Nano-DSF glass capillaries filled with different brines. Crystallisation processes can be observed at the extremities of the capillaries. The red arrow indicates extensive crystallisation at the extremity of the capillaries
Nano-DSF glass capillaries filled with different brines. Crystallisation processes can be observed at the extremities of the capillaries. The red arrow indicates extensive crystallisation at the extremity of the capillaries
Continuum-subtracted spectra of comet 3I obtained on August 28 and September 3+4. Three narrow FeI lines are detected on August 28 in this spectral range, FeI λ3719.93Å being the brightest
Orbital characterization of TOI-402 B around A using multiple datasets. (a): astrometric orbits of TOI-402 B around A. The blue filled circles are observed relative astrometry used in our analysis.
Application domain for mass measurements via small JWST atmospheric exploration programs. Size of known exoplanets with mass measurements (relative mass uncertainty, RMU, as color) versus their estimated TSM—data from Ref.37.
Examples of the template extraction from the atmospheric models at JWST’s spectral resolution (top panels) for three molecules, H2O (left column panels), CH4 (middle column panels) and CO (right column
Results of the forward modeling of β Pic b using the most recent spectro/photometric observations of the planet (including CRIRES+) using BT-Settl. Top panel: spectra (points) and photometry (squares) of
Climate simulations of Venus’s atmosphere. (a) A climate model that uses the H2SO4 clouds and gas concentrations predicted by the nominal photochemical simulation in Figure 2. (b) The same as
Parameter space showing the effect of GR on eccentricity oscillations due to an exterior planetary companion for a variety of combinations of the mass ratio m2/m1 and semi-major axis ratio
Kultur von Hypomyces completus Public Domain, Quelle: US Department of Agriculture, Agricultural Research Service, Systematic Botany and Mycology Laboratory, Larger image New research published in Nature Ecology & Evolution
JWST MIRI MRS spectra of DQ Tau. Various colors mark the different observing epochs, whose dates and the corresponding orbital phases are indicated in the upper left corner. The bottom






