Corner plot from the Full (left) and Upper Limits (right) Runs with associated CCF maps for TOI-1807 b. The blue contours represent the 1-, 2-, and 3-σ confidence intervals. Left:
Corner plot from the Full (left) and Upper Limits (right) Runs with associated CCF maps for TOI-1807 b. The blue contours represent the 1-, 2-, and 3-σ confidence intervals. Left:
– vs. for n-capture elements in the SMC. Abundance patterns are shown for Eu (leftmost panel), Zr (second leftmost) and Ba (second rightmost) and La (rightmost). Solid
A few highlights from the first recognition of Archaea to the cultivation of the first Asgard representatives and their cellular structures are shown. Symbols indicate the respective methods used. —
a, We levitate a 500-μm silica sphere in an acoustic trap above a silica target plate. b, Charge is measured by applying a frequency-swept electric field, E(t), and extracting the
The new MultiQ-IT prototype can cool, trap, filter, and redirect over a billion ionssimultaneously, dramatically improving dynamic range and signal-to-noise. Credit Lori Chertoff/The Rockefeller University Editor’s note: with recent speculation
Eimission spectra of 3I/ATLAS taken with BFOSC and YFOSC. For clarity, the full spectral range is divided into three panels with different vertical offsets to emphasize specific features. The left
With the Munsell Soil Colour Chart the cores are described visually in colour and structure as acurately as possible. Photo: Diekamp@ECORD_IODP3_NSF Credit Diekamp@ECORD_IODP3_NSF The goal of this expedition went far
Collisions between leftover planetesimals drives the redistribution of mass between bodies of different sizes, generating a so-called collisional size-frequency distribution (SFD) dominated, in number, by the smallest bodies. The Earth
Lunar Exploration Analysis Group (LEAG) The Lunar Exploration Analysis Group (LEAG) and Extraterrestrial Materials Analysis Group (ExMAG), were requested and empowered by NASA’s Science Mission Directorate (SMD) and Planetary Science
Credit: NASA/JPL-Caltech/KSC The National Academies’ Committee on Planetary Protection is hosting a virtual meeting that will inform NASA’s efforts to develop a prioritized list of factors that contribute to the






