Fa. Aharonian et al., Observations of Mkn 421 during 1997 and 1998 in the energy range above 500GeV with the HEGRA stereoscopic Cherenkov telescope system, ASTRON ASTR, 350(3), 1999, pp. 757-764
Since its commissioning in fall 1996, the stereoscopic system of Imaging At
mospheric Cherenkov Telescopes (IACTs) of HEGRA, with an energy flux sensit
ivity nu F-nu at 1 TeV of 10(-11) erg cm(-2) s(-1) for one hour of observat
ion time, has been used to monitor the BL Lac object Mkn 421 on a regular b
asis. In this paper, we report detailed temporal and spectral information a
bout the TeV characteristics of Mkn 421 in 1997 and 1998. We study the ligh
t curve, the shortest time scales of flux variability, the differential spe
ctra on a diurnal basis for several days with good gamma-ray statistics, an
d the time-averaged energy spectrum. Special emphasis is put on presenting
the data taken during the world-wide April 1997 multiwavelength campaign.