activity
20052024
most citedThe 10 micron amorphous silicate feature of fractal aggregates and compact particles with complex shapes

54 citations · 188 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2024★ 26 cited

Water depletion and 15NH3 in the atmosphere of the coldest brown dwarf observed with JWST/MIRI

H. Kühnle, P. Patapis, P. Mollière +21

With a temperature of K WISE0855 is the coldest brown dwarf observed so far. Using the James Webb Space Telescope (JWST) we obtained observations that allow us to charac…

astro-ph.EP2024★ 11 cited

Constraining the formation of WASP-39b using JWST transit spectroscopy

N. Khorshid, M. Min, J. Polman +1

Understanding the formation history of planets is one of the goals of studying exoplanet atmospheres. The atmospheric composition of planets can provide insights into the formation…

astro-ph.EP2020★ 42 cited

Mineral cloud and hydrocarbon haze particles in the atmosphere of the hot Jupiter JWST target WASP-43b

Ch. Helling, Y. Kawashima, V. Graham +5

Having a short orbital period and being tidally locked makes WASP-43b an ideal candidate for JWST observations. Phase curve observations of an entire orbit will enable the mapping…

astro-ph.EP2017★ 4 cited

Laboratory mid-IR spectra of equilibrated and igneous meteorites. Searching for observables of planetesimal debris

B. L. de Vries, H. Skogby, L. B. F. M. Waters +1

Meteorites contain minerals from Solar System asteroids with different properties (like size, presence of water, core formation). We provide new mid-IR transmission spectra of powd…

astro-ph.SR2014★ 21 cited

Location and sizes of forsterite grains in protoplanetary disks: interpretation from the Herschel DIGIT programme

K. M. Maaskant, B. L. de Vries, M. Min +4

The spectra of protoplanetary disks contain mid- and far- infrared emission features produced by forsterite dust grains. The spectral features contain information about the forster…

astro-ph.SR2014★ 30 cited

Herschel/PACS observations of the 69 band of crystalline olivine around evolved stars

J. A. D. L. Blommaert, B. L. de Vries, L. B. F. M. Waters +15

We present 48 Herschel/PACS spectra of evolved stars in the wavelength range of 67-72 m. This wavelength range covers the 69 m band of crystalline olivine ($\text{Mg}_{2-2x}\…