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.
| Original language | English (Ireland) |
|---|---|
| Number of pages | 7 |
| Journal | Astrophysical Journal |
| Volume | 583 |
| Issue number | 2, 1 |
| DOIs | |
| Publication status | Published - 1 Feb 2003 |
Authors (Note for portal: view the doc link for the full list of authors)
- Authors
- Hall, TA and Bond, IH and Bradbury, SM and Buckley, JH and Carson, MJ and Carter-Lewis, DA and Catanese, M and Dunlea, S and D'Vali, M and Fegan, DJ and Fegan, SJ and Finley, JP and Gaidos, JA and Gillanders, GH and Hillas, AM and Horan, D and Kertzman, M and Kieda, D and Kildea, J and Knapp, J and Krennrich, F and Lang, MJ and LeBohec, S and Lessard, R and Lloyd-Evans, J and McKernan, B and Moriarty, P and Muller, D and Ong, R and Quinn, J and Reynolds, PT and Rose, HJ and Sembroski, GH and Swordy, SP and Vassiliev, VV and Weekes, TC
- Hall, TA;Bond, IH;Bradbury, SM;Buckley, JH;Carson, MJ;Carter-Lewis, DA;Catanese, M;Dunlea, S;D'Vali, M;Fegan, DJ;Fegan, SJ;Finley, JP;Gaidos, JA;Gillanders, GH;Hillas, AM;Horan, D;Kertzman, M;Kieda, D;Kildea, J;Knapp, J;Krennrich, F;Lang, MJ;LeBohec, S;Lessard, R;Lloyd-Evans, J;McKernan, B;Moriarty, P;Muller, D;Ong, R;Quinn, J;Reynolds, PT;Rose, HJ;Sembroski, GH;Swordy, SP;Vassiliev, VV;Weekes, TC