Zobrazeno 1 - 10
of 1 040
pro vyhledávání: '"Şahin T"'
Determining the physical nature of a star requires precise knowledge of its stellar atmospheric parameters, including effective temperature, surface gravity, and metallicity. This study presents a new atomic line list covering a broad spectral range
Externí odkaz:
http://arxiv.org/abs/2410.08270
In this study, spectral, age, kinematic, and orbital dynamical analyses were conducted on metal-poor and high proper-motion (HPM) stars, HD 8724 and HD 195633, selected from the Solar neighborhood. This analysis combines detailed abundance measuremen
Externí odkaz:
http://arxiv.org/abs/2406.17776
Autor:
Kebapci, T. Y., Parlatan, S., Sert, S., Ozturk, I. K., Basar, G., Sahin, T., Bilir, S., Ferber, R., Tamanis, M., Kroger, S.
The hyperfine structure of 40 spectral lines of singly ionized thulium (Tm II) in emission spectra from a hollow cathode discharge lamp measured with a Fourier transform spectrometer in the wavelength range from 335 nm to 2345 nm has been investigate
Externí odkaz:
http://arxiv.org/abs/2405.05309
We propose a line list that may be useful for the abundance analysis of G-type stars in the wavelength range 4080 -- 6780 A. It is expected that the line list will be useful for surveys/libraries with overlapping spectral regions (e.g. ELODIE/SOPHIE
Externí odkaz:
http://arxiv.org/abs/2310.04129
Publikováno v:
Kafkas Universitesi Veteriner Fakültesi Dergisi, Vol 22, Iss 2, Pp 253-260 (2016)
Externí odkaz:
https://doaj.org/article/9209a168711442afbc25a7e4c7af4bca
This paper explores the ability of physics-informed neural networks (PINNs) to solve forward and inverse problems of contact mechanics for small deformation elasticity. We deploy PINNs in a mixed-variable formulation enhanced by output transformation
Externí odkaz:
http://arxiv.org/abs/2308.12716
Publikováno v:
Kafkas Universitesi Veteriner Fakültesi Dergisi, Vol 20, Iss 3, Pp 421-427 (2014)
Externí odkaz:
https://doaj.org/article/02832537b1484d7692f1bf2662f33e3a
Autor:
Pavlovski, K., Hummel, C. A., Tkachenko, A., Dervisoglu, A., Kayhan, C., Zavala, R. T., Hutter, D. J., Tycner, C., Sahin, T., Audenaert, J., Baeyens, R., Bodensteiner, J., Bowman, D. M., Gebruers, S., Jannsen, N. E., Mombarg, J. S. G.
Publikováno v:
A&A 658, A92 (2022)
Altough both components of the bright eclipsing binary $\alpha$ Dra having been resolved using long baseline interferometry and the secondary component shown to contribute some 15\% of the total flux, a spectroscopic detection of the companion star w
Externí odkaz:
http://arxiv.org/abs/2111.03887
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
In Procedia CIRP 2022 109:598-603