activity
20092026
most citedKepler Mission Design, Realized Photometric Performance, and Early Science

1.2k citations · 10.1k across the 44 of their papers we have counts for

collaborators

45 papers

astro-ph.EP2026

Energy distributions of precipitating electrons in Jupiter's auroral regions from combined Juno/JADE and Juno/JEDI measurements

B. Benmahi, V. Hue, N. André +17

Jupiter's auroras are produced by magnetospheric electrons precipitating into its atmosphere. Juno/JADE and Juno/JEDI together measure these electrons from 100 eV to 1 MeV. However…

astro-ph.EP2023★ 3 cited

Humid Evolution of Haze in the Atmosphere of Super-Earths in the Habitable Zone

Julien Maillard, Nathalie Carrasco, Christopher P. Rüger +8

Photochemical hazes are expected to form and significantly contribute to the chemical and radiative balance of exoplanets with relatively moderate temperatures, possibly in the hab…

astro-ph.EP2022

Moonraker -- Enceladus Multiple Flyby Mission

O. Mousis, A. Bouquet, Y. Langevin +50

Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could b…

astro-ph.EP2021★ 1 cited

Science goals and new mission concepts for future exploration of Titan's atmosphere geology and habitability: Titan POlar Scout/orbitEr and In situ lake lander and DrONe explorer (POSEIDON)

Sébastien Rodriguez, Sandrine Vinatier, Daniel Cordier +61

In response to ESA Voyage 2050 announcement of opportunity, we propose an ambitious L-class mission to explore one of the most exciting bodies in the Solar System, Saturn largest m…

astro-ph.EP2020★ 180 cited

The Occurrence of Rocky Habitable Zone Planets Around Solar-Like Stars from Kepler Data

Steve Bryson, Michelle Kunimoto, Ravi K. Kopparapu +79

We present occurrence rates for rocky planets in the habitable zones (HZ) of main-sequence dwarf stars based on the Kepler DR25 planet candidate catalog and Gaia-based stellar prop…

astro-ph.EP2020★ 16 cited

Interaction dust-plasma in Titan's ionosphere: an experimental simulation of aerosols erosion

Audrey Chatain, Nathalie Carrasco, Nathalie Ruscassier +3

Organic aerosols accumulated in Titan's orange haze start forming in its ionosphere. This upper part of the atmosphere is highly reactive and complex ion chemistry takes place at a…

astro-ph.EP2020★ 14 cited

Compositional Measurements of Saturn's Upper Atmosphere and Rings from Cassini INMS

J. Serigano, S. M. Hörst, C. He +4

The Cassini spacecraft's last orbits directly sampled Saturn's thermosphere and revealed a much more chemically complex environment than previously believed. Observations from the…

astro-ph.EP2019★ 17 cited

Positive Ion Chemistry in an N-CH Plasma Discharge: Key Precursors to the Growth of Titan Tholins

David Dubois, Nathalie Carrasco, Lora Jovanovic +3

Titan is unique in the solar system as it hosts a dense atmosphere mainly made of N and CH. Cassini-Huygens revealed the presence of an intense atmospheric photochemistry i…

astro-ph.EP2019★ 1 cited

An EUV Non-Linear Optics Based Approach to Study the Photochemical Processes of Titanś Atmosphere

Jérémy Bourgalais, Nathalie Carrasco, Ludovic Vettier +6

In situ exploration of the planetary atmospheres requires the development of laboratory experiments to understand the molecular growth pathways initiated by photochemistry in the u…

astro-ph.EP2019★ 18 cited

Structural study of analogues of Titan s haze by trapped ion mobility coupled with a Fourier transform ion cyclotron mass spectrometer

Christopher P. Rueger, Julien Maillard, Johann Le Maitre +8

The aerosols present in the atmosphere of the Saturn s moon Titan are of particular planetary science interest and several spacecraft missions already allowed to gather spectroscop…

astro-ph.EP2018★ 9 cited

Detection opportunity for aromatic signature in Titan s aerosols in the 4.1 to 5.3 micron range

Christophe Mathé, Thomas Gautier, Melissa G. Trainer +1

The Cassini/Huygens mission provided new insights on the chemistry of the upper atmosphere of Titan. The presence of large molecules and ions (>100 s of amu) detected by Cassini at…

astro-ph.EP2018★ 60 cited

Comparison of soluble and insoluble organic matter in analogues of Titan s aerosols

Julien Maillard, Nathalie Carrasco, Isabelle Schmitz-Afonso +2

Titan, the biggest moon of Saturn, has a thick atmosphere which presents similarities with the one thought to be on Earth at its beginning. The study of Titan s photochemical haze…

astro-ph.EP2017★ 26 cited

Titan organic aerosols: molecular composition and structure of laboratory analogues inferred from systematic pyrolysis gas chromatography mass spectrometry analysis

Marietta Morissona, Cyril Szopa, Nathalie Carrasco +2

Numerous studies have been carried out to characterize the chemical composition of laboratory analogues of Titan aerosols (tholins), but their molecular composition as well as thei…

astro-ph.EP2017★ 14 cited

Molecular Isomer Identification of Titan Tholins Organic Aerosols by Photoelectron/Photoion Coincidence Spectroscopy Coupled to VUV Synchrotron Radiation

Barbara Cunha-de-Miranda, Gustavo Garcia, François Gaie-Levrel +6

The chemical composition of Titan organic haze is poorly known. To address this issue, laboratory analogs named tholins are synthesized, and analyzed by methods requiring often an…

astro-ph.EP2017★ 7 cited

Decay of COSAC and Ptolemy Mass Spectra at Comet 67P/Churyumov-Gerasimenko

Harald Krüger, Fred Goesmann, Chaitanya Giri +11

The Rosetta lander Philae successfully landed on the nucleus of comet 67P/Churyumov-Gerasimenko on 12 November 2014. Philae is equipped with two gas analyzers: The Cometary Samplin…

astro-ph.EP2016★ 32 cited

Development of HPLC-Orbitrap method for identification of N-bearing molecules in complex organic material relevant to planetary environments

Thomas Gautier, Isabelle Schmitz-Afonso, David Touboul +3

Although the Cassini Spacecraft and the Huygens lander provided numerous information about Titan atmospheric chemistry and the formation of its aerosols, the exact composition of t…

astro-ph.EP2015★ 264 cited

Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)

F. Mullally, Jeffrey L. Coughlin, Susan E. Thompson +56

\We present the sixth catalog of Kepler candidate planets based on nearly 4 years of high precision photometry. This catalog builds on the legacy of previous catalogs released by t…

astro-ph.EP2013★ 231 cited

Planetary Candidates Observed by Kepler IV: Planet Sample From Q1-Q8 (22 Months)

Christopher J. Burke, Stephen T. Bryson, F. Mullally +37

We provide updates to the Kepler planet candidate sample based upon nearly two years of high-precision photometry (i.e., Q1-Q8). From an initial list of nearly 13,400 Threshold Cro…

astro-ph.EP2013★ 255 cited

Kepler-62: A five-planet system with planets of 1.4 and 1.6 Earth radii in the Habitable Zone

W. J. Borucki, E. Agol, F. Fressin +62

We present the detection of five planets -- Kepler-62b, c, d, e, and f -- of size 1.31, 0.54, 1.95, 1.61 and 1.41 Earth radii, orbiting a K2V star at periods of 5.7, 12.4, 18.2, 12…

astro-ph.EP2012★ 119 cited

On The Relative Sizes of Planets Within Kepler Multiple Candidate Systems

David R. Ciardi, Daniel C. Fabrycky, Eric B. Ford +5

We present a study of the relative sizes of planets within the multiple candidate systems discovered with the mission. We have compared the size of each planet to the size…

astro-ph.EP2012★ 484 cited

The Transiting Circumbinary Planets Kepler-34 and Kepler-35

William F. Welsh, Jerome A. Orosz, Joshua A. Carter +43

Most Sun-like stars in the Galaxy reside in gravitationally-bound pairs of stars called "binary stars". While long anticipated, the existence of a "circumbinary planet" orbiting su…

astro-ph.EP2012★ 1.1k cited

Planetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data

Natalie M. Batalha, Jason F. Rowe, Stephen T. Bryson +69

New transiting planet candidates are identified in sixteen months (May 2009 - September 2010) of data from the Kepler spacecraft. Nearly five thousand periodic transit-like signals…

astro-ph.EP2012★ 117 cited

Kepler-20: A Sun-like Star with Three Sub-Neptune Exoplanets and Two Earth-size Candidates

Thomas N. Gautier, David Charbonneau, Jason F. Rowe +41

We present the discovery of the Kepler-20 planetary system, which we initially identified through the detection of five distinct periodic transit signals in the Kepler light curve…

astro-ph.EP2012★ 186 cited

Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations

Jason H. Steffen, Daniel C. Fabrycky, Eric B. Ford +45

We present a method to confirm the planetary nature of objects in systems with multiple transiting exoplanet candidates. This method involves a Fourier-Domain analysis of the devia…