Sean N. Raymond researcher, astrophysicist
Raymond, Sean N.
![Sudoc [ABES], France](/viaf/images/flags/SUDOC.png "Sudoc [ABES], France")
VIAF ID: 306317210 (Personal)
Permalink: http://viaf.org/viaf/306317210
Preferred Forms
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100 1 _
‡a
Raymond , Sean N.
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100 1 _
‡a
Raymond, Sean N.
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100 0 _
‡a
Sean N. Raymond
‡c
researcher, astrophysicist
4xx's: Alternate Name Forms (2)
Works
| Title | Sources |
|---|---|
| Comets III |
|
| Constraining the origin of Earth’s volatiles with dynamical simulations and isotopic measurements of noble gases in meteorites. |
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| Déterminer l'origine des éléments volatils terrestres à l'aide de simulations dynamiques et de mesures isotopiques de gaz rares dans les météorites |
|
| Effet de la structure du disque sur la formation et la migration des planètes |
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| Etude des disques de débris avec un modèle numérique de nouvelle génération |
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| Evolution et habitabilité de systèmes planétaires autour d’étoiles de faible masse et de naines brunes |
|
| Exoplanetary Systems Dynamics. |
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| The far-infrared/radio correlation as probed byHerschel |
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| Formation of planetary systems by pebble accretion and migration: growth of gas giants |
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| Gas Giant Planets as Dynamical Barriers to Inward-Migrating Super-Earths |
|
| Generalized milankovitch cycles and long-term climatic habitability |
|
| The Grand Tack model: a critical review |
|
| The habitability of Proxima Centauri b. II. Possible climates and observability |
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| The HD 40307 planetary system: super-Earths or mini-Neptunes? |
|
| HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements |
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| HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm |
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| The HerMES SPIRE submillimeter local luminosity function |
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| HerMES: The submillimeter spectral energy distributions ofHerschel/SPIRE-detected galaxies |
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| The Herschel multi-tiered extragalactic survey: SPIRE-mm photometric redshifts |
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| High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT) |
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| Hot super-Earths and giant planet cores from different migration histories |
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| Impact, Hit and Run |
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| Implications de la chimie du xénon sur les contextes planétaire et nucléaire |
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| In-Situ Exploration of Objects on Oort Cloud Comet Orbits: OCCs, Manxes and ISOs |
|
| Is there an exoplanet in the Solar system? |
|
| Isolation Mass |
|
| Lindblad Resonance |
|
| A low mass for Mars from Jupiter's early gas-driven migration |
|
| Making other earths: dynamical simulations of terrestrial planet formation and water delivery |
|
| Making systems of Super Earths by inward migration of planetary embryos |
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| Mars’ growth stunted by an early giant planet instability |
|
| Mathematical encoding within multiresonant planetary systems as SETI beacons |
|
| Mean Motion Resonances from Planet-Planet Scattering |
|
| Mercury as the Relic of Earth and Venus Outward Migration |
|
| The Nature and Origins of Sub-Neptune Size Planets |
|
| The nature of the TRAPPIST-1 exoplanets |
|
| New worlds on the horizon: Earth-sized planets close to other stars |
|
| Nice Model |
|
| Orbital Period |
|
| The origins of nearly coplanar, non-resonant systems of close-in super-Earths |
|
| Outward Migration of Jupiter and Saturn in 3:2 or 2:1 Resonance in Radiative Disks: Implications for the Grand Tack and Nice Models |
|
| Planet formation imager: science vision and key requirements |
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| Planet–planet scattering as the source of the highest eccentricity exoplanets |
|
| Planet-planet scattering leads to tightly packed planetary systems |
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| Planetary system disruption by Galactic perturbations to wide binary stars. |
|
| Planetesimal rings as the cause of the Solar System’s planetary architecture |
|
| Les poussières et petits corps des systèmes planétaires extrasolaires |
|
| Purge, excitation dynamique et structuration des disques de débris soumis à l'interaction gravitationnelle de planètes et d'étoiles voisines |
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| Q* (Specific Energy to Destroy an Object) |
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| Realistic survey simulations for kilometer class near Earth objects |
|
| Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides |
|
| The roles of tidal evolution and evaporative mass loss in the origin of CoRoT-7 b |
|
| Rossiter-McLaughlin observations of 55 Cnc e |
|
| Runaway Growth |
|
| The science of exoplanets and their systems |
|
| The Search for Other Earths: Limits on the Giant Planet Orbits That Allow Habitable Terrestrial Planets to Form |
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| Secular behavior of exoplanets: self-consistency and comparisons with the planet-planet scattering hypothesis |
|
| Shaping of the Inner Solar System by the Gas-Driven Migration of Jupiter |
|
| Shepherding |
|
| Spectroscopic Properties of Cool Stars in the Sloan Digital Sky Survey: An Analysis of Magnetic Activity and a Search for Subdwarfs |
|
| A Strategy for Finding Near-Earth Objects with the SDSS Telescope |
|
| Stripping, dynamical excitation and structuring of debris disks undergoing gravitational interactions from neighbouring planets of stars. |
|
| Study of debris discs with a new generation numerical model. |
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| The Successful Prediction of the Extrasolar Planet HD 74156d |
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| Survivor Bias: Divergent Fates of the Solar System’s Ejected versus Persisting Planetesimals |
|
| Terrestrial planet formation constrained by Mars and the structure of the asteroid belt |
|
| Terrestrial planet formation in extra-solar planetary systems |
|
| Thermal Processing of Jupiter-family Comets during Their Chaotic Orbital Evolution |
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| Tidal dissipation and eccentricity pumping: implications for the depth of the secondary eclipse of 55 Cancri e |
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| Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186 |
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| Tides and the evolution of planetary habitability |
|
| TOI-4336 A b: A temperate sub-Neptune ripe for atmospheric characterization in a nearby triple M-dwarf system |
|
| TRAPPIST-1: Global results of the Spitzer Exploration Science Program Red Worlds |
|
| Vortex, Vortices |
|
| Water delivery and giant impacts in the ‘Grand Tack’ scenario |
|
