output
20022024
most citedThe Gaia mission

7.1k citations

Showing 2020Show all

32 papers · 1 filter

astro-ph.GA20202 cited

Dust evolution: going beyond the empirical

Nathalie Ysard

A key element when modeling dust in any astrophysical environment is a self-consistent treatment of the evolution of the dust material properties (size distribution, chemical compo…

astro-ph.IM202049 cited

The quantum efficiency and diffractive image artifacts of Si:As IBC mid-IR detector arrays at 5 10 m: Implications for the JWST/MIRI detectors

Andras Gaspar, George H. Rieke, Pierre Guillard +6

Arsenic doped back illuminated blocked impurity band (BIBIB) silicon detectors have advanced near and mid-IR astronomy for over thirty years; they have high quantum efficiency (QE)…

astro-ph.EP202024 cited

Irradiation dose affects the composition of organic refractory materials in space: Results from laboratory analogues

R. G. Urso, V. Vuitton, G. Danger +9

Context. Near- and mid-infrared observations have revealed the presence of organic refractory materials in the solar system, in cometary nuclei and on the surface of centaurs, Kuip…

astro-ph.SR20204 cited

Differential Emission Measure Evolution as a Precursor of Solar Flares

C. Gontikakis, I. Kontogiannis, M. K. Georgoulis +4

We analyse the temporal evolution of the Differential Emission Measure (DEM) of solar active regions and explore its usage in solar flare prediction. The DEM maps are provided by t…

astro-ph.CO202077 cited

First detection of stacked X-ray emission from cosmic web filaments

H. Tanimura, N. Aghanim, A. Kolodzig +2

We report the first statistical detection of X-ray emission from cosmic web filaments in ROSAT data. We selected 15,165 filaments at 0.2<z<0.6 ranging from 30 Mpc to 100 Mpc in len…

astro-ph.SR202038 cited

20 Years of ACE Data: How Superposed Epoch Analyses Reveal Generic Features in Interplanetary CME Profiles

F. Regnault, M. Janvier, P. Démoulin +4

Interplanetary coronal mass ejections (ICMEs) are magnetic structures propagating from the Sun's corona to the interplanetary medium. With over 20 years of observations at the L1 l…