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20012026
most citedThe PLATO 2.0 Mission

1.3k citations · 9.4k across the 163 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.EP2013★ 50 cited

Herschel HIFI observations of ionised carbon in the β Pictoris debris disk

G. Cataldi, A. Brandeker, G. Olofsson +9

Context: The dusty debris disk around the 20 Myr old main-sequence A-star β Pictoris is known to contain gas. Evidence points towards a secondary origin of the gas as opposed…

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★ 35 cited

High angular resolution imaging and infrared spectroscopy of CoRoT candidates

E. W. Guenther, M. Fridlund, R. Alonso +16

Studies of transiting extrasolar planets are of key importance for understanding the nature of planets outside our solar system because their masses, diameters, and bulk densities…

astro-ph.SR2013★ 220 cited

DUst Around NEarby Stars. The survey observational results

C. Eiroa, J. P. Marshall, A. Mora +47

Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system's counterparts are the asteroid and Edgew…

astro-ph.EP2013★ 47 cited

Kepler-77b: a very low albedo, Saturn-mass transiting planet around a metal-rich solar-like star

D. Gandolfi, H. Parviainen, M. Fridlund +18

We report the discovery of Kepler-77b (alias KOI-127.01), a Saturn-mass transiting planet in a 3.6-day orbit around a metal-rich solar-like star. We combined the publicly available…

astro-ph.EP2013★ 32 cited

CoRoT 101186644: A transiting low-mass dense M-dwarf on an eccentric 20.7-day period orbit around a late F-star

L. Tal-Or, T. Mazeh, R. Alonso +10

We present the study of the CoRoT transiting planet candidate 101186644, also named LRc01_E1_4780. Analysis of the CoRoT lightcurve and the HARPS spectroscopic follow-up observatio…