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Robust diffraction-limited near-infrared-to-near-ultraviolet wide-field imaging from stratospheric balloon-borne platforms—Super-pressure Balloon-borne Imaging Telescope performance
DOI: 10.1063/1.5139711 Bibcode: 2020RScI...91c4501R

Jauzac, Mathilde; Tam, Sut-Ieng; Benton, Steven J. +26 more

At a fraction of the total cost of an equivalent orbital mission, scientific balloon-borne platforms, operating above 99.7% of the Earth's atmosphere, offer attractive, competitive, and effective observational capabilities—namely, space-like seeing, transmission, and backgrounds—which are well suited for modern astronomy and cosmology. The Super-p…

2020 Review of Scientific Instruments
Gaia 12
Simple, compact, high-resolution monochromatic x-ray source for characterization of x-ray calorimeter arrays
DOI: 10.1063/5.0005206 Bibcode: 2020RScI...91h3110L

Eckart, M. E.; Kilbourne, C. A.; Leutenegger, M. A. +6 more

X-ray calorimeters routinely achieve very high spectral resolution, typically a few eV full width at half maximum (FWHM). Measurements of calorimeter line shapes are usually dominated by the natural linewidth of most laboratory calibration sources. This compounds the data acquisition time necessary to statistically sample the instrumental line bro…

2020 Review of Scientific Instruments
Hitomi 5
INFRA-ICE: An ultra-high vacuum experimental station for laboratory astrochemistry
DOI: 10.1063/5.0027920 Bibcode: 2020RScI...91l4101S

Santoro, Gonzalo; Sobrado, Jesús. M.; Tajuelo-Castilla, Guillermo +7 more

Laboratory astrochemistry aims at simulating, in the laboratory, some of the chemical and physical processes that operate in different regions of the universe. Amongst the diverse astrochemical problems that can be addressed in the laboratory, the evolution of cosmic dust grains in different regions of the interstellar medium (ISM) and its role in…

2020 Review of Scientific Instruments
Rosetta 4