Zobrazeno 1 - 10
of 503
pro vyhledávání: '"J. Molenda"'
Autor:
J. Molenda-Zakowicz
Publikováno v:
Odessa Astronomical Publications, Vol 14, Iss 0, Pp 156-158 (2017)
We apply the False Alarm Probability analysis, (FAP), to the multiperiodicity search. Then we show the necessity of using the FAP method in the analysis of the astronomical time-series. We present the results obtained for 153 stars supposed or known
Externí odkaz:
https://doaj.org/article/cb16a71e836445b2a213141a766ad0dc
Autor:
Zong, Weikai, Fu, Jian-Ning, De Cat, Peter, Wang, Jiaxin, Shi, Jianrong, Luo, Ali, Zhang, Haotong, Frasca, A., Żakowicz, J. Molenda, Gray, R. O., Corbally, C. J., Catanzaro, G., Cang, Tianqi, Wang, Jiangtao, Chen, Jianjun, Hou, Yonghui, Liu, Jiaming, Niu, Hubiao, Pan, Yang, Tian, Hao, Yan, Hongliang, Zhang, Yong, Zuo, Heng
Phase \RNum{2} of the LAMOST-{\sl Kepler/K}2 survey (LK-MRS), initiated in 2018, aims at collecting medium-resolution spectra ($R\sim7,500$; hereafter MRS) for more than $50,000$ stars with multiple visits ($\sim60$ epochs) over a period of 5 years (
Externí odkaz:
http://arxiv.org/abs/2009.06843
Autor:
Zong, Weikai, Fu, Jian-Ning, De Cat, Peter, Shi, Jianrong, Luo, Ali, Zhang, Haotong, Frasca, A., Corbally, C. J., Żakowicz, J. Molenda, Catanzaro, G., Gray, R. O., Wang, Jiangtao, Pan, Yang, Ren, Anbing, Zhang, Ruyuan, Jin, Mengqi, Wu, Yue, Dong, Subo, Xie, Ji-Wei, Zhang, Wei, Hou, Yonghui, collaboration, LAMOST-Kepler
The LAMOST-Kepler (LK-) project was initiated to use the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) to make spectroscopic follow-up observations for the targets in the field of the Kepler mission. The Kepler field is divided i
Externí odkaz:
http://arxiv.org/abs/1810.02753
Akademický článek
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Akademický článek
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Autor:
A. Frasca, J. Molenda-Żakowicz, J. Alonso-Santiago, G. Catanzaro, P. De Cat, J. N. Fu, W. Zong, J. X. Wang, T. Cang, J. T. Wang
In this work we present the results of our analysis of 16,300 medium-resolution LAMOST spectra of late-type stars in the Kepler field with the aim of determining the stellar parameters, activity level, lithium atmospheric content, and binarity. We ha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::638724163cda214c90719faf965557cd
http://arxiv.org/abs/2205.04757
http://arxiv.org/abs/2205.04757
Publikováno v:
Acta Crystallographica Section A Foundations and Advances. 78:e494-e494
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5d99060732f51558870f2e7dc2a41297
https://doi.org/10.1107/s2053273322092543
https://doi.org/10.1107/s2053273322092543
Publikováno v:
Acta Crystallographica Section A Foundations and Advances. 78:e502-e502
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aeb1a936c8296288ca1a41b9a4736c2d
https://doi.org/10.1107/s2053273322092464
https://doi.org/10.1107/s2053273322092464
Publikováno v:
Acta Crystallographica Section A Foundations and Advances. 78:e503-e503
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f98832bf8315a0c676aebf8abadc16a1
https://doi.org/10.1107/s2053273322092452
https://doi.org/10.1107/s2053273322092452
Publikováno v:
PRZEMYSŁ CHEMICZNY. 1:186-192
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9e4d40da80e6c7ef2833448af8a45018
https://doi.org/10.15199/62.2018.8.29
https://doi.org/10.15199/62.2018.8.29