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Incremental Fermi Large Area Telescope Fourth Source Catalog

文献类型:期刊论文

作者Abdollahi, S.83; Acero, F.82; Baldini, L.81; Ballet, J.82; Bastieri, D.78,79,80; Bellazzini, R.77; Berenji, B.76; Berretta, A.75; Bissaldi, E.73,74; Blandford, R. D.72
刊名ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
出版日期2022-06-01
卷号260期号:2
ISSN号0067-0049
DOI10.3847/1538-4365/ac6751
产权排序第48完成单位
文献子类Article
英文摘要

We present an incremental version (4FGL-DR3, for Data Release 3) of the fourth Fermi Large Area Telescope (LAT) catalog of gamma-ray sources. Based on the first 12 years of science data in the energy range from 50 MeV to 1 TeV, it contains 6658 sources. The analysis improves on that used for the 4FGL catalog over eight years of data: more sources are fit with curved spectra, we introduce a more robust spectral parameterization for pulsars, and we extend the spectral points to 1 TeV. The spectral parameters, spectral energy distributions, and associations are updated for all sources. Light curves are rebuilt for all sources with 1 yr intervals (not 2 month intervals). Among the 5064 original 4FGL sources, 16 were deleted, 112 are formally below the detection threshold over 12 yr (but are kept in the list), while 74 are newly associated, 10 have an improved association, and seven associations were withdrawn. Pulsars are split explicitly between young and millisecond pulsars. Pulsars and binaries newly detected in LAT sources, as well as more than 100 newly classified blazars, are reported. We add three extended sources and 1607 new point sources, mostly just above the detection threshold, among which eight are considered identified, and 699 have a plausible counterpart at other wavelengths. We discuss the degree-scale residuals to the global sky model and clusters of soft unassociated point sources close to the Galactic plane, which are possibly related to limitations of the interstellar emission model and missing extended sources.

学科主题天文学 ; 天体物理学 ; 实测天体物理学 ; 星系与宇宙学
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词GAMMA-RAY EMISSION ; TRANSITIONAL MILLISECOND PULSAR ; COSMIC-RAY ; X-RAY ; DISCOVERY ; BLAZAR ; 3FHL
资助项目Department of Energy in the United States ; Commissariat a l'Energie Atomique ; Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France ; Agenzia Spaziale Italiana ; Istituto Nazionale di Fisica Nucleare in Italy ; Ministry of Education, Culture, Sports, Science and Technology (MEXT) ; High Energy Accelerator Research Organization (KEK) ; Japan Aerospace Exploration Agency (JAXA) in Japan ; K. A. Wallenberg Foundation ; Swedish Research Council ; Swedish National Space Board in Sweden ; Istituto Nazionale di Astrofisica in Italy ; DOE[DE-AC02-76SF00515] ; National Aeronautics and Space Administration ; NSF[1816904] ; Centre National d'Etudes Spatiales in France
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP Publishing Ltd
WOS记录号WOS:000819154400001
资助机构Department of Energy in the United States ; Commissariat a l'Energie Atomique ; Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France ; Agenzia Spaziale Italiana ; Istituto Nazionale di Fisica Nucleare in Italy ; Ministry of Education, Culture, Sports, Science and Technology (MEXT) ; High Energy Accelerator Research Organization (KEK) ; Japan Aerospace Exploration Agency (JAXA) in Japan ; K. A. Wallenberg Foundation ; Swedish Research Council ; Swedish National Space Board in Sweden ; Istituto Nazionale di Astrofisica in Italy ; DOE[DE-AC02-76SF00515] ; National Aeronautics and Space Administration ; NSF[1816904] ; Centre National d'Etudes Spatiales in France
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/25237]  
专题云南天文台_高能天体物理研究组
云南天文台_中国科学院天体结构与演化重点实验室
通讯作者Ballet, J.
作者单位1.Center for Astrophysics and Cosmology, University of Nova Gorica, Nova Gorica, Slovenia
2.Praxis Inc., Alexandria, VA 22303, USA;
3.Institució Catalana de Recerca i Estudis Avançats (ICREA), E-08010 Barcelona, Spain;
4.Institut d'Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain;
5.Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Magrans s/n, E-08193 Barcelona, Spain;
6.Department of Physics, University of Maryland, College Park, MD 20742, USA;
7.Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya 464-8601, Japan;
8.Purdue University Northwest, Hammond, IN 46323, USA;
9.Laboratoire d'Astrophysique de Bordeaux, Université de Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, F-33615 Pessac, France;
10.NYCB Real-Time Computing Inc., Lattingtown, NY 11560-1025, USA;
推荐引用方式
GB/T 7714
Abdollahi, S.,Acero, F.,Baldini, L.,et al. Incremental Fermi Large Area Telescope Fourth Source Catalog[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2022,260(2).
APA Abdollahi, S..,Acero, F..,Baldini, L..,Ballet, J..,Bastieri, D..,...&Zaharijas, G..(2022).Incremental Fermi Large Area Telescope Fourth Source Catalog.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,260(2).
MLA Abdollahi, S.,et al."Incremental Fermi Large Area Telescope Fourth Source Catalog".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 260.2(2022).

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来源:云南天文台

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