A low level of extragalactic background light as revealed by γ-rays from blazars
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A. Noutsos | U. Schwanke | C. Boisson | H. Sol | D. Emmanoulopoulos | K. Bernlöhr | M. Panter | A. G. Akhperjanian | A. R. Bazer-Bachi | J. F. Glicenstein | P. M. Chadwick | H. J. Dickinson | S. J. Nolan | K. J. Orford | S. M. Rayner | M. Holleran | B. C. Raubenheimer | G. Fontaine | B. Khélifi | A. Djannati-Ataï | P. Espigat | R. Terrier | M. Hauser | G. Vasileiadis | G. Pelletier | A. Jacholkowska | J. A. Hinton | J. Ripken | F. Feinstein | S. Funk | W. Hofmann | B. Giebels | P. Goret | G. Heinzelmann | G. Hermann | Nu. Komin | A. Marcowith | M. de Naurois | S. Pita | M. Punch | M. Raue | O. Reimer | L. Rob | V. Sahakian | R. Steenkamp | C. Stegmann | J.-P. Tavernet | M. Tluczykont | C. van Eldik | C. Venter | P. Vincent | M. Beilicke | G. Rowell | V. Borrel | L. Costamante | D. Berge | A. Konopelko | T. Lohse | S. Gillessen | S. Klages | I. Braun | R. Cornils | T. J. L. McComb | J. M. Martin | C. Hadjichristidis | D. Spangler | D. Hauser | Y. A. Gallant | O. Martineau-Huynh | M. Lemoine-Goumard | I. J. Latham | Y. Fuchs | O. Bolz | A. M. Brown | B. Degrange | R. Le Gallou | M. Ouchrif | L. Saugé | R. Schlickeiser | C. Schuster | C. G. Théoret | S. J. Wagner | W. Benbow | N. Leroy | L. Rolland | F. Breitling | J. L. Osborne | S. Schlenker | G. Henri | A. Lemière | G. Pühlhofer | F. Aharonian | D. Horns | O. C. de Jager | L.-M. Chounet | C. Masterson | A. Reimer | H. J. Völk | L. O'C. Drury | G. Dubus | J. Raux | M. Siewert
[1] E. L. Wright. DIRBE minus 2MASS: Confirming the Cosmic Infrared Background at 2.2 Microns , 2000, astro-ph/0004192.
[2] T. Weekes,et al. Discovery of Spectral Variability of Markarian 421 at TeV Energies , 2002, astro-ph/0207184.
[3] L. Cambresy,et al. The Cosmic Infrared Background at 1.25 and 2.2 Microns Using DIRBE and 2MASS: A Contribution Not Due to Galaxies? , 2001 .
[4] Volker Bromm,et al. The contribution of the first stars to the cosmic infrared background , 2001, astro-ph/0111467.
[5] SIMULTANEOUS CONSTRAINTS ON THE SPECTRUM OF THE EXTRAGALACTIC BACKGROUND LIGHT AND THE INTRINSIC TeV SPECTRA OF MARKARIAN 421, MARKARIAN 501, AND H1426+428 , 2004, astro-ph/0406565.
[6] Stsci,et al. Observational Gamma-ray Cosmology , 2005, astro-ph/0502177.
[7] R. Arendt,et al. The Near-Infrared Background: Interplanetary Dust or Primordial Stars? , 2005, astro-ph/0508262.
[8] L. Drury,et al. Nonlinear theory of diffusive acceleration of particles by shock waves , 2001 .
[9] E. al.,et al. Observations of H1426+428 with HEGRA - Observations in 2002 and reanalysis of 1999&2000 data , 2003, astro-ph/0301437.
[10] E. al.,et al. The time averaged TeV energy spectrum of MKN 501 of the extraordinary 1997 outburst as measured with the stereoscopic Cherenkov telescope system of HEGRA , 1999, astro-ph/9903386.
[11] F. Aharonian,et al. TeV observations of H1426+428 with HEGRA , 2004 .
[12] E. Dwek,et al. A Tentative Detection of the Cosmic Infrared Background at 3.5 μm from COBE/DIRBE Observations , 1998 .
[13] A. Kashlinsky. Cosmic infrared background and early galaxy evolution , 2004 .
[14] B. Madore,et al. The First Detections of the Extragalactic Background Light at 3000, 5500, and 8000 Å. II. Measurement of Foreground Zodiacal Light , 2001, astro-ph/0112193.
[15] Piero MadauJoseph Silk. Population III and the near-infrared background excess , 2005 .
[16] M. Kawada,et al. Infrared Telescope in Space Observations of the Near-Infrared Extragalactic Background Light , 2004, astro-ph/0411593.
[17] R. Gould,et al. Opacity of the Universe to High-Energy Photons , 1966 .
[18] O. C. de Jager,et al. TeV gamma rays from 3C 279 - A possible probe of origin and intergalactic infrared radiation fields , 1992 .
[19] Comments on ``The first detections of the Extragalactic Background Light at 3000, 5500, and 8000 A'' by Bernstein, Freedman and Madore , 2003, astro-ph/0303196.
[20] Michael G. Hauser,et al. THE COSMIC INFRARED BACKGROUND: Measurements and Implications ⁄ , 2001 .
[21] Probing galaxy formation with high energy gamma-rays , 2000, astro-ph/0201119.
[22] J. Jelley. High-Energy γ-Ray Absorption in Space by a 3.5°K Microwave Field , 1966 .
[23] K. Abromeit. Music Received , 2023, Notes.
[24] A. I. Nikishov. ABSORPTION OF HIGH ENERGY PHOTONS IN THE UNIVERSE , 1961 .
[25] E. L. Wright,et al. Number Counts at 3 μm < λ < 10 μm from the Spitzer Space Telescope , 2004 .
[26] et al,et al. H.E.S.S. Observations of PKS 2155-304 , 2004, astro-ph/0411582.
[27] W. Freedman,et al. The First Detections of the Extragalactic Background Light at 3000, 5500, and 8000 Å. I. Results , 2001, astro-ph/0112153.
[28] L. Costamante,et al. TeV candidate BL Lac objects , 2001, astro-ph/0112201.
[29] Lucia Pozzetti,et al. Deep galaxy counts, extragalactic background light and the stellar baryon budget , 1999, astro-ph/9907315.
[30] T. Totani,et al. Diffuse Extragalactic Background Light versus Deep Galaxy Counts in the Subaru Deep Field: Missing Light in the Universe? , 2001, astro-ph/0102328.
[31] K. Mattila. Has the Optical Extragalactic Background Light Been Detected? , 2003 .