Results 11 to 20 of about 18,989 (273)

Astrophysical Neutrinos and Blazars [PDF]

open access: yesUniverse, 2021
We review and discuss recent results on the search for correlations between astrophysical neutrinos and γ-ray-detected sources, with many extragalactic studies reporting potential associations with different types of blazars.
P. Giommi, P. Padovani
semanticscholar   +6 more sources

Blazars at the Cosmic Dawn [PDF]

open access: yesThe Astrophysical Journal, 2020
The uncharted territory of the high-redshift (z ≳ 3) universe holds the key to understanding the evolution of quasars. In an attempt to identify the most extreme members of the quasar population, that is, blazars, we have carried out a multiwavelength ...
V. Paliya   +7 more
semanticscholar   +7 more sources

Origin of Blazar Activity [PDF]

open access: bronzeSymposium - International Astronomical Union, 1999
Models of Blazars based on the propagation of finite discontinuities or fronts in the Poynting flux jet from the innermost regions of an accretion disk around a black hole are discussed. Such fronts may be responsible for short time–scale (from less than hours to days) flares in different wavebands from high frequency radioband to TeV, with delay in ...
M. M. Romanova
openalex   +4 more sources

Characterizing Long-term Optical Variability Properties of γ-Ray-bright Blazars [PDF]

open access: yesAstrophysical Journal, 2021
Optical observations of a sample of 12 γ-ray-bright blazars from four optical data archives—American Association of Variable Star Observers, Small and Moderate Aperture Research Telescope System, Catalina, and Steward Observatory—are compiled to create ...
G. Bhatta
semanticscholar   +1 more source

Classification of unassociated fermi-LAT sources [PDF]

open access: yesITM Web of Conferences, 2022
The Large Area Telescope (LAT) on board NASA’s Fermi Gamma-ray Space telescope has detected 5788 sources in the 4FGL catalogue. Among them, 271 have been associated to pulsars, 3436 to blazars, and 1782 remain unassociated sources.
Meng Qiyu
doaj   +1 more source

An Optical Overview of Blazars with LAMOST. I. Hunting Changing-look Blazars and New Redshift Estimates [PDF]

open access: yes, 2021
The extragalactic γ-rays sky observed by the Fermi Large Area Telescope (LAT) is dominated by blazars. In the fourth release of the Fermi LAT Point Source Catalog (4FGL) are sources showing a multifrequency behavior similar to that of blazars but lacking
H. Peña-Herazo   +8 more
semanticscholar   +1 more source

The Spectral Energy Distributions for 4FGL Blazars

open access: yesAstrophysical Journal Supplement Series, 2022
In this paper, the multiwavelength data from radio to X-ray bands for 2709 blazars in the 4FGL-DR3 catalog are compiled to calculate their spectral energy distributions using a parabolic equation log(νfν)=P1logν−P22+P3 .
J. H. Yang   +21 more
semanticscholar   +1 more source

Testing the Blazar Sequence with Spectra of Recently Discovered Dim Blazars from the Fermi Unassociated Catalog

open access: yesThe Astrophysical Journal, 2023
Recent works have developed samples of blazars from among the Fermi Large Area Telescope unassociated sources via machine-learning comparisons with known blazar samples. Continued analysis of these new blazars tests the predictions of the blazar sequence
Stephen Kerby, Abraham D. Falcone
doaj   +1 more source

The recognition of blazars and the blazar spectral sequence [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2005
Accepted for publication in ...
Ian Browne, Sonia Anton, Sonia Anton
openaire   +3 more sources

The blazar sequence revised [PDF]

open access: yesAstronomische Nachrichten, 2021
We propose and test a fairly simple idea that could account for the blazar sequence: all jets are launched with similar energy per baryon, independently of their power. For instance, flat‐spectrum radio quasars (FSRQs), the most powerful jets, manage to accelerate to high bulk Lorentz factor, as observed in the radio.
Dimitrios Giannios   +2 more
openaire   +3 more sources

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