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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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Bibliographic Details
Published in:	The Astronomical journal 2020-12, Vol.161 (1)
Main Authors:	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:	Article
Language:	English
Subjects:	Exoplanets Gaussian Processes regression Mini Neptunes Radial velocity Super Earths Transit photometry
Online Access:	Get full text
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