22:06 <raptop> o_O https://arxiv.org/abs/2307.10931

22:06 <galois> [arXiv] “Haze optical depth in exoplanet atmospheres varies with rotation rate: Implications for observations” Maureen Cohen, Paul I. Palmer, Adiv Paradise et al. — «Transmission spectroscopy supports the presence of uncharacterised, light-scattering and -absorbing aerosols in the atmospheres of many exoplanets. The complexity of factors influencing the formation, 3-D transport, radiative impact, and removal of aerosols makes…»

22:08 <raptop> Tau-Ceti is located pole-on https://arxiv.org/abs/2307.10394

22:08 <galois> [arXiv] “Refining the Stellar Parameters of $τ$ Ceti: a Pole-on Solar Analog” Maria Korolik, Rachael M. Roettenbacher, Debra A. Fischer et al. — «To accurately characterize the planets a star may be hosting, stellar parameters must first be well-determined. $\tau$ Ceti is a nearby solar analog and often a target for exoplanet searches. Uncertainties in the observed rotational velocities have made constraining $\tau$ Ceti's…»

22:08 <raptop> ...the what telescope? https://arxiv.org/abs/2307.10468

22:08 <galois> [arXiv] “The Greenland Telescope: Construction, Commissioning, and Operations in Pituffik” Ming-Tang Chen, Keiichi Asada, Satoki Matsushita et al. — «In 2018, the Greenland Telescope (GLT) started scientific observation in Greenland. Since then, we have completed several significant improvements and added new capabilities to the telescope system. This paper presents a full review of the GLT system, a summary of our observation…»