Detection of a giant flare displaying quasi-periodic pulsations from a pre-main-sequence M star by the Next Generation Transit Survey
Detection of a giant flare displaying quasi-periodic pulsations from a pre-main-sequence M star by the Next Generation Transit Survey
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DOI：
10.1093/mnras/sty3036
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发表时间：
2018-11
影响因子：
4.8
通讯作者：
J. Jackman;P. Wheatley;C. Pugh;D. Kolotkov;A. Broomhall;G. Kennedy;S. Murphy;R. Raddi;M. Burleigh-M
中科院分区：
文献类型：
--
作者：
J. Jackman;P. Wheatley;C. Pugh;D. Kolotkov;A. Broomhall;G. Kennedy;S. Murphy;R. Raddi;M. Burleigh-M
这项研究是基于在ESO La Silla Paranal天文台的NGTS项目下收集的数据。NGTS设施由一个研究所联盟资助，该研究所联盟由沃里克大学、莱斯特大学、贝尔法斯特女王大学、日内瓦大学、Deutsches Zentrum fur Luft- und Raumfahrt e. V.（DLR;根据'Grosinvestion GI-NGTS'）、剑桥大学以及英国科学技术设施理事会（STFC;项目参考ST/M001962/1）组成。JAGJ由STFC博士生资助1763096。PJW和RGW得到STFC合并赠款ST/P000495/1的支持。AMB感谢沃里克大学高级研究所的支持，并得到STFC综合赠款ST/P000320/1的支持。MNG由STFC奖参考1490409以及艾萨克·牛顿助学金支持。CEP感谢欧洲研究理事会在SeismoSun研究项目第321141号下提供的支持。JSJ感谢Fondecyt赠款1161218的支持和CATA-Basal（PB 06，CONICYT）的部分支持。DYK感谢STFC综合赠款ST/P000320/1的支持。GMK是由皇家社会作为皇家社会大学研究员的支持。我们也感谢AMB领导的ISSI团队进行了有益的讨论。本出版物使用了2 MASS的数据产品，该数据产品是马萨诸塞州大学和红外处理和分析中心/加州理工学院的联合项目，由美国国家航空航天局和国家科学基金会资助。本出版物使用了WISE的数据产品，WISE是加州大学洛杉矶分校和喷气推进实验室/加州理工学院的联合项目，由美国国家航空航天局资助。SkyMapper的国家设施能力是通过澳大利亚研究理事会的ARC LIEF赠款LE 130100104资助的，该赠款授予悉尼大学、澳大利亚国立大学、斯威本科技大学、昆士兰州大学、西澳大利亚大学、墨尔本大学、科廷科技大学、莫纳什大学和澳大利亚天文台。SkyMapper由澳大利亚国立大学天文学和天体物理学研究学院拥有和运营。调查数据由澳大利亚国立大学的SkyMapper团队处理和提供。全天空虚拟天文台（ASVO）的SkyMapper节点由国家计算基础设施（NCI）托管。澳大利亚天文学有限公司（AAL）和澳大利亚政府通过联邦教育投资基金（EIF）和国家合作研究基础设施战略（NCRIS），特别是国家电子研究合作工具和资源（NeCTAR）和澳大利亚国家数据服务项目（ANDS），为ASVO的SkyMapper节点的开发和支持提供了部分资金。这项工作利用了欧洲航天局（欧空局）使命盖亚任务（https：//www.cosmos.esa.int/gaia）的数据，这些数据由盖亚数据处理和分析联合会（DPAC; https：//www.cosmos.esa.int/web/gaia/dpac/consortium）处理。国家机构，特别是参加《盖亚多边协定》的机构，为该方案提供了资金。
This research is based on data collected under the NGTS project at the ESO La Silla Paranal Observatory. The NGTS facility is funded by a consortium of institutes consisting of the University of Warwick, the University of Leicester, Queen’s University Belfast, the University of Geneva, the Deutsches Zentrum fur Luft- und Raumfahrt e.V. (DLR; under the ‘Grosinvestition GI-NGTS’), the University of Cambridge, together with the UK Science and Technology Facilities Council (STFC; project reference ST/M001962/1). JAGJ is supported by STFC PhD studentship 1763096. PJW and RGW are supported by the STFC consolidated grant ST/P000495/1. AMB acknowledges the support of the Institute of Advanced Study, University of Warwick, and is also supported by the STFC consolidated grant ST/P000320/1. MNG is supported by the STFC award reference 1490409 as well as the Isaac Newton Studentship. CEP acknowledges support from the European Research Council under the SeismoSun Research Project No. 321141. JSJ acknowledges support by Fondecyt grant 1161218 and partial support by CATA-Basal (PB06, CONICYT). DYK acknowledges support by the STFC consolidated grant ST/P000320/1. GMK is supported by the Royal Society as a Royal Society University Research Fellow. We also acknowledge and thank the ISSI team led by AMB for useful discussions. This publication makes use of data products from the 2MASS, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This publication makes use of data products from the WISE, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. The national facility capability for SkyMapper has been funded through ARC LIEF grant LE130100104 from the Australian Research Council, awarded to the University of Sydney, the Australian National University, Swinburne University of Technology, the University of Queensland, the University of Western Australia, the University of Melbourne, Curtin University of Technology, Monash University and the Australian Astronomical Observatory. SkyMapper is owned and operated by the Australian National University’s Research School of Astronomy and Astrophysics. The survey data were processed and provided by the SkyMapper Team at the ANU. The SkyMapper node of the All-Sky Virtual Observatory (ASVO) is hosted at the National Computational Infrastructure (NCI). Development and support the SkyMapper node of the ASVO has been funded in part by Astronomy Australia Limited (AAL) and the Australian Government through the Commonwealth’s Education Investment Fund (EIF) and National Collaborative Research Infrastructure Strategy (NCRIS), particularly the National eResearch Collaboration Tools and Resources (NeCTAR) and the Australian National Data Service Projects (ANDS). This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC; https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.