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Incremental Fermi Large Area Telescope fourth source catalog

Author
Abdollah, S.; Coronado-Blázquez, Javier; Gammaldi, Viviana; Sánchez Conde, Miguel Ángeluntranslated
Entity
UAM. Departamento de Física Teórica
Publisher
American Astronomical Society
Date
2022-06-01
Citation
10.3847/1538-4365/ac6751
The Astrophysical Journal Supplement Series 260.2 (2022): 53
 
 
 
ISSN
0067-0049 (print); 1538-4365 (online)
DOI
10.3847/1538-4365/ac6751
Editor's Version
https://doi.org/10.3847/1538-4365/ac6751
Subjects
Blazars; Galaxies; BL Lacertae Object; Física
URI
http://hdl.handle.net/10486/706443
Note
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
Rights
© 2022 The Author(s)

Licencia Creative Commons
Esta obra está bajo una Licencia Creative Commons Atribución 4.0 Internacional.

Abstract

We present an incremental version (4FGL-DR3, for Data Release 3) of the fourth Fermi Large Area Telescope (LAT) catalog of 3-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(but are kept in the list), while 74 are newly associated, 10 have an improved association, and seven associations were withdrawn.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
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Google™ Scholar:Abdollah, S. - Coronado-Blázquez, Javier - Gammaldi, Viviana - Sánchez Conde, Miguel Ángel

This item appears in the following Collection(s)

  • Producción científica en acceso abierto de la UAM [16855]

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All the documents from Biblos-e Archivo are protected by copyrights. Some rights reserved.
Universidad Autónoma de Madrid. Biblioteca
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