201 citations · 685 across the 9 of their papers we have counts for
9 papers
Inferring the dust emission at submillimeter and millimeter wavelengths using neural networks
D. Paradis, C. Mény, A. Noriega-Crespo +3
The Planck mission provided all-sky dust emission maps in the submm to mm range at an angular resolution of 5'. In addition, some specific sources can be observed at long wavelengt…
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…
Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues II: Mg and Fe-rich amorphous silicates
K. Demyk, C. Meny, H. Leroux +5
To model the cold dust emission observed in the diffuse interstellar medium, in dense molecular clouds or in cold clumps that could eventually form new stars, it is mandatory to kn…
Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues I: Mg-rich glassy silicates
K. Demyk, C. Meny, X. -H. Lu +11
A wealth of data from the Herschel and Planck satellites and now from ALMA, revealing cold dust thermal emission, is available for astronomical environments ranging from interstell…
Low temperature FIR and submm mass absorption coefficient of interstellar silicate dust analogues
A. Coupeaud, K. Demyk, C. Meny +7
Cold dust grains emission in the FIR/submm is usually expressed as a modified black body law in which the dust mass absorption coefficient (MAC), is described with a temperature- a…
Far-infrared to millimeter astrophysical dust emission I: A model based on physical properties of amorphous solids
C. Meny, V. Gromov, N. Boudet +3
We propose a new description of astronomical dust emission in the spectral region from the Far-Infrared to millimeter wavelengths. Unlike previous classical models, this descriptio…