@article{2026A&A...707A.320P,
 adsnote = {Provided by the SAO/NASA Astrophysics Data System},
 adsurl = {https://ui.adsabs.harvard.edu/abs/2026A&A...707A.320P},
 archiveprefix = {arXiv},
 author = {Ponti, G. and Yeung, M.~C.~H. and Stel, G. and Locatelli, N. and Zheng, X. and Stelzer, B. and Merloni, A. and Caramazza, M. and Magaudda, E. and Sasaki, M. and Dennerl, K. and Reiprich, T.~H. and Schwope, A. and Becker, W. and Freyberg, M.},
 doi = {10.1051/0004-6361/202556925},
 eid = {A320},
 eprint = {2602.03941},
 journal = {åp},
 keywords = {stars: coronae, Galaxy: general, Galaxy: halo, X-rays: diffuse background, X-rays: general, X-rays: stars, Astrophysics of Galaxies, High Energy Astrophysical Phenomena, Solar and Stellar Astrophysics},
 month = {March},
 pages = {A320},
 primaryclass = {astro-ph.GA},
 title = {Low-mass stars dominate the hot (0.7 keV) Galactic X-ray emission},
 volume = {707},
 year = {2026}
}