INSIGHTS INTO THE HIGH-ENERGY γ-RAY EMISSION OF MARKARIAN 501 FROM EXTENSIVE MULTIFREQUENCY OBSERVATIONS IN THE FERMI ERA
By A. Abdo, M. Ackermann, M. Ajello, A. Allafort, L. Baldini, J. Ballet, G. Barbiellini, M. Baring, D. Bastieri, K. Bechtol and 440 more. 2011
165 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/5a36269802259dc70d426965aee4f76095cee511
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Citations in the corpus
- THE ORIGIN OF THE EXTRAGALACTIC GAMMA-RAY BACKGROUND AND IMPLICATIONS FOR DARK MATTER ANNIHILATION (2015, background): “…Finke et al. (2010), and use γa=1.7 and γb=2.6, which reproduces the long-term averaged spectra of bright BL Lacs with GeV-TeV measurements (RBS 0413, Mrk 421, Mrk 501, see Aliu et al. 2012; Abdo et al. 2011a,b) and those of bright FSRQs (like 3C 454.3, 3C 279, 3C 273, etc.) observed by Fermi-LAT.”
- THE EXTRAGALACTIC BACKGROUND LIGHT, THE HUBBLE CONSTANT, AND ANOMALIES: CONCLUSIONS FROM 20 YEARS OF TeV GAMMA-RAY OBSERVATIONS (2015, background): “…in 2000–2001 and MAGIC in 2004–2005, major outburst of PKS 2155–304 in 2006 observed by MAGIC and H.E.S.S.: Aharonian et al. 2002; Aleksić et al. 2010, 2012c; Abramowski et al. 2013, respectively), or to both (2006–2008 campaign on Markarian 421 by VERITAS, including flares: Abdo et al. 2011).”
- The extragalactic background light and the gamma-ray opacity of the universe (2012, background): “…279, PKS 1510-08) and spectral hardening (1ES 0502+675) in the GeV regime (Abdo, A. A. et al., 2010), while the spectra of other blazars (Mrk 421, Abdo et al., 2011b), (Mrk 501, Abdo et al., 2011a) extend without any cutoff to 300 GeV (Abdo et al., 2010b), or multi-TeV energies (Krennrich et…”
- BLAZARS AS ULTRA-HIGH-ENERGY COSMIC-RAY SOURCES: IMPLICATIONS FOR TeV GAMMA-RAY OBSERVATIONS (2011, background): “…IC 310 (Aleksíc et al. 2010; Neronov et al. 2010), intermediate-synchrotron-peaked objects like 3C 66A (Acciari et al. 2009a; Aliu et al. 2009; Abdo et al. 2011a) and BL Lac (Albert et al. 2007a; Abdo et al. 2011b), and the GeV luminous, high-redshift FSRQs 3C 279 (z=0.538; Aleksíc et al.…”