The Crab Nebula as a standard candle in very high-energy astrophysics
Abstract
The continuum high-energy gamma-ray emission between 1 GeV and 105 GeV from the Crab Nebula has been measured for the first time in overlapping energy bands by the Fermi large-area telescope (Fermi/LAT) below ≈100 GeV and by ground-based imaging air Cherenkov telescopes (IACTs) above ≈60 GeV. To follow up on the phenomenological approach suggested by Hillas et al. (1998), the broad band spectral and spatial measurement (from radio to low-energy gamma-rays <1 GeV) is used to extract the shape of the electron spectrum. While this model per construction provides an excellent description of the data at energies <1 GeV, the predicted inverse Compton component matches the combined Fermi/LAT and IACT measurements remarkably well after including all relevant seed photon fields and fitting the average magnetic field to B = (124 ± 6 (stat.) +15-6 (sys.)) μG. The close match of the resulting broad band inverse Compton component with the combined Fermi/LAT and IACTs data is used to derive instrument specific energy-calibration factors. These factors can be used to combine data from Fermi/LAT and IACTs without suffering from systematic uncertainties on the common energy scale. As a first application of the cross calibration, we derive an upper limit to the diffuse gamma-ray emission between 250 GeV and 1 TeV based upon the combined measurements of Fermi/LAT and the H.E.S.S. ground-based Cherenkov telescopes. Finally, the predictions of the magneto-hydrodynamic flow model of Kennel & Coroniti (1984) are compared to the measured SED.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- November 2010
- DOI:
- 10.1051/0004-6361/201014108
- arXiv:
- arXiv:1008.4524
- Bibcode:
- 2010A&A...523A...2M
- Keywords:
-
- ISM: individual objects: Crab Nebula;
- radiation mechanisms: non-thermal;
- acceleration of particles;
- magnetohydrodynamics (MHD);
- gamma rays: diffuse background;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- Added journal ref., corrected formula for production rates (missing frequency inserted)