[PDF] Top 20 A search for transiting planets in the β Pictoris system
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A search for transiting planets in the β Pictoris system
... extrasolar planets over twenty years ago through the radial velocity technique (Mayor & Queloz 1995; Marcy & Butler 1995) rapidly led to the detection of multiple planet systems (Butler et ...solar ... See full document
5
YETI – search for young transiting planets
... our search for young transiting planets at ages of 2 to 20 ...two transiting candidates were found so far, for which follow-up is partly ... See full document
5
A SEARCH FOR ADDITIONAL PLANETS IN THE NASA EPOXI OBSERVATIONS OF THE EXOPLANET SYSTEM GJ 436
... dwarf transiting exoplanet system GJ 436 obtained with the Extrasolar Planet Observation and Characterization (EPOCh) component of the NASA EPOXI ...a search of the high-precision time series for ... See full document
14
A search for transiting extrasolar planets in the open cluster NGC 4755
... Already, there are three small spacecrafts that have been sent to the orbit for transit observations, the Canadian MOST, French/ESA COROT and NASA Kepler. The first two were initially conceived with the primary objective ... See full document
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Planets in orbit around β Pictoris formed the orbital architecture of planetesimal belts?
... and β Pic dust are very much alike (Knacke et ...and β Pic dust, we do not find a reason that small dust particles dominate the scattering cross ...the β Pic debris disk have revealed an effect of ... See full document
6
A Simulation of Transit Timing Variation
... the search for exoplanets to simulate the transit timing varia- tion observed in the Kepler-19 ...planet transiting the star varies due to the gravitation- al effects of other planets orbiting the ... See full document
9
Three's company : an additional non transiting super Earth in the bright HD 3167 system, and masses for all three planets
... The proper motion of HD 3167 is quite large ( 107 mas yr −1 in R.A. and − 173 mas yr − 1 in decl.; Huber et al. 2016 ) . In the 63 years since, the 1953 Palomar Observatory Sky Survey ( POSS ) images, HD 3167 has moved ... See full document
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Detection of nitrogen gas in the β Pictoris circumstellar disc
... Re- search PlanetS supported by the Swiss National Science Foundation (SNSF), and has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and ... See full document
8
The L 98 59 system : three transiting, terrestrial size planets orbiting a nearby M dwarf
... respectively. The impact parameter had a uniform prior between zero and one plus the planet-to-star radius ratio. Eccentricity had a beta prior with α= 0.867 and β= 3.03 ( as suggested by Kipping 2013b ) , and ... See full document
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Post-conjunction detection of beta Pictoris b with VLT/SPHERE
... old β Pictoris is a unique proxy for the study of the early stages of planetary system formation and evolution, when giant planets are formed, Earth- mass planets may still be forming, ... See full document
7
Transiting exocomets detected in broadband light by TESS in the β Pictoris system
... the Transiting Exoplanet Survey Satel- lite (TESS; Ricker et ...sectors. β Pictoris (TIC 270577175, T = ...the β Pictoris observations in detail to exclude any systematic e ff ects or ... See full document
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Transiting exocomets detected in broadband light by TESS in the β Pictoris system
... modeling of the tail ejecta and its particle size distribution and the subsequent acceleration due to radiation pressure from the star, for different distributions of the sizes of the ejected parti- cles. Not knowing the ... See full document
8
Transiting extra solar planets in the field of open cluster NGC 7789
... detect planets of longer periods, conse quently probing larger orbital distances from the host ...extra-solar planets has increased the precision obtained from the RV measurements to around '^l-2ms~^ (Pepe ... See full document
175
The WASP-South search for transiting exoplanets
... 2006; 2007). The main limitations of the WASP design are the large pixels, often leading to blending, and the “red noise”, which usually exceeds photon noise at magnitudes brighter than 12. Red noise is introduced by ... See full document
6
Detection of nitrogen gas in the β pictoris circumstellar disk
... Research PlanetS supported by the Swiss National Science Foundation (SNSF), and has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation ... See full document
9
K2 114b and K2 115b : two transiting warm Jupiters
... The number of known transiting hot Jupiter exoplanets — gas giant exoplanets in short orbital periods of only a few days — is now in the few hundreds. Despite that large number there are still several open ... See full document
11
Two transiting earth-size planets near resonance orbiting a nearby cool star
... We also obtained near-infrared adaptive optics images of EPIC 206011691 at Keck Observatory on the night of 2015 July 24 UT. Observations were obtained with the 1024 × 1024 NIRC2 array and the natural guide star ... See full document
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Two massive rocky planets transiting a K dwarf 6 5 parsecs away
... of planets + orbits), then we used an adaptive Markov Chain Monte-Carlo (MCMC) code 9 to explore each of these solutions in terms of model marginal likelihood and posterior probability distribution functions ... See full document
23
Two small temperate planets transiting nearby M dwarfs in K2 campaigns 0 and 1
... our search of the K2 C0 data and is the fi rst validated planet from that fi ...of planets known as sub-Neptunes: planets smaller than Neptune with substantial H / He atmospheres ( Marcy et ...small ... See full document
15
On the search for transits of the planets orbiting Gliese 876
... Jupiter-mass planets are rarely asso- ciated with M ...giant planets orbiting red dwarfs seems to be a natural consequence of the core accre- tion theory of planet formation ( Laughlin et ...mass ... See full document
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