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1. Satellites of infinite rank in the smooth concordance group

   https://doi.org/10.1007/s00222-020-01026-w  

   Hedden, Matthew; Pinzón-Caicedo, Juanita (July 2021, Inventiones mathematicae)

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2. Gas and Star Formation in Satellites of Milky Way Analogs

   https://doi.org/10.3847/1538-4357/ad3076  

   Jones, Michael G.; Sand, David J.; Karunakaran, Ananthan; Spekkens, Kristine; Oman, Kyle A.; Bennet, Paul; Besla, Gurtina; Crnojević, Denija; Cuillandre, Jean-Charles; Fielder, Catherine E.; et al (April 2024, The Astrophysical Journal)

   Abstract We have imaged the entirety of eight (plus one partial) Milky Way (MW)–like satellite systems, a total of 42 (45) satellites, from the Satellites Around Galactic Analogs II catalog in both Hαand Hiwith the Canada–France–Hawaii Telescope and the Jansky Very Large Array. In these eight systems we have identified four cases where a satellite appears to be currently undergoing ram pressure stripping (RPS) as its Higas collides with the circumgalactic medium (CGM) of its host. We also see a clear suppression of gas fraction (M_HI/M_*) with decreasing (projected) satellite–host separation—to our knowledge, the first time this has been observed in a sample of MW-like systems. Comparisons to the Auriga, A Project Of Simulating The Local Environment, and TNG50 cosmological zoom-in simulations show consistent global behavior, but they systematically underpredict gas fractions across all satellites by roughly 0.5 dex. Using a simplistic RPS model, we estimate the average peak CGM density that satellites in these systems have encountered to be $\log {\rho }_{\mathrm{cgm}}/\mathrm{g}{\mathrm{cm}}^{-3}\approx -27.3$. Furthermore, we see tentative evidence that these satellites are following a specific star formation rate to gas fraction relation that is distinct from field galaxies. Finally, we detect one new gas-rich satellite in the UGC 903 system with an optical size and surface brightness meeting the standard criteria to be considered an ultra-diffuse galaxy. 

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3. Is 9D localization possible with unsynchronized LEO Satellites?

   https://doi.org/10.1109/MILCOM61039.2024.10773638  

   Emenonye, Don-Roberts; Dhillon, Harpreet S; Buehrer, R Michael (October 2024, IEEE MILCOM)
4. Satellites reveal Earth's seasonally shifting dust emission sources

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   Chappell, Adrian; Webb, Nicholas P.; Hennen, Mark; Schepanski, Kerstin; Ciais, Philippe; Balkanski, Yves; Zender, Charles S.; Tegen, Ina; Zeng, Zhenzhong; Tong, Daniel; et al (April 2023, Science of The Total Environment)
5. Detailed Abundances in the Ultra-faint Magellanic Satellites Carina II and III

   https://doi.org/10.3847/1538-4357/ab6213  

   Ji, A. P.; Li, T. S.; Simon, J. D.; Marshall, J.; Vivas, A. K.; Pace, A. B.; Bechtol, K.; Drlica-Wagner, A.; Koposov, S. E.; Hansen, T. T.; et al (January 2020, The Astrophysical Journal)