Zobrazeno 1 - 10
of 78
pro vyhledávání: '"Phase dispersion minimization"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 508:3975-3994
Active galactic nucleus (AGN) emission is dominated by stochastic, aperiodic variability which overwhelms any periodic/quasi-periodic signal (QPO) if one is present. The Auto Correlation Function (ACF) and Phase Dispersion Minimization (PDM) techniqu
Publikováno v:
Universe, Vol 7, Iss 429, p 429 (2021)
Universe
Volume 7
Issue 11
Universe
Volume 7
Issue 11
The light curve period of an asteroid plays an important role in determining the rotation period, the collision evolution and the YORP effect. There are many period extraction algorithms used to find the light curve period of asteroids with long term
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
[Aims] The final aim of this paper is to expand the sparse group of X-ray binaries with gamma-ray counterparts as laboratories to study high-energy processes under physical conditions that periodically repeat. [Methods] A follow-up of a candidate sys
We apply the ${\tt weirddetector}$, a nonparametric signal detection algorithm based on phase dispersion minimization, in a search for low duty-cycle periodic signals in the Transiting Exoplanet Survey Satellite (${\it TESS}$) photometry. Our approac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c935d989d720a16883bfb62b376b3eb2
We present the analysis of 34 light curves in $V$ and $I$ of 17 giant stars in the globular cluster NGC 3201, to check if such stars are variable and if their variability has some kind of impact on the iron abundance as obtained from spectroscopic me
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd6e9d389b90deea346ad947c89b9aa5
The Weird Detector: Flagging periodic, coherent signals of arbitrary shape in time series photometry
Autor:
Adam Wheeler, David M. Kipping
By design, model-based approaches for flagging transiting exoplanets in light curves, such as boxed least squares, excel at detecting planets with low S/N at the expense of finding signals that are not well described by the assumed model, such as sel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::49bb9cafb0adba30204f88ef907b2241
http://arxiv.org/abs/1903.09213
http://arxiv.org/abs/1903.09213
The aim of this study is to accurately calculate the rotational period of CS\,Vir by using {\sl STEREO} observations and investigate a possible period variation of the star with the help of all accessible data. The {\sl STEREO} data that cover five-y
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a80e87f6d984c965a6104601cd0b6f93
Publikováno v:
Astronomische Nachrichten. 335:1018-1036
A unique short-period (P = 0.65356(1) d) Mercury-size Kepler exoplanet candidate KIC012557548b has been discovered recently by Rappaport et al. (2012). This object is a transiting disintegrating exoplanet with a circum-planetary material–comet-like
Periodicity detection in irregularly sampled light curves by robust regression and outlier detection
Publikováno v:
Statistical Analysis and Data Mining: The ASA Data Science Journal. 6:73-89
An important task in astroparticle physics is the detection of periodicities in irregularly sampled time series, called light curves. Many periodogram methods for light curves may be characterized as fitting periodic models using least squares regres
Autor:
Luke Burkhart, Cesar I. Fuentes, Danielle M. Hastings, Jean-Luc Margot, Michael E. Brown, Matthew J. Holman, Daniel C. Fabrycky, Darin Ragozzine
Publikováno v:
Hastings, DM; Ragozzine, D; Fabrycky, DC; Burkhart, LD; Fuentes, C; Margot, J-L; et al.(2016). THE SHORT ROTATION PERIOD OF HI'IAKA, HAUMEA'S LARGEST SATELLITE. ASTRONOMICAL JOURNAL, 152(6). doi: 10.3847/0004-6256/152/6/195. UCLA: Retrieved from: http://www.escholarship.org/uc/item/7q75z7fq
Hi'iaka is the larger outer satellite of the dwarf planet Haumea. Using relative photometry from the Hubble Space Telescope and Magellan and a phase dispersion minimization analysis, we have identified the rotation period of Hi'iaka to be ~9.8 hrs (d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7802faee546d56cbe973df1ea9c6dccf
http://arxiv.org/abs/1610.04305
http://arxiv.org/abs/1610.04305