Examples of using Light curve in English and their translations into Vietnamese
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Visual light curve for ρ Cassiopeiae from 1933 to 2015.
In addition, the merger model explains the multiple peaks in the light curve observed during the outburst.
Y Canum Venaticorum light curve, including RGB photoelectric measurements.
In 1991, a rotation period of Nereid of about13.6 hours was determined by an analysis of its light curve.
AAVSO light curve of recurrent nova T Pyx from 1 Jan 1966 to 17 Nov 2010.
The graph shows a comparison of a voltage versus transmitted light curve of a typical TN and a supertwist nematic(STN) display.
The shape of the light curve is fairly consistent from cycle to cycle, with the rise being steeper than the fall.
A blend scenario as an alternative explanation from an analysis combining allavailable radial velocity measurements with the OGLE light curve.
However, Type Ib light curves may peak at lower luminosity and may be redder.
Observational evidence based on Kepler observationsindicates much of the Blazhko effect's two-cycle light curve modulation is due to simple period-doubling.
Himalia's rotational light curve from Earth-based observations taken between August and October 2010.[7].
Kepler-7's candidate was not found to be one of these false positives,such as an eclipsing binary star that may generate a light curve that mimics that of transiting planetary companions.
Based on its light curve, Selene has an estimated rotation period of 0.3947±0.0004 days, or just under 9.5 hours.
Non-spherical optical lens PMMA Siamese,emitting angle design with light curve, reducing light loss by increasing the optical reflection.
Light curve of the asteroid 201 Penelope based on images taken on 6 October 2006 at Mount John University Observatory.
The UV spectroscopy was also used to calculate a light curve to precisely show just how much of the star's light is blocked out during transit.
For eclipsing binary stars- Eclipse mapping produces images and maps of spots on both stars.[2]For stars with transiting extrasolar planets- Light curve variations.[3].
There is a huge complex of dips in the light curve that appear, and they last for like a hundred days, all the way up into the Kepler mission's end.
Follow-up observations were conducted by a team of British, Spanish, French, Swiss and American astronomers using the photometer on the James Gregory Telescope in Scotland; using visual comparisons to the nearby bright star HD 80408,the star's light curve was better defined.
He looked through light curves that were flagged as eclipsing binaries by volunteers of the Planet Hunters citizen science project.[4].
As with the discovery of Kepler-9d, the Kepler team ran theinformation through numerous models to see if Kepler-11g's light curve could fit the profile of some other object, including an eclipsing binary star in the background that may have contaminated the data.
The study of the light curve, together with other observations, can give a lot of information about the physical process that produces it or constrain the physical theories about it.
After our largest survey to date,we have recently detected a strong candidate moon signal in the light curve of Kepler-1625b," the team wrote in a public request to observe the planet with the Hubble Space Telescope.
After several months, the light curve changes its decline rate again as positron emission becomes dominant from the remaining cobalt-56, although this portion of the light curve has been little-studied.
As a consequence, the orbiting debris field may be an"uneven ring of dust", causing erratic light fluctuations in the apparent luminosity of the parent star,as may have been responsible for the oddly flickering light curves associated with the starlight observed from certain variable stars, such as that from KIC 8462852, RZ Piscium and WD 1145+017.
For eclipsing variables, the shape of the light curve indicates the degree of totality, the relative sizes of the stars, and their relative surface brightnesses.
Others such as Miravariables have somewhat less regular light curves with large amplitudes of several magnitudes, while the semiregular variables are less regular still and have smaller amplitudes.[1].
In the late 1990s,a network of astronomers worldwide gathered light curve data that was ultimately used to derive the spin states and shape models of 10 new asteroids, including(165) Loreley.
The name"heartbeat" comes from the similarity of the light curve of the star with what a heartbeat looks like through an electrocardiogram if their brightness was mapped over time.[1] Many heartbeat stars have been discovered with the Kepler Space Telescope.[2].