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Title: Development of the Model of Galactic Interstellar Emission for Standard Point-Source Analysis of Fermi Large Area Telescope Data

Journal Article · · The Astrophysical Journal. Supplement Series (Online)
 [1]
  1. Commissariat a l'Energie Atomique et aux Energies Alternatives (CEA-Saclay), Gif-sur-Yvette (France); et al.

Most of the celestial γ rays detected by the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope originate from the interstellar medium when energetic cosmic rays interact with interstellar nucleons and photons. Conventional point and extended source studies rely on the modeling of this diffuse emission for accurate characterization. We describe here the development of the Galactic Interstellar Emission Model (GIEM) that is the standard adopted by the LAT Collaboration and is publicly available. The model is based on a linear combination of maps for interstellar gas column density in Galactocentric annuli and for the inverse Compton emission produced in the Galaxy. We also include in the GIEM large-scale structures like Loop I and the Fermi bubbles. The measured gas emissivity spectra con rm that the cosmic-ray proton density decreases with Galactocentric distance beyond 5 kpc from the Galactic Center. The measurements also suggest a softening of the proton spectrum with Galactocentric distance. We observe that the Fermi bubbles have boundaries with a shape similar to a catenary at latitudes below 20° and we observe an enhanced emission toward their base extending in the North and South Galactic direction and located within ~4° of the Galactic Center.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
Fermi LAT Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1355675
Journal Information:
The Astrophysical Journal. Supplement Series (Online), Vol. 223, Issue 2; ISSN 1538-4365
Publisher:
American Astronomical Society/IOPCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 251 works
Citation information provided by
Web of Science

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The $γ$-ray spectrum of the core of Centaurus A as observed with H.E.S.S. and Fermi-LAT text January 2018
Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar text January 2018
Detection of persistent VHE gamma-ray emission from PKS 1510-089 by the MAGIC telescopes during low states between 2012 and 2017 text January 2018
Fermi-LAT Stacking Analysis Technique: An Application to Extreme Blazars and Prospects for their CTA Detection text January 2019
Fermi Large Area Telescope Fourth Source Catalog text January 2020
Gamma-ray blazar spectra with H.E.S.S. II mono analysis: The case of PKS 2155−304 and PG 1553+113 journal April 2017
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Multiwavelength observations of a VHE gamma-ray flare from PKS 1510−089 in 2015 text January 2017
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The Einstein@Home Gamma-ray Pulsar Survey. I. Search Methods, Sensitivity and Discovery of New Young Gamma-ray Pulsars text January 2016
Galactic Bulge Preferred Over Dark Matter for the Galactic Center Gamma-Ray Excess text January 2016
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High-energy gamma-ray activity from V404 Cygni detected by AGILE during the 2015 June outburst text January 2017
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The Einstein@Home Gamma-Ray Pulsar Survey II. Source Selection, Spectral Analysis and Multi-wavelength Follow-up text January 2017
Imprints of Cosmic Rays in Multifrequency Observations of the Interstellar Emission text January 2017
FBQS J1644+2619: multiwavelength properties and its place in the class of gamma-ray emitting Narrow Line Seyfert 1s text January 2018
SED constraints on the highest-$z$ blazar jet: QSO J0906+6930 text January 2018
Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar text January 2018
Observing and modeling the gamma-ray emission from pulsar/pulsar wind nebula complex PSR J0205+6449/3C 58 text January 2018
A Luminous and Highly-variable Gamma-ray Flare Following the 2017 Periastron of PSR B1259-63/LS 2883 text January 2018
Gamma-ray flaring activity of NGC 1275 in 2016-2017 measured by MAGIC text January 2018
The first catalog of Fermi-LAT sources below 100 MeV text January 2018
Disentangling multiple high-energy emission components in the Vela X pulsar wind nebula with the Fermi Large Area Telescope text January 2018
On the progressive hardening of the cosmic-ray proton spectrum in the inner Galaxy text January 2018
Evidence for Cosmic-Ray Escape in the Small Magellanic Cloud using Fermi Gamma-rays text January 2018
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Hard and bright gamma-ray emission at the base of the Fermi bubbles text January 2019
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