Astrobiology73- Page

Left: Eccentricity posterior generated by fitting the first nine chronological transits of TOI 555.01. Right: Eccentricity posterior generated by fitting the first nine chronological long-cadence transits of KOI 247.01. —

GMM fits to the unbinned radius data, along with corresponding histograms, are presented for the entire low-mass star sample and for M, K, and G stellar types. The Super-Earth and

ℓ1 periodogram for the stars HD 10700 (left), HD 102365 (centre), and HD 304636 (right). The ten strongest peaks periods are identified in the image; the associated FAP is listed

RAIR spectra (top) and difference spectra (bottom) for irradiation of the (a) CO:PHP mixed ice and (b) CO/PHP layered ice, focusing on the region around the CO stretching mode. The

The average total power of individual airport radar systems, averaged over one-hour intervals as seen from Barnard’s Star. — Royal Astronomical Society Radar systems used by civilian airports and military

Detection of HD 135344 Ab with VLT/SPHERE. — astro-ph.EP HD 135344 AB is a young visual binary system that is best known for the protoplanetary disk around the secondary star.

Graphical Abstract — Istanbul Technical University Dr. Seda Işık, who completed her doctorate at Istanbul Technical University (ITU) Eurasia Institute of Earth Sciences in the Earth System Science Program, achieved