Search for tev emissions from pulsars in binary systems
View/ Open
Full Text
Date
2003-02-01Author
Hall, T. A.
Bond, I. H.
Bradbury, S. M.
Buckley, J. H.
Carson, M. J.
Carter‐Lewis, D. A.
Catanese, M.
Dunlea, S.
D’Vali, M.
Fegan, D. J.
Fegan, S. J.
Finley, J. P.
Gaidos, J. A.
Gillanders, G. H.
Hillas, A. M.
Horan, D.
Kertzman, M.
Kieda, D.
Kildea, J.
Knapp, J.
Krennrich, F.
Lang, M. J.
LeBohec, S.
Lessard, R.
Lloyd‐Evans, J.
McKernan, B.
Moriarty, P.
Muller, D.
Ong, R.
Quinn, J.
Reynolds, P. T.
Rose, H. J.
Sembroski, G. H.
Swordy, S. P.
Vassiliev, V. V.
Weekes, T. C.
Metadata
Show full item recordUsage
This item's downloads: 0 (view details)
Cited 19 times in Scopus (view citations)
Recommended Citation
Hall, T. A. Bond, I. H.; Bradbury, S. M.; Buckley, J. H.; Carson, M. J.; Carter‐Lewis, D. A.; Catanese, M.; Dunlea, S.; D’Vali, M.; Fegan, D. J.; Fegan, S. J.; Finley, J. P.; Gaidos, J. A.; Gillanders, G. H.; Hillas, A. M.; Horan, D.; Kertzman, M.; Kieda, D.; Kildea, J.; Knapp, J.; Krennrich, F.; Lang, M. J.; LeBohec, S.; Lessard, R.; Lloyd‐Evans, J.; McKernan, B.; Moriarty, P.; Muller, D.; Ong, R.; Quinn, J.; Reynolds, P. T.; Rose, H. J.; Sembroski, G. H.; Swordy, S. P.; Vassiliev, V. V.; Weekes, T. C. (2003). Search for tev emissions from pulsars in binary systems. The Astrophysical Journal 583 (2), 853-860
Published Version
Abstract
A survey of binary systems containing pulsars was conducted, with the intention of detecting Galactic sources of very high energy gamma-ray emission. Observations were carried out with the Whipple 10 m imaging atmospheric Cerenkov telescope. Standard analysis techniques were applied to these sources to search for steady, unpulsed emission. Periodic tests were also performed to search for emission correlated with both the orbital and spin phases, where appropriate. Analyses indicate that the binaries in this study do not emit detectable levels of very high energy photons within the sensitivity of our instrument. The flux upper limits presented here fail to seriously constrain emission models.