Abstract
A four-year database (spring 1984 through spring 1987) of observations of Hercules X-1 by the Whipple Observatory Collaboration is being analyzed as a whole for evidence of TeV γ-ray emission. The full distribution of Rayleigh powers near the x-ray pulsar frequency differs significantly from the background distribution, giving evidence for sporadic emission at better than a 99% confidence level.
| Original language | English |
|---|---|
| Pages (from-to) | 200-204 |
| Number of pages | 5 |
| Journal | Nuclear Physics B - Proceedings Supplements |
| Volume | 14 |
| Issue number | 1 |
| DOIs | |
| State | Published - Mar 1990 |