Incremental Fermi Large Area Telescope Fourth Source Catalog

被引：350

作者：

Abdollahi, S. ^{[1
,14
,15
]}

Acero, F. ^{[2
,3
]}

Baldini, L. ^{[4
,5
]}

Ballet, J. ^{[2
,3
]}

Bastieri, D. ^{[6
,7
,8
]}

Bellazzini, R. ^{[9
]}

Berenji, B. ^{[10
]}

Berretta, A. ^{[11
]}

Bissaldi, E. ^{[12
,13
]}

Blandford, R. D. ^{[14
,15
]}

Bloom, E. ^{[14
,15
]}

Bonino, R. ^{[16
,17
]}

Brill, A. ^{[18
]}

Britto, R. J. ^{[19
]}

Bruel, P. ^{[20
]}

Burnett, T. H. ^{[21
]}

Buson, S. ^{[22
]}

Cameron, R. A. ^{[14
,15
]}

Caputo, R. ^{[18
]}

Caraveo, P. A. ^{[23
]}

Castro, D. ^{[18
,24
]}

Chaty, S. ^{[2
,3
]}

Cheung, C. C. ^{[25
]}

Chiaro, G. ^{[23
]}

Cibrario, N. ^{[16
]}

Ciprini, S. ^{[26
,27
]}

Coronado-Blazquez, J. ^{[28
,29
]}

Crnogorcevic, M. ^{[30
]}

Cutini, S. ^{[31
]}

D'Ammando, F. ^{[32
]}

De Gaetano, S. ^{[12
,13
]}

Digel, S. W. ^{[14
,15
]}

Di Lalla, N. ^{[14
,15
]}

Dirirsa, F. ^{[33
,34
]}

Di Venere, L. ^{[12
,13
]}

Dominguez, A. ^{[35
]}

Fallah Ramazani, V. ^{[36
]}

Fegan, S. J. ^{[20
]}

Ferrara, E. C. ^{[18
,30
,37
]}

Fiori, A. ^{[38
]}

Fleischhack, H. ^{[18
,37
,39
]}

Franckowiak, A. ^{[36
]}

Fukazawa, Y. ^{[40
]}

Funk, S. ^{[41
]}

Fusco, P. ^{[12
,13
]}

Galanti, G. ^{[23
]}

Gammaldi, V. ^{[28
,29
]}

Gargano, F. ^{[13
]}

Garrappa, S. ^{[42
]}

Gasparrini, D. ^{[26
,27
]}

机构：

[1] Univ Toulouse, IRAP, CNRS, UPS,CNES, F-31028 Toulouse, France

[2] Univ Paris Saclay, F-91191 Gif Sur Yvette, France

[3] Univ Paris Cite, CEA, CNRS, AIM, F-91191 Gif Sur Yvette, France

[4] Univ Pisa, I-56127 Pisa, Italy

[5] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[6] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[7] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy

[8] Univ Padua, Ctr Space Studies & Act G Colombo, Via Venezia 15, I-35131 Padua, Italy

[9] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[10] Calif State Univ Los Angeles, Dept Phys & Astron, Los Angeles, CA 90032 USA

[11] Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy

[12] Univ & Politecn Bari, Dipartimento Fis M Merlin, Via Amendola 173, I-70126 Bari, Italy

[13] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy

[14] Stanford Univ, Dept Phys, WW Hansen Expt Phys Lab, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA

[15] Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA

[16] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy

[17] Univ Torino, Dipartimento Fis, I-10125 Turin, Italy

[18] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[19] Univ Free State, Dept Phys, POB 339, ZA-9300 Bloemfontein, South Africa

[20] Ecole Polytech, CNRS, Lab Leprince Ringuet, IN2P3, F-91128 Palaiseau, France

[21] Univ Washington, Dept Phys, Seattle, WA 98195 USA

[22] Univ Wurzburg, Inst Theoret Phys & Astrophys, D-97074 Wurzburg, Germany

[23] INAF, Ist Astrofis Spaziale & Fis Cosm Milano, Via E Bassini 15, I-20133 Milan, Italy

[24] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[25] Naval Res Lab, Div Space Sci, Washington, DC 20375 USA

[26] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy

[27] Agenzia Spaziale Italiana, Space Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy

[28] Univ Autonoma Madrid, Inst Fis Teor, UAM, CSIC, E-28049 Madrid, Spain

[29] Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain

[30] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[31] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy

[32] INAF, Ist Radioastron, I-40129 Bologna, Italy

[33] Ethiopian Space Sci & Technol Inst, Astron & Astrophys Res Dev Dept, Entoto Observ, Addis Ababa, Ethiopia

[34] Ethiopian Space Sci & Technol Inst, Res Ctr, Addis Ababa, Ethiopia

[35] Univ Complutense Madrid, Grp Altas Energias, E-28040 Madrid, Spain

[36] Ruhr Univ Bochum, Fac Phys & Astron, Astron Inst AIRUB, D-44780 Bochum, Germany

[37] Ctr Res & Explorat Space Sci & Technol CRESST, Greenbelt, MD 20771 USA

[38] Univ Pisa, Dipartimento Fis Enrico Fermi, I-56127 Pisa, Italy

[39] Catholic Univ Amer, Washington, DC 20064 USA

[40] Hiroshima Univ, Dept Phys Sci, Hiroshima 7398526, Japan

[41] Friedrich Alexander Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, Erwin Rommel Str 1, D-91058 Erlangen, Germany

[42] Deutsch Elektronen Synchrotron DESY, D-15738 Zeuthen, Germany

[43] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[44] Univ Bordeaux, CNRS, LP2I Bordeaux, UMR 5797, F-33170 Gradignan, France

[45] George Washington Univ, Dept Phys, 725 21st St NW, Washington, DC 20052 USA

[46] Georg August Univ Gottingen, Inst Theoret Phys, Fac Phys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany

[47] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

[48] Univ North Florida, Dept Phys, 1 UNF Dr, Jacksonville, FL 32224 USA

[49] Chinese Acad Sci, Yunnan Observ, 396 Yangfangwang, Kunming 650216, Yunnan, Peoples R China

[50] Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, 396 Yangfangwang, Kunming 650216, Yunnan, Peoples R China

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2022年 / 260卷 / 02期

基金：

美国国家科学基金会; 瑞典研究理事会; 美国国家航空航天局;

关键词：

GAMMA-RAY EMISSION; TRANSITIONAL MILLISECOND PULSAR; COSMIC-RAY; X-RAY; DISCOVERY; BLAZAR; 3FHL;

D O I：

10.3847/1538-4365/ac6751

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

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.

引用

页数：24

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