activity
19942019
most citedThe PLATO 2.0 Mission

1.3k citations · 2.6k across the 16 of their papers we have counts for

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Showing astro-ph.EPShow all

10 papers · 1 filter

astro-ph.EP2016★ 77 cited

Formation of bi-lobed shapes by sub-catastrophic collisions: A late origin of comet 67P/C-G's structure

M. Jutzi, W. Benz

The origin of the particular shape of a small body like comet 67P/Churyumov-Gerasimenko (67P/C-G) is a topic of active research. How and when it acquired its peculiar characteristi…

astro-ph.EP2016★ 56 cited

How primordial is the structure of comet 67P/C-G? Combined collisional and dynamical models suggest a late formation

M. Jutzi, W. Benz, A. Toliou +2

There is an active debate about whether the properties of comets as observed today are primordial or, alternatively, if they are a result of collisional evolution or other processe…

astro-ph.EP2014★ 37 cited

Planet Population Synthesis

W. Benz, S. Ida, Y. Alibert +2

With the increasing number of exoplanets discovered, statistical properties of the population as a whole become unique constraints on planet formation models provided a link betwee…

astro-ph.EP2013★ 1.3k cited

The PLATO 2.0 Mission

H. Rauer, C. Catala, C. Aerts +159

PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it…

astro-ph.EP2013★ 253 cited

CHEOPS: A Transit Photometry Mission for ESA's Small Mission Programme

C. Broeg, A. Fortier, D. Ehrenreich +18

Ground based radial velocity (RV) searches continue to discover exoplanets below Neptune mass down to Earth mass. Furthermore, ground based transit searches now reach milli-mag pho…

astro-ph.EP2012★ 141 cited

Planet formation models: the interplay with the planetesimal disc

A. Fortier, Y. Alibert, F. Carron +2

According to the sequential accretion model, giant planet formation is based first on the formation of a solid core which, when massive enough, can gravitationally bind gas from th…

astro-ph.EP2012★ 111 cited

Dust-trapping Rossby vortices in protoplanetary disks

H. Meheut, Z. Meliani, P. Varniere +1

One of the most challenging steps in planet formation theory is the one leading to the formation of planetesimals of kilometre size. A promising scenario involves the existence of…

astro-ph.EP2012★ 98 cited

Formation and long-term evolution of 3D vortices in protoplanetary discs

H. Meheut, R. Keppens, F. Casse +1

In the context of planet formation, anticyclonic vortices have recently received lots of attention for the role they can play in planetesimals formation. Radial migration of interm…

astro-ph.EP2011★ 4 cited

Application of recent results on the orbital migration of low mass planets: convergence zones

C. Mordasini, K. -M. Dittkrist, Y. Alibert +3

Previous models of the combined growth and migration of protoplanets needed large ad hoc reduction factors for the type I migration rate as found in the isothermal approximation. I…

astro-ph.EP2010★ 90 cited

CoRoT-10b: a giant planet in a 13.24 day eccentric orbit

A. S. Bonomo, A. Santerne, R. Alonso +47

The space telescope CoRoT searches for transiting extrasolar planets by continuously monitoring the optical flux of thousands of stars in several fields of view. We report the disc…