LIGHT CURVES
The Lick AGN Monitoring Project 2011: Photometric Light Curves
... AGN light curves ( Kelly et ...driving light curves, our inferences are robust with respect to the assumption of Gaussian processes, since Gaussian processes are effectively used as a fl exible ...
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Accretion disc time lag distributions : applying CREAM to simulated AGN light curves
... Cross-correlating short and long wavelength light curves is the traditional way to measure both continuum–line and continuum– continuum time delays. Two cross-correlation techniques to mea- sure lags ...
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NEW LIGHT CURVES AND EPHEMERIS FOR THE CLOSE ECLIPSING BINARY V963 PERSEI
... their light curves with a model having three spots on the secondary and one on the primary ...the light variation that RGS found, and the system remains an interesting ...
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The W Ursae Majoris systems : interpretation of light curves and line profiles
... li'or cal;rulating light curves and line profiles, the surface is broken up into one to four thousand elements of area, the nU1J1ber depending on the accuracy desired... elements of area[r] ...
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Modelling the KIC8462852 light curves : compatibility of the dips and secular dimming with an exocomet interpretation
... optical light curve of KIC8462852, and the lack of variability at current detection thresholds in the infrared light curves, are compatible with an origin in circumstellar material distributed around ...
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The similarity of light curves of Fermi Blazars
... Data of sources could be downloaded from the website of LAT Monitored Source List Light Curves. Commonly, Fluxes of Fermi source is highly variable. Here, F ( t ) denotes the flux at time t. Because the ...
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Chromatic transit light curves of disintegrating rocky planets
... transit light curves of our simulated tails using the Monte-Carlo radiative transfer code MCMax3D (Min et ...transit light curves for optically thick ...
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More rapidly rotating PMS M dwarfs with light curves suggestive of orbiting clouds of material
... phased light curves showing multiple scallops or ...” light curve morphology are mid-to-late M dwarfs without evidence of active accretion and with photometric periods generally < 1 ...phased ...
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A procedure for maize genotypes discrimination to drought by chlorophyll fluorescence imaging rapid light curves
... The experiments were carried out in a greenhouse at National Agroenergy Research Center (https:// www.embrapa.br/en/agroenergia), in Brasilia, Bra- zil (S—15.732°, W—47.900°) from November 2015 to February 2016. Three ...
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Temporal studies on GRB light curves for neutrino flux predictions in multi-collision zone models
... GRB light curve and taking into account the data taking conditions and the detector response during the GRB episode [7], the number of expected signal in the ANTARES neutrino telescope from GRB 110918A was ...
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Lasers, lenses and light curves : adaptive optics microscopy and peculiar transiting exoplanets
... a brightness contrast of up to nine orders of magnitude for the case of Jupiter, or ten order of magnitude for Earth for visible light (Des Marais et al., 2002). In addition, exoplanets appear in close proximity ...
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The coronal monsoon : thermal nonequilibrium revealed by periodic coronal rain
... This time lag is a fi rst indication that the plasma of the pulsating bundle of loops is predominantly seen when cooling. Indeed, when the plasma temperature evolves in response to a heat input, either impulsive ( Viall ...
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PHL 1445 : an eclipsing cataclysmic variable with a substellar donor near the period minimum
... eclipse light curves (phases 0, 1413, 1430 and 1431) observed not too far apart in time (2011 November–2012 January), with clear bright spot ingresses at a similar position, were phase-folded and ...average ...
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Machine learning approaches to exoplanet transit detection and candidate validation in wide field ground based surveys
... Since the start of the Wide-angle Search for Planets (WASP) program, more than 160 transiting exoplanets have been discovered in the WASP data. In the past, possible transit-like events identified by the WASP pipeline ...
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X-ray spectroscopy of the IP PQ Gem
... (Fig. 3, Section 3.5). These two results imply that variability in both the absorption and the normalization of the hard X-rays over the spin cycle could be the cause of the observed modulation in the spin- folded ...
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Optical transients in the WASP survey
... and spectral properties [24]. Systems that are only known to have had one nova eruption are known as classical novae. The duration of these eruptions can vary dramatically. V1500 Cyg only took 3.6 days to decrease 3 ...
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Pair-instability Supernova Explosions in 1D, 2D, and 3D and Their Observational Signatures.
... Here, we present explosions and light curves for four progenitor models, with relatively shallow envelopes, that span the PISN mass range.. Our light curves.[r] ...
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FIRST RESULT OF THE CZECH RR LYRAE STARS OBSERVATION PROJECT
... well-covered light curves to determine ephemerides, periods, light curve characteristics (amplitude, rising time) and finally to obtain Fourier parameters to estimate the basic physical ...
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HATS-60b-HATS-69b: 10 transiting planets from HATSouth
... HATSouth light curve of each target, including the period, transit depth, transit duration, and signal- to-noise ratio ( S / N ) for the top peak in the BLS ...
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Atmospheric characterization of the ultra hot Jupiter MASCARA 2b/KELT 20b : Detection of CaII, FeII, NaI, and the Balmer series of H (Hα, Hβ, and Hγ) with high dispersion transit spectroscopy
... The transmission light curves of each individual CaII line and the transmission light curve after combining of all three lines see Appendix C present consistent absorption depth values i[r] ...
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