Ultra-low noise mid-infrared detector — AIP The mid-infrared (MIR) wavelength range, from 5 to 25 micrometers, is an important regime for astrophysics as it can be used to detect the
Ultra-low noise mid-infrared detector — AIP The mid-infrared (MIR) wavelength range, from 5 to 25 micrometers, is an important regime for astrophysics as it can be used to detect the
(A) Pre and post irradiation spectra of the fiducial 10 K 2:1 benzene:ozone experiment. (B) Spectra of pure phenol ice at 10 K, (C) Spectra of a ∼ 30:1 benzene:phenol
The PLL analysis of the fifth detected transit of TOI-5388 b at 1881.03 TBJD. Each square represents the flux of a pixel, with respect to time, and the color scale
Imagine standing on the precipice of time, gazing into the vast expanse of the cosmos, where every twinkle of a star tells a story of creation, evolution, and the inexorable
SPHEREx measures the abundances and properties of ice species by taking absorption spectra toward background stars and protostars. This comprehensive survey toward ∼10 million targets spans the evolutionary stages of
Diagram of the SPHEREx observatory, showing (from top to bottom) the three conical photon shields with a cutaway view, the telescope, radiator panel for the mid-wave infrared (MWIR) detectors, the
The US’s federally funded space program has been struggling of late. With the recent cancellation of the Mars Sample Return mission, and mass layoffs / resignations taking place at NASA,
January 20, 2026 – Washington, D.C.—The Commercial Space Federation (CSF) is pleased to welcome Max Space, Slingshot Aerospace, and Muon Space. Together, these companies strengthen CSF’s advocacy efforts across space
One of the closest planetary nebulas to Earth, the Helix Nebula has become a favorite among astronomers using ground- and space-based telescopes to study the final moments of a dying
Investigative filmmaker James Fox is hosting a press conference with new testimony and evidence regarding UAP allegations.






