Sentences with phrase «photometry timing»
The occultation photometry timing is consistent with a circular orbit, at e < 0.01 (1 -LCB- \ sigma -RCB--RRB-, and e < 0.09 (3 -LCB- \ sigma -RCB--RRB-.
https://arxiv.org/ Not exact matches
For these studies we use the high - precision time - resolved Hubble Space Telescope near - infrared spectroscopy and Spitzer Space Telescope photometry in multiple programs.
This unique and unprecedented coverage is the first time that a nova has any substantial amount of fast photometry.
The presence of a second, non-transiting planet was inferred from the transit time variations (TTVs) of Kepler - 19b, over 8 quarters of Kepler photometry, although neither mas... ▽ More We report a detailed characterization of the Kepler - 19 system.
The presence of a second, non-transiting planet was inferred from the transit time variations (TTVs) of Kepler - 19b, over 8 quarters of Kepler photometry, although neither mass nor period could be determined.
Although AIJ maintains the general purpose image processing capabilities of ImageJ, AIJ is streamlined for time - series differential photometry, light curve detrending and fitting, and light curve plotting, especially for applications requiring ultra-precise light curves (e.g., exoplanet transits).
The data returned from Kepler are unique in terms of the number of stars observed, precision of photometry for time series observations, and the temporal extent of high duty cycle observations.
Of these candidates, 219 are new in this catalog and include two new candidates in multi-planet systems (KOI - 82.06 and KOI... ▽ More We present the Kepler Object of Interest (KOI) catalog of transiting exoplanets based on searching four years of Kepler time series photometry (Data Release 25, Q1 — Q17).
Abstract: We present the Kepler Object of Interest (KOI) catalog of transiting exoplanets based on searching four years of Kepler time series photometry (Data Release 25, Q1 — Q17).
... ▽ More Early time - series photometry from NASA's Kepler spacecraft has revealed a planet transiting the star we term Kepler - 4, at RA = 19h02m27.68 s, Dec = +50:08:08.7.
For an additional candidate, we present multi-color follow - up photometry during a subsequent time of eclipse, which reveals that this candidate consists of a blend of an eclipsing binary and a physically unassociated star.
The characteristics of the host star are well constrained by high - resolution spectroscopy combined with an asteroseismic analysis of the Kepler photometry, leading to an estimated mass and radius of 0.970 + / - 0.060 M... ▽ More A search of the time - series photometry from NASA's Kepler spacecraft reveals a transiting planet candidate orbiting the 11th magnitude G5 dwarf KIC 10593626 with a period of 290 days.
Abstract: A search of the time - series photometry from NASA's Kepler spacecraft reveals a transiting planet candidate orbiting the 11th magnitude G5 dwarf KIC 10593626 with a period of 290 days.