A low upper-mass limit for the central black hole in the late-type galaxy NGC 4414
A low upper-mass limit for the central black hole in the late-type galaxy NGC 4414
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DOI：
10.1051/0004-6361/201629480
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发表时间：
2016-10
影响因子：
6.5
通讯作者：
S. Thater;D. Krajnovi'c;M. Bourne;M. Cappellari;T. Zeeuw;E. Emsellem;J. Magorrian;R. McDermid;M. Sarzi;G. Ven
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作者：
S. Thater;D. Krajnovi'c;M. Bourne;M. Cappellari;T. Zeeuw;E. Emsellem;J. Magorrian;R. McDermid;M. Sarzi;G. Ven
作者感谢Tony Wong提供的NGC 4414的CO数据和Remco货车den Bosch对NGC 4414的MGE模型进行的富有成效的讨论。M.C.感谢皇家学会大学研究奖学金的支持。根据由大学天文学研究协会运营的双子座天文台获得的观测结果，在GN-2007 A-Q-45方案下，根据与代表双子座伙伴关系的国家科学基金会达成的合作协议：国家科学基金会（美国）、国家研究理事会（加拿大）、CONICYT（智利）、澳大利亚研究理事会（澳大利亚）、Ministerio da Ciudad、Tecnologia e Inovacao（巴西）和Ministerio de Ciudad、Tecnologia e Innovacion Productiva（阿根廷）。根据美国航天局/欧空局哈勃空间望远镜的观测结果，从空间望远镜科学研究所的欧空局哈勃科学档案馆获得，该档案馆由大学天文学研究协会经营，根据NASA合同NAS 5-26555。SDSS-III的资金由阿尔弗雷德·斯隆基金会、参与机构、国家科学基金会和美国能源部科学办公室提供。SDSS-III的网址是http://www.sdss3.org/。SDSS-III由SDSS-III合作参与机构的天体物理研究联合会管理，包括亚利桑那大学、巴西参与小组、布鲁克海文国家实验室、卡内基梅隆大学、佛罗里达大学、法国参与小组、德国参与小组、哈佛大学、加那利群岛天体物理研究所、密歇根州立大学/圣母院/JINA参与小组、约翰霍普金斯大学、劳伦斯伯克利国家实验室、马克斯普朗克天体物理研究所、马克斯普朗克地外物理研究所、新墨西哥州州立大学、纽约大学、俄亥俄州州立大学、宾夕法尼亚州立大学、朴茨茅斯大学、普林斯顿大学、西班牙参与小组、东京大学、犹他州大学、范德比尔特大学、弗吉尼亚大学、华盛顿大学、和耶鲁大学。本研究使用了蒙太奇。它由美国国家科学基金会资助，资助号为ACI-1440620，之前由美国国家航空航天局地球科学技术办公室计算技术项目资助，合作协议号为NCC 5 -626，NASA和加州理工学院。这项研究利用了由加州理工学院喷气推进实验室根据与美国国家航空航天局的合同运作的美国航天局/国际公共事务委员会河外数据库。我们承认使用HyperLeda数据库（http：leda.univ-lyon1.fr）
The authors want to thank Tony Wong for providing the CO data of NGC 4414 and Remco Van den Bosch for fruitful discussions regarding the MGE model of NGC 4414. M.C. acknowledges support from a Royal Society University Research Fellowship. Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministerio da Ciencia, Tecnologia e Inovacao (Brazil) and Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina), under program GN-2007A-Q-45. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the ESA Hubble Science Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. This research made use of Montage. It is funded by the National Science Foundation under Grant Number ACI-1440620, and was previously funded by the National Aeronautics and Space Administration’s Earth Science Technology Office, Computation Technologies Project, under Cooperative Agreement Number NCC5-626 between NASA and the California Institute of Technology. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. We acknowledge the usage of the HyperLeda database (http://leda.univ-lyon1.fr)