133 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR7 papers
- Institut d'Astrophysique SpatialeFR3 papers
- Université de LilleFR3 papers
- California Institute of TechnologyUS2 papers
- Infrared Processing and Analysis CenterUS2 papers
- Institut de Recherche en Astrophysique et PlanétologieFR2 papers
- Leibniz Institute for Tropospheric ResearchDE2 papers
- Leipzig UniversityDE2 papers
- Ludwig-Maximilians-Universität MünchenDE2 papers
- National Institute for AstrophysicsIT2 papers
- PhysicoChimie des Processus de Combustion et de l'AtmosphèreFR2 papers
- Université Fédérale de Toulouse Midi-PyrénéesFR2 papers
11 papers
Typical daily profiles of PM concentrations in parisian underground railway stations
Valisoa Rakotonirinjanahary, Suzanne Crumeyrolle, Mateusz Bogdan +1
To enhance the understanding of air quality within underground railway stations (URS), a methodology has been developed to establish a baseline profile of particle concentrations (…
Correlations between laboratory line lists for FeH, CrH, and NiH and M-star spectra collected with ESPaDOnS and SPIRou
P. Crozet, J. Morin, A. J. Ross +9
Molecular bands of metal oxides and hydrides dominate the optical and near-infrared spectra of M dwarfs. High-resolution spectra of these bands have immense potential for determini…
Low-temperature optical constants of amorphous silicate dust analogues
K. Demyk, V. Gromov, C. Meny +8
Cosmic dust models are key ingredients in advancing our understanding of astronomical environments as diverse as interstellar clouds in galaxies, circumstellar envelopes around evo…
Path-tracing Monte Carlo Library for 3D Radiative Transfer in Highly Resolved Cloudy Atmospheres
Najda Villefranque, Fleur Couvreux, Richard Fournier +5
Interactions between clouds and radiation are at the root of many difficulties in numerically predicting future weather and climate and in retrieving the state of the atmosphere fr…
IPRT polarized radiative transfer model intercomparison project - Three-dimensional test cases (phase B)
C. Emde, V. Barlakas, C. Cornet +6
Initially unpolarized solar radiation becomes polarized by scattering in the Earth's atmosphere. In particular molecular scattering polarizes electromagnetic radiation, but also sc…
IPRT polarized radiative transfer model intercomparison project - Phase A
C. Emde, V. Barlakas, C. Cornet +8
The polarization state of electromagnetic radiation scattered by atmospheric particles such as aerosols, cloud droplets, or ice crystals contains much more information about the op…
The O2 A-band in fluxes and polarization of starlight reflected by Earth-like exoplanets
Thomas Fauchez, Loic Rossi, Daphne M. Stam
Earth-like, potentially habitable exoplanets are prime targets in the search for extraterrestrial life. Information about their atmosphere and surface can be derived by analyzing l…
The pros and cons of the inversion method approach to derive 3D dust emission properties of the ISM: the Hi-GAL field centred on (l,b)=(30,0)
Alessio Traficante, Roberta Paladini, Mathieu Compiegne +13
Herschel FIR continuum data obtained as part of the Hi-GAL survey have been used, together with the GLIMPSE 8 m and MIPSGAL 24 m data, to attempt the first 3D-decomposition o…
A multi-wavelength investigation of RCW175: an HII region harboring spinning dust emission
C. T. Tibbs, R. Paladini, M. Compiegne +9
Using infrared, radio continuum and spectral observations, we performed a detailed investigation of the HII region RCW175. We determined that RCW175, which actually consists of two…
Swinging Atwood's Machine: Experimental and Theoretical Studies
Olivier Pujol, José-Philippe Pérez, Jean-Pierre Ramis +3
A Swinging Atwood Machine (SAM) is built and some experimental results concerning its dynamic behaviour are presented. Experiments clearly show that pulleys play a role in the moti…
Chiral Perturbation Theory
F. Cornet
An introduction to the methods and ideas of Chiral Perturbation Theory is presented in this talk. The discussion is illustrated with some phenomenological predictions that can be c…