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Left part: a schematic view of the ISEAge UHV setup. The IR beam path is shown with red. The T-shaped optical holder with the Ge window is shown with green. The direction of molecular species injection is shown with arrow. Cad models are taken from Kurt J. Lesker cataloguea . The radiation shield is omitted for clarity. Right part: a typical image of Ge window surface obtained with the scanning-probe microscope for the 10x10 µm area. The colour scheme indicates the registered peak to valley height from the lowest point (dark brown) to the highest point (light yellow) in nm. --- astro-ph.GA

Astrochemistry, Astronomy & Telescopes, Biochemistry & Organic Chemistry, Imaging & Spectroscopy, Interstellar, Status Report

Infrared Spectra of Solid HCN Embedded in Various Molecular Environments for Comparison with the Data Obtained with JWST

by Keith CowingAugust 18, 2024August 17, 2024

HCN molecules serve as an important tracer for chemical evolution of elemental nitrogen in the regions of star and planet formation. This is largely explained by the fact that N […]

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Infrared Spectra of Solid HCN Embedded in Various Molecular Environments for Comparison with the Data Obtained with JWST

A Martian Horizon Last Monday Afternoon

Habitable-zone Earths At The Detection Frontier: Measured Completeness And False-alarm Rate Of A Transit Pipeline For The PLATO M-dwarf Sample

A Homogeneous Survey Of JWST MIRI Transmission Spectra Of 10 Exoplanets

Retrieving Ocean Glint Reflectance Signatures From Directly Imaged Earth-like Exoplanets

Analytical Platform (Microsampling, Catapulting, Trapping, and LIBS) for the Characterization of Discrete Domains in Samples of Astrochemical Interest