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20022026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2014 · astro-ph.EPShow all

7 papers · 2 filters

astro-ph.EP201432 cited

Can the masses of isolated planetary-mass gravitational lenses be measured by terrestrial parallax?

M. Freeman, L. C. Philpott, F. Abe +22

Recently Sumi et al. (2011) reported evidence for a large population of planetary-mass objects (PMOs) that are either unbound or orbit host stars in orbits > 10 AU. Their result wa…

astro-ph.EP201432 cited

A six-part collisional model of the main asteroid belt

Helena Cibulková, Miroslav Brož, Paula G. Benavidez

In this work, we construct a new model for the collisional evolution of the main asteroid belt. Our goals are to test the scaling law of Benz and Asphaug (1999) and ascertain if it…

astro-ph.EP201444 cited

Physical and dynamical properties of the main belt triple asteroid (87) Sylvia

J. Berthier, Frédéric Vachier, Franck Marchis +2

We present the analysis of high angular resolution observations of the triple Asteroid (87) Sylvia collected with three 8-10 m class telescopes (Keck, VLT, Gemini North) and the Hu…

astro-ph.EP201447 cited

Excitation of the Orbital Inclination of Iapetus during Planetary Encounters

David Nesvorny, David Vokrouhlicky, Rogerio Deienno +1

Saturn's moon Iapetus has an orbit in a transition region where the Laplace surface is bending from the equator to the orbital plane of Saturn. The orbital inclination of Iapetus t…

astro-ph.EP201451 cited

Space weathering simulations through controlled growth of iron nanoparticles on olivine

T. Kohout, J. Čuda, J. Filip +9

Airless planetary bodies are directly exposed to space weathering. The main spectral effects of space weathering are darkening, reduction in intensity of silicate mineral absorptio…

astro-ph.EP201467 cited

Orbital Perturbations of the Galilean Satellites During Planetary Encounters

R. Deienno, D. Nesvorny, D. Vokrouhlicky +1

The Nice model of the dynamical instability and migration of the giant planets can explain many properties of the present Solar System, and can be used to constrain its early archi…