Vanderspek, Roland; Huang, Chelsea X.; Vanderburg, Andrew; Ricker, George R.; Latham, David W.; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; Burt, Jennifer; Dittmann, Jason; Newton, Elisabeth; Quinn, Samuel N.; Shporer, Avi; Charbonneau, David; Irwin, Jonathan; Ment, Kristo; Winters, Jennifer G.; Collins, Karen A.; Evans, Phil; Gan, Tianjun; Hart, Rhodes; Jensen, Eric L. N.; Kielkopf, John; Mao, Shude; Waalkes, William; Bouchy, François; Marmier, Maxime; Nielsen, Louise D.; Ottoni, Gaël; Pepe, Francesco; Ségransan, Damien; Udry, Stéphane; Henry, Todd; Paredes, Leonardo A.; James, Hodari-Sadiki; Hinojosa, Rodrigo H.; Silverstein, Michele L.; Palle, Enric; Berta-Thompson, Zachory; Crossfield, Ian; Davies, Misty D.; Dragomir, Diana; Fausnaugh, Michael; Glidden, Ana; Pepper, Joshua; Morgan, Edward H.; Rose, Mark; Twicken, Joseph D.; Villaseñor, Jesus Noel S.; Yu, Liang; Bakos, Gaspar; Bean, Jacob; Buchhave, Lars A.; Christensen-Dalsgaard, Jørgen; Christiansen, Jessie L.; Ciardi, David R.; Clampin, Mark; De Lee, Nathan; Deming, Drake; Doty, John; Jernigan, J. Garrett; Kaltenegger, Lisa; Lissauer, Jack J.; McCullough, P. R.; Narita, Norio; Paegert, Martin; Pal, Andras; Rinehart, Stephen; Sasselov, Dimitar; Sato, Bun'ei; Sozzetti, Alessandro; Stassun, Keivan G.; Torres, Guillermo
(2019)
Data from the newly commissioned Transiting Exoplanet Survey Satellite has revealed a "hot Earth" around LHS 3844, an M dwarf located 15 pc away. The planet has a radius of 1.303+/- 0.022 R <SUB>?</SUB> and orbits the star ...