STACEE Observations of Mrk 421 During the 2001 Flare
| dc.creator | STACEE Collaboration | |
| dc.creator | Boone, L. M. | |
| dc.creator | Bramel, D. | |
| dc.creator | Chae, E. | |
| dc.creator | Covault, C. E. | |
| dc.creator | Fortin, P. | |
| dc.creator | Gingrich, D. M. | |
| dc.creator | Hanna, D. S. | |
| dc.creator | Hinton, J. A. | |
| dc.creator | Mukherjee, R. | |
| dc.creator | Mueller, C. | |
| dc.creator | Ong, R. A. | |
| dc.creator | Ragan, K. | |
| dc.creator | Scalzo, R. A. | |
| dc.creator | Schuette, D. R. | |
| dc.creator | Theoret, C. G. | |
| dc.creator | Williams, D. A. | |
| dc.date | 2003-01-17 | |
| dc.date.accessioned | 2026-07-07T02:07:15Z | |
| dc.date.available | 2026-07-07T02:07:15Z | |
| dc.description | STACEE is a ground based gamma-ray observatory that uses a heliostat array, built for solar energy research, to detect atmospheric Cherenkov radiation from gamma-ray initiated extensive air showers. During the first half of 2001, a prototype detector, STACEE-48, was used to detect the blazar Markarian 421, which was in an extremely active state. Observations from March to May of 2001 yielded an integral flux of (8.0+/-0.7_{stat}+/-1.5_{sys})x 10^-10 1/cm^2/s at energies above 140+/-20 GeV, and provide some evidence of correlated trends on time scales of a week or more in the GeV and X-ray bands. | |
| dc.description | 6 pages, 6 figures. To appear in proceedings "The Universe Viewed in Gamma-rays", Kashiwa, Japan 2002 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0301369 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0301369 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5636 | |
| dc.subject | Astrophysics | |
| dc.title | STACEE Observations of Mrk 421 During the 2001 Flare | |
| dc.type | text |