TESS-Keck 勘测。XX.15 颗新的 TESS 行星和对所有巡天目标的统一 RV 分析

A. Polanski, J. Lubin, C. Beard, Joseph M. Akana Murphy, R. Rubenzahl, M. Hill, I. Crossfield, A. Chontos, P. Robertson, H. Isaacson, S. R. Kane, D. Ciardi, N. Batalha, C. Dressing, B. Fulton, Andrew W. Howard, Dan Huber, E. Petigura, L. Weiss, Isabel Angelo, A. Behmard, S. Blunt, C. Brinkman, Fei Dai, P. Dalba, T. Fetherolf, S. Giacalone, L. Hirsch, R. Holcomb, M. Kosiarek, A. Mayo, M. MacDougall, T. Močnik, D. Pidhorodetska, M. Rice, L. Rosenthal, N. Scarsdale, E. Turtelboom, Dakotah B. Tyler, Judah Van Zandt, S. Yee, D. R. Coria, Shannon D. Dulz, J. Hartman, Aaron Householder, Sarah Lange, Andrew Langford, Emma M. Louden, Jared C. Siegel, E. Gilbert, E. Gonzales, J. Schlieder, A. Boyle, J. Christiansen, Catherine A. Clark, Rachel B. Fernandes, M. Lund, A. Savel, H. Gill, C. Beichman, R. Matson, E. Matthews, E. Furlan, S. Howell, N. Scott, M. Everett, J. Livingston, I. O. Ershova, D. Cheryasov, B. Safonov, J. Lillo-Box, D. Barrado, M. Morales-Calder'on
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摘要

Transiting Exoplanet Survey Satellite(TESS)发现了数百个新世界,TESS 的候选行星数量现已超过开普勒确认的行星总数。由于巡天设计的不同,与开普勒目标相比,TESS继续提供更适合后续跟踪研究的行星,包括通过径向速度(RV)观测进行质量测量。在这项工作中,我们介绍了TESS-Keck巡天(TKS)质量目录:对所有TKS RV巡天数据的统一分析,得出了126颗行星和候选信号的质量约束。其中包括 58 项精确度达到 ≥5σ 的质量测量。通过重要的质量测量(15)或统计验证(17),我们确认或验证了来自TESS任务的32颗新行星,而且我们在整个样本中没有发现可能的假阳性证据。这项工作同时也是对所有以前未公布的TKS巡天数据的一次数据发布,其中包括我们三年巡天过程中的9204次RV测量和相关活动指标。我们借此机会评估了巡天的性能,发现我们实现了许多目标,包括测量了38颗小行星(<4 R ⊕)的质量,几乎达到了TESS任务的基础科学要求。此外,我们还评估了作为巡天支持的自动行星探测器的性能,并观测到由于其更均匀的相位覆盖而对系统参数产生的有意义的约束。最后,我们将测得的质量与常用的质量-半径关系所预测的质量进行了比较,并调查了系统偏差的证据。
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The TESS-Keck Survey. XX. 15 New TESS Planets and a Uniform RV Analysis of All Survey Targets
The Transiting Exoplanet Survey Satellite (TESS) has discovered hundreds of new worlds, with TESS planet candidates now outnumbering the total number of confirmed planets from Kepler. Owing to differences in survey design, TESS continues to provide planets that are better suited for subsequent follow-up studies, including mass measurement through radial velocity (RV) observations, compared to Kepler targets. In this work, we present the TESS-Keck Survey’s (TKS) Mass Catalog: a uniform analysis of all TKS RV survey data that has resulted in mass constraints for 126 planets and candidate signals. This includes 58 mass measurements that have reached ≥5σ precision. We confirm or validate 32 new planets from the TESS mission either by significant mass measurement (15) or statistical validation (17), and we find no evidence of likely false positives among our entire sample. This work also serves as a data release for all previously unpublished TKS survey data, including 9,204 RV measurements and associated activity indicators over our three-year survey. We took the opportunity to assess the performance of our survey and found that we achieved many of our goals, including measuring the mass of 38 small (<4 R ⊕) planets, nearly achieving the TESS mission’s basic science requirement. In addition, we evaluated the performance of the Automated Planet Finder as survey support and observed meaningful constraints on system parameters, due to its more uniform phase coverage. Finally, we compared our measured masses to those predicted by commonly used mass–radius relations and investigated evidence of systematic bias.
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