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The extended lobes of radio galaxies are examined as sources of X-ray and gamma-ray emission via inverse Compton scattering of 3K background photons. The Compton spectra of two exemplary examples, Fornax A and Centaurus A, are estimated…

天体物理学 · 物理学 2009-06-23 C. C. Cheung

With assistance of the identified/associated sources in the second Fermi Large Area Telescope (LAT) catalog, we analyze and resolve the spatial distribution and the distributions of the gamma-ray spectral and variability indices of the…

高能天体物理现象 · 物理学 2015-06-15 Zhu Mao , Yun-Wei Yu

The small angular scale fluctuations of the (on large scale) isotropic gamma-ray background (IGRB) carry information about the presence of unresolved source classes. A guaranteed contribution to the IGRB is expected from the unresolved…

高能天体物理现象 · 物理学 2019-08-15 A. Cuoco , T. Linden , M. N. Mazziotta , J. M. Siegal-Gaskins , Vincenzo Vitale , E. Komatsu

A Galactic cosmic-ray transport model featuring non-homogeneous transport has been developed over the latest years. This setup is aimed at reproducing gamma-ray observations in different regions of the Galaxy (with particular focus on the…

高能天体物理现象 · 物理学 2022-10-18 Pedro De la Torre Luque , Daniele Gaggero , Dario Grasso

We study the capabilities of the Fermi-LAT instrument on board of the Fermi mission to constrain particle dark matter properties, as annihilation cross section, mass and branching ratio into dominant annihilation channels, with gamma-ray…

高能天体物理现象 · 物理学 2017-02-22 Nicolas Bernal , Sergio Palomares-Ruiz

We propose a method of measurement of extragalactic magnetic fields in observations of TeV gamma-rays from distant blazars. Multi-TeV gamma-rays are emitted by these sources in narrow jet with opening angle of few degrees. These primary…

天体物理学 · 物理学 2008-11-26 A. Neronov , D. V. Semikoz

X-ray and gamma-ray observations can help understand the origin of the electron and positron signals reported by ATIC, PAMELA, PPB-BETS, and Fermi. It remains unclear whether the observed high-energy electrons and positrons are produced by…

高能天体物理现象 · 物理学 2012-04-03 Antoine Calvez , Warren Essey , Malcolm Fairbairn , Alexander Kusenko , Michael Loewenstein

The launch of the Fermi gamma-ray space telescope and the imaging air Cerenkov telescopes H.E.S.S., MAGIC, and VERITAS have substantially transformed our knowledge of gamma-ray sources in the last decade. The extragalactic gamma-ray sky is…

高能天体物理现象 · 物理学 2013-09-02 C. Pfrommer

We report on the results of a search for $\gamma$-ray pair halos with a stacking analysis of low-redshift blazars using data from the Fermi Large Area Telescope. For this analysis we used a number of a-priori selection criteria, including…

高能天体物理现象 · 物理学 2015-11-25 Wenlei Chen , James H. Buckley , Francesc Ferrer

2 years worth of archival FERMI-LAT data was used to search for the gamma-ray emission from the Andromeda galaxy. The data show no noticeable elliptical image. Subsequent on-off source aperture photometry analysis using a CO image template…

高能天体物理现象 · 物理学 2015-05-19 H. Ögelman , N. Aksaker , S. Anılan , H. Dereli , N. Emrahoğlu , I. Yegingil

We report the detection of a cross-correlation signal between {\it Fermi} Large Area Telescope diffuse gamma-ray maps and catalogs of clusters. In our analysis, we considered three different catalogs: WHL12, redMaPPer and PlanckSZ. They all…

宇宙学与河外天体物理 · 物理学 2017-02-06 Enzo Branchini , Stefano Camera , Alessandro Cuoco , Nicolao Fornengo , Marco Regis , Matteo Viel , Jun-Qing Xia

Analyses have found a "haze" of anomalous microwave emission surrounding the Galactic Center in the WMAP sky maps. A recent study using Fermi data detected a similar haze in the gamma-ray. Several studies have modeled these hazes as…

高能天体物理现象 · 物理学 2015-05-18 Matthew McQuinn , Matias Zaldarriaga

LHAASO, a ground-based observatory, is unveiling new frontiers in our understanding of high-energy $\gamma-$rays and cosmic rays. It has recently observed high energy diffuse $\gamma-$rays from the Galactic plane in the TeV-PeV range. For…

高能物理 - 唯象学 · 物理学 2025-09-17 Celine Boehm , Ranjan Laha , Tarak Nath Maity

The isotropic diffuse $\gamma$-ray background (IGRB) has been detected by various experiments and recently the Fermi-LAT Collaboration has precisely measured its spectrum in a wide energy range. The origin of the IGRB is still unclear and…

高能天体物理现象 · 物理学 2016-06-22 Mattia Di Mauro

All-sky explorations by Fermi-LAT have revolutionized our view of the gamma-ray sky. While its ongoing all-sky survey counts thousands of sources, essential issues related to the nature of unassociated sources call for sensitive all-sky…

高能天体物理现象 · 物理学 2016-06-22 Eugenio Bottacini , Marco Ajello

A leading hypothesis for the nature of the elusive dark matter are thermally produced, weakly interacting massive particles that arise in many theories beyond the standard model of particle physics. Their self-annihilation in astrophysical…

高能物理 - 唯象学 · 物理学 2017-08-23 Torsten Bringmann

Building on our previous cross-correlation analysis (Xia et al. 2011) between the isotropic gamma-ray background (IGRB) and different tracers of the large-scale structure of the universe, we update our results using 60-months of data from…

宇宙学与河外天体物理 · 物理学 2015-06-24 Jun-Qing Xia , Alessandro Cuoco , Enzo Branchini , Matteo Viel

The Fermi Gamma-ray Space Telescope has been detecting a wealth of sources where the multi-wavelength counterpart is either inconclusive or missing altogether. We present a combination of factors that can be used to identify…

高能天体物理现象 · 物理学 2015-06-17 F. Acero , D. Donato , R. Ojha , J. Stevens , P. G. Edwards , E. Ferrara , J. Blanchard , J. E. J. Lovell , D. J. Thompson

We search for gamma-ray emission from 114 Galactic high mass X-ray binaries, including 4 well studied catalogued sources, in 12.5 years of Fermi-LAT data in conjunction with the 10-year point source catalogue. Where a gamma-ray excess…

高能天体物理现象 · 物理学 2022-03-02 Max Harvey , Cameron B. Rulten , Paula M. Chadwick

Recent evidence for a large Galactic halo, based on cosmic-ray radioactive nuclei, implies a significant contribution from inverse Compton emission at high Galactic latitudes. We present predictions for the expected intensity distribution,…

天体物理学 · 物理学 2007-05-23 A. W. Strong , I. V. Moskalenko , O. Reimer