Early Results from the HUMDRUM Survey: A Small, Earth-mass Planet Orbits TOI-1450A
M. Brady, J. Bean, A. Seifahrt, D. Kasper, R. Luque, G. Stef’ansson, J. St"urmer, D. Charbonneau, K. Collins, J. Doty, Z. Essack, A. Fukui, F. Grau Horta, C. Hedges, C. Hellier, J. Jenkins, N. Narita, S. Quinn, A. Shporer, R. Schwarz, S. Seager, K. Stassun, S. Striegel, C. Watkins, J. Winn, R. Zambelli
arXiv:2405.10400v1 Announce Type: new
Abstract: M dwarf stars provide us with an ideal opportunity to study nearby small planets. The HUMDRUM (HUnting for M Dwarf Rocky planets Using MAROON-X) survey uses the MAROON-X spectrograph, which is ideally suited to studying these stars, to measure precise masses of a volume-limited ($arXiv:2405.10400v1 Announce Type: new
Abstract: M dwarf stars provide us with an ideal opportunity to study nearby small planets. The HUMDRUM (HUnting for M Dwarf Rocky planets Using MAROON-X) survey uses the MAROON-X spectrograph, which is ideally suited to studying these stars, to measure precise masses of a volume-limited ($