The TANAMI Multiwavelength Program: Dynamic spectral energy distributions of southern blazars⋆-猫眼课题宝

DOI：

10.1051/0004-6361/201628595

发表时间：

2016-05

期刊：

Astronomy and Astrophysics

影响因子：

6.5

通讯作者：

中科院分区：

物理与天体物理2区

文献类型：

作者：

F. Krauß;J. Wilms;M. Kadler;R. Ojha;R. Schulz;J. Trustedt;P. Edwards;J. Stevens;E. Ros;W. Baumgartner;T. Beuchert;J. Blanchard;S. Buson;B. Carpenter;T. Dauser;S. Falkner;N. Gehrels;C. Grafe;S. Gulyaev;H. Hase;S. Horiuchi;A. Kreikenbohm;I. Kreykenbohm;M. Langejahn;K. Leiter;J. Lovell;C. Muller;T. Natusch;R. Nesci;T. Pursimo;C. Phillips;C. Plotz;J. Quick;A. Tzioumis;S. Weston

我们感谢裁判的有益评论。我们感谢S。库提尼为她有用的评论。我们感谢S。Markoff进行有益的讨论。我们感谢J.珀金斯，L。Baldini和S.迪格尔仔细阅读手稿。感谢M。巴克斯顿感谢她对SMARTS数据的帮助。我们感谢Deutsche Forschungsgemeinschaft grant WI 1860-10/1（TANAMI）和GRK 1147、Deutsches Zentrum fur Luft- und Raumfahrt赠款50 OR 1311和50 OR 1103以及Helmholtz Alliance for Astroparticle Physics（HAP）的支持和部分资助。这项研究由NASA通过费米客座研究员赠款NNH 09 ZDA 001 N，NH 10 ZDA 001 N，NNH 12 ZDA 001 N和NNH 13 ZDA 001 N-FERMI提供部分资金。这项研究得到了戈达德太空飞行中心NASA博士后项目的支持，该项目由橡树岭联合大学通过与NASA的合同管理。急诊室部分由西班牙MINECO项目AYA 2012 -38491-C 02 -01和Generalitat Valenciana项目PROMETEO II/2014/057支持。感谢J。Davis开发了slxfig模块，该模块用于准备本工作中的图形。感谢T。约翰逊的费米/LAT SED脚本，这是用来计算费米/LAT光谱。这项研究利用了由德国班贝格的Karl Remeis-Observatory博士在http://www.sternwarte.uni-erlangen.de/isis/上提供的ISIS脚本集合。长基线阵列和澳大利亚望远镜紧凑阵列是澳大利亚望远镜国家设施的一部分，该设施由澳大利亚联邦资助，作为由CSIRO管理的国家设施运行。本文利用了最新的SMARTS光学/近红外光变曲线，可在www.astro.yale.edu/smarts/glast/home.php上获得。费米LAT协作感谢许多机构和研究所的慷慨持续支持，这些机构和研究所支持LAT的开发和运行以及科学数据分析。这些机构包括美国的国家航空和航天局和能源部、法国的原子能委员会和国家科学研究中心/国家核物理和粒子物理研究所、意大利的意大利空间研究所和国家核物理研究所、教育、文化、体育、科学和技术部（文部科学省）、高能加速器研究组织（KEK）和日本宇宙航空研究开发机构（JAXA）在日本，和K.A.瓦伦堡基金会、瑞典研究理事会和瑞典国家航天委员会。感谢意大利国家天文学研究所和法国国家空间研究中心在运行阶段为科学分析提供的额外支持

We thank the referee for helpful comments. We thank S. Cutini for her useful comments. We thank S. Markoff for helpful discussions. We thank J. Perkins, L. Baldini, and S. Digel for carefully reading the manuscript. We thank M. Buxton for her help with the SMARTS data. We acknowledge support and partial funding by the Deutsche Forschungsgemeinschaft grant WI 1860-10/1 (TANAMI) and GRK 1147, Deutsches Zentrum fur Luft- und Raumfahrt grants 50 OR 1311 and 50 OR 1103, and the Helmholtz Alliance for Astroparticle Physics (HAP). This research was funded in part by NASA through Fermi Guest Investigator grants NNH09ZDA001N, NH10ZDA001N, NNH12ZDA001N, and NNH13ZDA001N-FERMI. This research was supported by an appointment to the NASA Postdoctoral Program at the Goddard Space Flight Center, administered by Oak Ridge Associated Universities through a contract with NASA. E.R. was partially supported by the Spanish MINECO project AYA2012-38491-C02-01 and by the Generalitat Valenciana project PROMETEO II/2014/057. We thank J. E. Davis for the development of the slxfig module that was used to prepare the figures in this work. We thank T. Johnson for the Fermi/LAT SED scripts, which were used to calculate the Fermi/LAT spectra. This research has made use of a collection of ISIS scripts provided by the Dr. Karl Remeis-Observatory, Bamberg, Germany at http://www.sternwarte.uni-erlangen.de/isis/. The Long Baseline Array and Australia Telescope Compact Array are part of the Australia Telescope National Facility, which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. This paper has made use of up-to-date SMARTS optical/near-infrared light curves that are available at www.astro.yale.edu/smarts/glast/home.php. The Fermi LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT as well as scientific data analysis. These include the National Aeronautics and Space Administration and the Department of Energy in the United States, the Commissariat a l’Energie Atomique and the Centre National de la Recherche Scientifique / Institut National de Physique Nucleaire et de Physique des Particules in France, the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), High Energy Accelerator Research Organization (KEK) and Japan Aerospace Exploration Agency (JAXA) in Japan, and the K.A. Wallenberg Foundation, the Swedish Research Council and the Swedish National Space Board in Sweden. Additional support for science analysis during the operations phase is gratefully acknowledged from the Istituto Nazionale di Astrofisica in Italy and the Centre National d’Etudes Spatiales in France

The TANAMI Multiwavelength Program: Dynamic spectral energy distributions of southern blazars⋆

文献摘要

被引文献

相似文献