Physical Parameters of the Multiplanet Systems HD 106315 and GJ 9827 Based on observations obtained at the W. M. Keck Observatory, which is operated jointly by the University of California and the California Institute of Technology. † †This paper includes data gathered with the 6.5 meter Magellan Telescopes located at Las Campanas Observatory, Chile

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Veröffentlicht in:	The Astronomical journal 2020-12, Vol.161 (1)
Hauptverfasser:	Kosiarek, Molly R., Berardo, David A., Crossfield, Ian J. M., Laguna, Cesar, Piaulet, Caroline, Akana Murphy, Joseph M., Howell, Steve B., Henry, Gregory W., Isaacson, Howard, Fulton, Benjamin, Weiss, Lauren M., Petigura, Erik A., Behmard, Aida, Hirsch, Lea A., Teske, Johanna, Burt, Jennifer A., Mills, Sean M., Chontos, Ashley, Močnik, Teo, Howard, Andrew W., Werner, Michael, Livingston, John H., Krick, Jessica, Beichman, Charles, Gorjian, Varoujan, Kreidberg, Laura, Morley, Caroline, Christiansen, Jessie L., Morales, Farisa Y., Scott, Nicholas J., Crane, Jeffrey D., Wang, Sharon Xuesong, Shectman, Stephen A., Rosenthal, Lee J., Grunblatt, Samuel K., Rubenzahl, Ryan A., Dalba, Paul A., Giacalone, Steven, Villanueva, Chiara Dane, Liu, Qingtian, Dai, Fei, Hill, Michelle L., Rice, Malena, Kane, Stephen R., Mayo, Andrew W.
Format:	Artikel
Sprache:	eng
Schlagworte:	Exoplanets Gaussian Processes regression Mini Neptunes Radial velocity Super Earths Transit photometry
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