The multifrequency emission of Mrk 501 From radio to TeV gamma-rays

By K. Katarzyński, H. Sol, A. Kus. 2001

137 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/b46759e1fa097d944063d87d959f724cc1917ab9

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. A. Marscher
2. F. Tavecchio
3. Y. Kovalev
4. E. Orlando
5. C. Dermer
6. M. Lister
7. A. Pushkarev
8. L. Maraschi

In Nuclear and High Energy Physics

1. A. Marscher
2. F. Tavecchio
3. C. Dermer
4. E. Orlando
5. Y. Kovalev
6. M. Lister
7. L. Maraschi
8. A. Pushkarev

Citations in the corpus

• A hadronic origin for ultra-high-frequency-peaked BL Lac objects (2014, methodology): “The leptonic part of the code we present here is a direct evolution of the SSC code developed by Katarzyński et al. (2001) (hereafter K01) : a spherical emitting region of radius R, moving with Doppler factor δ in a relativistic jet with angle ϑ to the line of sight, is filled with a tangled,…”
• Photopolarimetric Monitoring of Blazars in the Optical and Near-Infrared Bands with the Kanata Telescope. I. Correlations between Flux, Color, and Polarization (2011, background): “In addition, it has been reported that the UV–IR emission of Mrk 501 can be reproduced with a strong contribution of an elliptical galaxy (Katarzyński et al. 2001).”
• Log-parabolic spectra and particle acceleration in blazars. III. SSC emission in the TeV band from Mkn 501 (2005, unknown): “As a further point Konopelko et al. (2003) and Krawczynski et al. (2002) usedδ values of 50 and 45, respectively, while Katarzynski et al. (2001) used 14, very close to our choice.”
• Variable Very High Energy γ-Ray Emission from Markarian 501 (2007, methodology): “…− 36, 0.07 − 0.6G from 1997 SEDs modeled with one-zone SSC requiring γ-ray transparency of the emitting blob; Kataoka et al. (1999): δ, B≃15, 0.2G from one-zone SSC modeling of simultaneous 1996 SED; Katarzyński et al. (2001): δ, B = 14, 0.2G from SSC modeling of non-simultaneous broadband SED.”
• Parsec-Scale Properties of Markarian 501 (2003, methodology): “Similarly, in Mkn 501 the expected Doppler factor should be > ∼ 10, as obtained from fits of synchrotron selfCompton (SSC) models (Katarzyński et al. 2001; Tavecchio et al. 2001).”
• INSIGHTS INTO THE HIGH-ENERGY γ-RAY EMISSION OF MARKARIAN 501 FROM EXTENSIVE MULTIFREQUENCY OBSERVATIONS IN THE FERMI ERA (2011, methodology): “…studied in the past (e.g., Pian et al. 1998; Villata & Raiteri 1999; Krawczynski et al. 2000; Sambruna et al. 2000; Tavecchio et al. 2001; Katarzyński et al. 2001; Ghisellini et al. 2002; Gliozzi et al. 2006; Anderhub et al. 2009), but the nature of this object is still far from being…”