory for early stellar evolution
Ahmet Erdem, Derya Surgit, Burcu Ozkardes +6
New spectrometric (HERCULES) and ground-based multi-colour photometric data on the multiple star V410 Puppis are combined with satellite photometry (HIPPARCOS and TESS), as well as…
A photometric and astrometric study of the open clusters NGC 1664 and NGC 6939
S. Koc, T. Yontan, S. Bilir +5
This study calculated astrophysical parameters, as well as kinematic and galactic orbital parameters, of the open clusters NGC 1664 and NGC 6939. The work is based on CCD UBV and G…
A study of the Czernik 2 and NGC 7654 open clusters using CCD UBV photometric and Gaia EDR3 data
B. Akbulut, S. Ak, T. Yontan +5
We analysed the open clusters Czernik 2 and NGC 7654 using CCD UBV photometric and Gaia Early Data Release 3 (EDR3) photometric and astrometric data. Structural parameters of the t…
Absolute Parameters of Young Stars: V Puppis
Edwin Budding, Tom Love, Mark G. Blackford +2
New spectrometric data on V Pup are combined with satellite photometry (HIPPARCOS and recent TESS) to allow a revision of the absolute parameters with increased precision. We find:…
Exoplanet System Kepler-2 with comparisons to Kepler-1 and 13
Michael D. Rhodes, Caglar Puskullu, Edwin Budding +1
We have carried out an intensive study of photometric (Kepler Mission) and spectroscopic data on the system Kepler-2 (HAT-P-7A) using the dedicated software WinFitter. The mean ind…
Transit modelling of selected Kepler systems
Q. Y. Huang, T. Banks, E. Budding +2
This paper employs a simple model, considering just geometry and linear or quadratic limb darkening, to fit Kepler transit data via a Markov Chain Monte Carlo (MCMC) methodology fo…