Astrobiology86- Page

Target pixel files of TOI-3493 in TESS sectors 37 (left) and 64 (right). The electron counts are color-coded. The red-bordered pixels are used in the simple aperture photometry. TOI-3493 is

Breakdown of our best-fit model for the transit spectrum of TOI-270 d. Absorption bands of CH4, CO2 are clearly visible and one isolated absorption band of CS2 contributes at 4.6

Evolution of protein-coding gene length distributions across evolutionary time Credit ill./©: Fernando J. Ballesteros An international collaboration between four senior scientists from Mainz, Valencia, Madrid, and Zurich has published groundbreaking

Science Magazine cover — AAAS New findings from NASA’s Curiosity Mars rover could provide an answer to the mystery of what happened to the planet’s ancient atmosphere and how Mars

Spitzer Space Telescope has captured an image of an unusual comet that experiences frequent outbursts, which produce abrupt changes in brightness. Periodic comet Schwassmann-Wachmann I (P/SW-1) has a nearly circular

Calculated albedo of K2-18b for the median values of Pcloud, T, CH4, and CO2, for three different instrumental offset cases (Table 1) (Madhusudhan et al. 2023). With a perfectly reflecting

A graphical summary of our most important findings with emphasis placed on the origin, fate, and context of “missing ammonia” in the atmosphere of TOI-270 d. Numbers indicate a sequence

183 TESS systems with multiple planet candidates and/or confirmed planets (grey circles showing transiting planets), with the peak of the Dynamite v3 orbital period posterior distributions under the period ratio