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pro vyhledávání: '"Starspot"'
Akademický článek
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Publikováno v:
Advances in Space Research. 69:499-513
Chromospherically active binaries’ (CABs) are late-type evolved stars with strong chromosphere/coronae and high flare activity levels. Starspot evolution in these CABs and binaries reveals strong stellar and chromospheric activities. In binaries, t
Akademický článek
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Autor:
J. E. Hughes, Stephen C. Marsden, Matthew W. Mengel, D. Burton, Nikolai Piskunov, S. V. Jeffers, Ian A. Waite, N. Shaw, G. M. Perugini, E. Hébrard
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 508:3304-3320
The evolution in latitude of sunspots is a key feature of the cyclic solar dynamo. Here, we present the results of a spectroscopic and spectropolarimetric monitoring campaign on the young (∼20 Myr old) early G star HIP 89829, in order to investigat
Correcting the effect of stellar spots on ARIEL transmission spectra – II. The limb-darkening effect
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:6118-6131
This paper is part of an effort to correct the transmission spectra of a transiting planet orbiting an active star. In Paper I (Cracchiolo et al. 2020) we have demonstrated a methodology to minimize the potential bias induced by unocculted star spots
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:1795-1813
The parameter space for modelling stellar systems is vast and complicated. To find best-fitting models for a star one needs a statistically robust way of exploring this space. We present a new machine-learning approach to predict the modelling parame
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 504:4302-4311
We study the detached eclipsing binary, KIC 5359678, with starspot modulation using the high-quality Kepler photometry and LAMOST spectroscopy. The phoebe model, optimal for this binary, reveals that this system is a circular detached binary, compose
Autor:
James A. G. Jackman, Jack S. Acton, Michael R. Goad, Rosanna H. Tilbrook, Didier Queloz, Edward Gillen, Sarah L. Casewell, Boris T. Gänsicke, Samuel Gill, Simon Hodgkin, Maximilian N. Günther, David R. Anderson, Richard G. West, Liam Raynard, Beth A. Henderson, Joshua T. Briegal, Chloe E. Pugh, Daniel Bayliss, Matthew R. Burleigh, James S. Jenkins, Peter J. Wheatley, Christopher A. Watson
Publikováno v:
Jackman, J A G, Wheatley, P J, Acton, J S, Anderson, D R, Bayliss, D, Briegal, J T, Burleigh, M R, Casewell, S L, Gänsicke, B T, Gill, S, Gillen, E, Goad, M R, Günther, M N, Henderson, B A, Hodgkin, S T, Jenkins, J S, Pugh, C, Queloz, D, Raynard, L, Tilbrook, R H, Watson, C A & West, R G 2021, ' Stellar flares detected with the Next Generation Transit Survey ', Monthly Notices of the Royal Astronomical Society, vol. 504, no. 3, pp. 3246-3264 . https://doi.org/10.1093/mnras/stab979
We present the results of a search for stellar flares in the first data release from the Next Generation Transit Survey (NGTS). We have found 610 flares from 339 stars, with spectral types between F8 and M6, the majority of which belong to the Galact
Publikováno v:
Chinese Astronomy and Astrophysics. 45:67-81
We present a newly discovered magnetically active binary system detected by Yunnan-Hong Kong wide field survey, with an orbital period of 0.60286 days. Two color photometry for the system was performed using the 1 m Cassegrain telescope of Yunnan Obs
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 501:1733-1747
The goal of this study is to assess the impact of the stellar spots on the extraction of the planetary transmission spectra observed by ARIEL. We develop a method to model the stellar spectrum of a star in the presence of spots by using the out-of-tr