output
20022024
most citedThe Gaia mission

7.1k citations

Showing 2017Show all

34 papers · 1 filter

astro-ph.EP201742 cited

Dependence of the Martian radiation environment on atmospheric depth: Modeling and measurement

Jingnan Guo, Tony C. Slaba, Cary Zeitlin +9

The energetic particle environment on the Martian surface is influenced by solar and heliospheric modulation and changes in the local atmospheric pressure (or column depth). The Ra…

astro-ph.GA201715 cited

Probing the baryon cycle of galaxies with SPICA mid- and far-infrared observations

F. F. S. van der Tak, S. C. Madden, P. Roelfsema +29

The SPICA mid and far-infrared telescope will address fundamental issues in our understanding of star formation and ISM physics in galaxies. A particular hallmark of SPICA is the o…

astro-ph.CO201715 cited

Mean Energy Density of Photogenerated Magnetic Fields Throughout the Epoch of Reionization

Jean-Baptiste Durrive, Hiroyuki Tashiro, Mathieu Langer +1

Magnetic fields are ubiquitous in the Universe. They seem to be present at virtually all scales and all epochs. Yet, whether the fields on cosmological scales are of astrophysical…

astro-ph.IM201725 cited

Polyaromatic disordered carbon grains as carriers of the UV bump: FUV to mid-infrared spectroscopy of laboratory analogs

Lisseth Gavilan, Kim Cuong Le, Thomas Pino +3

A multiwavelength study of laboratory carbons with varying degrees of hydrogenation and sp hybridization is required to characterize the structure of the carbonaceous carriers…

astro-ph.EP201754 cited

Dome C UltraCarbonaceous Antarctic MicroMeteorites Infrared and Raman fingerprints

E. Dartois, C. Engrand, J. Duprat +5

UltraCarbonaceous Antarctic MicroMeteorites (UCAMMs) represent a small fraction of interplanetary dust particles reaching the Earth's surface and contain large amounts of an organi…

astro-ph.SR2017125 cited

ALMA discovery of a rotating SO/SO flow in HH212. A possible MHD disk wind?

B. Tabone, S. Cabrit, E. Bianchi +7

We wish to constrain the possible contribution of a magnetohydrodynamic disk wind (DW) to the HH212 molecular jet. We mapped the flow base with ALMA Cycle 4 at 0.13" 60 au re…