Archive for June, 2025110- Page

Planning diagram showing variation in latitude range (between heavy black lines) vs. season (solar longitude, LS) for SHARAD standard VLR observations wherein all associated spacecraft maneuvers occur when the MRO

Distribution of simulated EEC yield (solid contours) and underlying planet population (dotted contours) around FGK-type stars within 20 pc. We show the planetary radius over incident flux distribution, where the

χ2 maps for the CS RT models. The free parameters f0 and Re are on the x− and y−axes, respectively. The red + sign denotes the best-fit model, and the

MUSE and NIRCam images of d203-504 environment. Left: MUSE NFM composite image of both d203-506 (bottom left) and d203-504 (top). Red: the (λ8727˚A) map showing disk contributions from both