[PDF] Top 20 On the search for transits of the planets orbiting Gliese 876
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On the search for transits of the planets orbiting Gliese 876
... to search for transits by the P 30 day and P 60 day outer planets of the three-planet system orbiting the nearby M dwarf Gl ...two planets experience strong mutual perturbations, which ... See full document
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A SEARCH FOR ADDITIONAL PLANETS IN THE NASA EPOXI OBSERVATIONS OF THE EXOPLANET SYSTEM GJ 436
... a search of the high-precision time series for additional planets around GJ 436, which could be revealed either directly through their photometric transits or indirectly through the variations these ... See full document
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Spectroscopic transit search: a self-calibrating method for detecting planets around bright stars
... A majority of the exoplanets discovered to date has been through the simultaneous photometric monitoring of several thousands of stars and looking for the decrement in stellar flux as a com- panion transits the ... See full document
8
Wide angle search for extrasolar planets by the transit method
... transit search on the PASS0 and SuperWASP lightcurves from Chapters 3 and 4 using the AoVtr ...we search for transits, we find no convincing candidates, and we would require more observations for 5 ... See full document
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The Anglo-Australian planet search. XXV. A candidate massive Saturn analog orbiting HD 30177
... separated planets, the inclination between the two orbits seems to play a minimal role in their ...the planets; from a dynamical point of view, given the assumption that the two planets formed in a ... See full document
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A Search for Additional Planets in Five of the Exoplanetary Systems Studied by the Nasa Epoxi Mission
... known transits in each data set by iteratively excluding those observations (using an ephemeris for the known planet derived from the EPOCh observations) from the points used to generate the flat- field surface, ... See full document
11
The little dippers : transits of star grazing exocomets?
... The search was conducted using LcTools, 1 a free and publicly available software program that provides a set of applications for efficiently building and visually inspecting large numbers of light curves (Kip- ... See full document
15
A Lack of Planets in 47 Tucanae from a Hubble Space Telescope Search*
... of transits, and density of sampling such that a (Gaussian noise) rms value falling below this curve would provide greater than ...two transits in each ...shorter transits, the S/N for which is ... See full document
6
A search for transiting planets in the β Pictoris system
... for transits from the ground for magnitudes from 8 to 10 (Pepper et ...measuring transits around bright stars via space ...PLAnetary Transits and Oscillations of stars ...terrestrial planets ... See full document
5
Three newly discovered sub Jupiter mass planets : WASP 69b and WASP 84b transit active K dwarfs and WASP 70Ab transits the evolved primary of a G4+K3 binary
... a search for transits on each season of data from each camera separately and we perform combined searches on all WASP data available on each star, allowing for photometric off- sets between data ...shallow ... See full document
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The little dippers: transits of star-grazing exocomets?
... The search was conducted using LcTools, 1 a free and publicly available software program that provides a set of applications for efficiently building and visually inspecting large numbers of light curves (Kip- ... See full document
14
The Pan-Pacific planet search. VI. Giant planets orbiting HD 86950 and HD 222076
... the large uncertainty can be attributed to phase gaps which allow for a family of high-eccentricity solutions. As in our previous work, we checked the All-Sky Automated Survey ( ASAS ) V-band photometric data ( Pojmanski ... See full document
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The Anglo-Australian planet search. XX. A solitary ice-giant planet orbiting HD 102365
... three planets noted above with similar properties to HD 102365b (Gl 876e, HD 69830d & Gl 581f) all lie in multiple ...(Gl 876 and Gl 581) host four and six exoplanets, ...additional planets (see ... See full document
19
From Jets to GEMSS*: pan-spectral detection, observation and characterization of the M-Dwarf Exoplanet System Gliese 876 - and beyond. Transit photometry, radial velocity, and millimeter interferometry to constrain and characterize the nearest multiple planet system
... Gl 876 system ( Marcy et al. 2001; Rivera et al. 2005). The two planets induce a total ve- locity half-amplitude of the star of nearly ...three planets, all orbiting the star in the same ... See full document
152
Three planets orbiting Wolf 1061
... The NASA Kepler mission has demonstrated that a high fraction of low-mass stars are planet hosts ( Dressing & Charbonneau 2013, 2015; Kopparapu 2013 ) , and the evidence is mounting that multi-planet systems are ... See full document
7
From Jets to GEMSS*: pan-spectral detection, observation and characterization of the M-Dwarf Exoplanet System Gliese 876 - and beyond. Transit photometry, radial velocity, and millimeter interferometry to constrain and characterize the nearest multiple planet system
... with transits by the outer two planets, one using radial velocities and one using ...planet transits in front of its star, an asymmetry in the star’s spectral lines is produced since parts of the ... See full document
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The Anglo-Australian planet search. XX. A solitary ice-giant planet orbiting HD 102365
... three planets noted above with similar properties to HD 102365 b (Gl 876e, HD 69830d, and Gl 581f) all lie in multiple ...(Gl 876 and Gl 581) host four and six exoplanets, ...additional planets (see ... See full document
7
Elevation Variation with Low Earth Orbiting Search and Rescue Satellites for the Station Implemented in Kosovo
... Receive-only ground stations, specifically computer based designed systems, to track the search and rescue satellites as they pass across the sky are called Local User Terminals (LUT). The LUTs are fully automated ... See full document
6
Transits and starspots in the WASP 6 planetary system
... By determining λ and ψ of the planetary system, it is possible to begin to understand the primary process in the dynamical evolution of the system. The RM effect can be used to ascertain a value for λ . One limitation of ... See full document
10
Exoplanet transits as the foundation of an interstellar communications network
... of planets experience perturba- tions from their neighbouring planets, from companion stars if they are present, and from close encounters with neighbouring stars (provided that the encounter is ... See full document
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