activity
20102021
most citedThe D/H ratio in the atmospheres of Uranus and Neptune from Herschel PACS observations

110 citations · 572 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2021★ 38 cited

First direct measurement of auroral and equatorial jets in the stratosphere of Jupiter

T. Cavalié, B. Benmahi, V. Hue +11

Context. The tropospheric wind pattern in Jupiter consists of alternating prograde and retrograde zonal jets with typical velocities of up to 100 m/s around the equator. At much hi…

astro-ph.EP2020★ 7 cited

18-year long monitoring of the evolution of H2O vapor in the stratosphere of Jupiter with the Odin space telescope

B. Benmahi, T. Cavalié, M. Dobrijevic +14

Comet Shoemaker-Levy 9 impacted Jupiter in July 1994, leaving its stratosphere with several new species, among them water vapor (H2O). With the aid of a photochemical model H2O can…

astro-ph.EP2019★ 26 cited

Herschel map of Saturn's stratospheric water, delivered by the plumes of Enceladus

T. Cavalié, V. Hue, P. Hartogh +13

Context. The origin of water in the stratospheres of Giant Planets has been an outstanding question ever since its first detection by ISO some 20 years ago. Water can originate fro…

astro-ph.SR2018

Line identifications in the spectrum of Lupi A

R. Monier, T. Kılıçoğlu

We present new abundance determinations for the sharp-lined HgMn star χ Lupi A from archival FEROS spectra. Selected unblended lines with accurate atomic data have been synthesized…

astro-ph.IM2018

Multi-scale three-dimensional visualization of emission, scattering and absorption in active galactic nuclei using Virtual Observatories tools

F. Marin, J. Desroziers, A. Schaaff

Whether aimed for the study of the planetary systems, the distribution of the stars in the galaxies or the formation of the large-scale structures in the Universe, the sizes of num…

astro-ph.EP2017★ 100 cited

Scientific rationale for Uranus and Neptune in situ explorations

O. Mousis, D. H. Atkinson, T. Cavalié +53

The ice giants Uranus and Neptune are the least understood class of planets in our solar system but the most frequently observed type of exoplanets. Presumed to have a small rocky…

astro-ph.SR2017★ 101 cited

Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars

Gaia Collaboration, G. Clementini, L. Eyer +588

Parallaxes for 331 classical Cepheids, 31 Type II Cepheids and 364 RR Lyrae stars in common between Gaia and the Hipparcos and Tycho-2 catalogues are published in Gaia Data Release…

astro-ph.EP2013★ 110 cited

The D/H ratio in the atmospheres of Uranus and Neptune from Herschel PACS observations

H. Feuchtgruber, E. Lellouch, G. Orton +9

Herschel-PACS measurements of the rotational R(0) and R(1) HD lines in the atmospheres of Uranus and Neptune are analyzed in order to derive a D/H ratio with improved precision for…

astro-ph.EP2010★ 24 cited

First results on Martian carbon monoxide from Herschel/HIFI observations

P. Hartogh, M. I. Błęcka, C. Jarchow +48

We report on the initial analysis of Herschel/HIFI carbon monoxide (CO) observations of the Martian atmosphere performed between 11 and 16 April 2010. We selected the (7-6) rotatio…

astro-ph.EP2010★ 80 cited

Herschel/HIFI observations of Mars: first detection of O_2 at submillimetre wavelengths and upper limits on HCl and H_2O_2

P. Hartogh, C. Jarchow, E. Lellouch +47

We report on an initial analysis of Herschel/HIFI observations of hydrogen chloride (HCl), hydrogen peroxide (H_2O_2), and molecular oxygen (O_2) in the Martian atmosphere performe…

astro-ph.EP2010★ 76 cited

First results of Herschel/PACS observations of Neptune

E. Lellouch, P. Hartogh, H. Feuchtgruber +51

We report on the initial analysis of a Herschel/PACS full range spectrum of Neptune, covering the 51-220 micrometer range with a mean resolving power of ~ 3000, and complemented by…

astro-ph.EP2010★ 10 cited

The Herschel-SPIRE submillimetre spectrum of Mars

B. M. Swinyard, P. Hartogh, S. Sidher +44

We have obtained the first continuous disk averaged spectrum of Mars from 450 to 1550 Ghz using the Herschel-SPIRE Fourier Transform Spectrometer. The spectrum was obtained at a co…