Publications

@article{HilgenZeeden2020a,

title = {Paleoclimate records reveal elusive∼ 200-kyr eccentricity cycle for the first time},

author = {Frits Hilgen and Christian Zeeden and Jacques Laskar},

year  = {2020},

date = {2020-01-01},

journal = {Global and Planetary Change},

volume = {194},

pages = {103296},

note = {Publisher: Elsevier},

keywords = {},

pubstate = {published},

tppubtype = {article}

}

@article{GalbrunBoulila2020a,

title = {" Short" or" long" Rhaetian? Astronomical calibration of Austrian key sections},

author = {Bruno Galbrun and Slah Boulila and Leopold Krystyn and Sylvain Richoz and Silvia Gardin and Annachiara Bartolini and Martin Maslo},

year  = {2020},

date = {2020-01-01},

journal = {Global and Planetary Change},

volume = {192},

pages = {103253},

note = {Publisher: Elsevier},

keywords = {},

pubstate = {published},

tppubtype = {article}

}

@article{BoulilaCharbonnier2020a,

title = {Unraveling short-and long-term carbon cycle variations during the Oceanic Anoxic Event 2 from the Paris Basin Chalk},

author = {Slah Boulila and Guillaume Charbonnier and Jorge E. Spangenberg and Silvia Gardin and Bruno Galbrun and Justine Briard and Laurence Le Callonnec},

year  = {2020},

date = {2020-01-01},

journal = {Global and Planetary Change},

volume = {186},

pages = {103126},

note = {Publisher: Elsevier},

keywords = {},

pubstate = {published},

tppubtype = {article}

}

@article{BoulilaBrange2020a,

title = {Astronomical pacing of Late Cretaceous third-and second-order sea-level sequences in the Foz do Amazonas Basin},

author = {Slah Boulila and Célia Brange and Alberto Machado Cruz and Jacques Laskar and Christian Gorini and Tadeu Dos Reis and Cleverson Guizan Silva},

year  = {2020},

date = {2020-01-01},

journal = {Marine and Petroleum Geology},

volume = {117},

pages = {104382},

note = {Publisher: Elsevier},

keywords = {},

pubstate = {published},

tppubtype = {article}

}

@article{FiengaDeram2019a,

title = {INPOP19a planetary ephemerides},

author = {A. Fienga and P. Deram and V. Viswanathan and A. Di Ruscio and L. Bernus and D. Durante and M. Gastineau and J. Laskar},

url = {https://ui.adsabs.harvard.edu/abs/2019NSTIM.109.....F},

year  = {2019},

date = {2019-12-01},

urldate = {2022-12-01},

journal = {Notes Scientifiques et Techniques de l'Institut de Mecanique Celeste},

volume = {109},

abstract = {INPOP19a is the new ephemerides for the orbits of the 8 planets of the solar system, the moon, Pluto as well as 14000 asteroids. It is fitted over about 155000 planetary observations including 9 positions of Jupiter deduced from the Juno mission, an extension of the Cassini data sample from 2014 to 2017 for the Saturn orbit and of the MEX data from 2016.4 to 2017.4 for the Mars orbit. The asteroid orbits were fitted on the almost 2 millions of observations obtained by the GAIA mission and delivered with the DR2. The INPOP dynamical modeling was also modified in comparison to the previous version, INPOP17a. A ring modeling the accelerations induced by Trans-Neptunian objects as well as the 9 most massive TNOs have been added in order to improve the fit to the Saturn observations. A new estimation of the TNO ring mass has been produced. Finally, a new Bayesian procedure for the computation of the masses of 343 main-belt asteroids has been applied and leads to an important improvement in the accuracy of the Mars orbit and of its extrapolation capabilities.},

note = {ADS Bibcode: 2019NSTIM.109.....F},

keywords = {},

pubstate = {published},

tppubtype = {article}

}

@article{BernusMinazzoli2019a,

title = {Constraining the Mass of the Graviton with the Planetary Ephemeris INPOP},

author = {L. Bernus and O. Minazzoli and A. Fienga and M. Gastineau and J. Laskar and P. Deram},

url = {https://ui.adsabs.harvard.edu/abs/2019PhRvL.123p1103B},

doi = {10.1103/PhysRevLett.123.161103},

issn = {0031-9007},

year  = {2019},

date = {2019-10-01},

urldate = {2022-12-01},

journal = {Physical Review Letters},

volume = {123},

pages = {161103},

abstract = {We use the planetary ephemeris INPOP17b to constrain the existence of a Yukawa suppression to the Newtonian potential, generically associated with the graviton's mass. We also give an interpretation of this result for a specific case of fifth force framework. We find that the residuals for the Cassini spacecraft significantly (90% C.L.) degrade for Compton wavelengths of the graviton smaller than 1.83 ×1013 km , which correspond to a graviton mass bigger than 6.76 ×10-23 eV /c2. This limit is comparable in magnitude to the one obtained by the LIGO-Virgo Collaboration in the radiative regime. We also use this specific example to defend that constraints on alternative theories of gravity obtained from postfit residuals may be generically overestimated.},

note = {ADS Bibcode: 2019PhRvL.123p1103B},

keywords = {},

pubstate = {published},

tppubtype = {article}

}

@article{RambauxViswanathan2019a,

title = {Dynamical model of lunar core and observational constraint from Lunar Laser Ranging},

author = {Nicolas Rambaux and Vishnu Viswanathan and Agnes Fienga and Jacques Laskar and Mickael Gastineau},

url = {https://ui.adsabs.harvard.edu/abs/2019EPSC...13.1607R},

year  = {2019},

date = {2019-09-01},

urldate = {2022-12-01},

volume = {2019},

pages = {EPSC--DPS2019--1607},

abstract = {Our Moon is one of the most studied objects in the Solar system; we benefit from chemical, geophysical, and geodetical observations achieved by multiple Earth ground based telescopes and in situ missions such as GRAIL and Apollo. However, its deep interior properties remains a puzzle because the lunar core is very small implying small signature in the observational data set. This paper focuses on the description of a new lunar core rotational model included in INPOP and used to provide a determination of the radius and geometry of the lunar core-mantle boundary (CMB) from the LLR observations.},

note = {Conference Name: EPSC-DPS Joint Meeting 2019 ADS Bibcode: 2019EPSC...13.1607R},

keywords = {},

pubstate = {published},

tppubtype = {article}

}