2003ApJ...583..853H


Query : 2003ApJ...583..853H

2003ApJ...583..853H - Astrophys. J., 583, 853-860 (2003/February-1)

Search for TeV emissions from pulsars in binary systems.

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., LE BOHEC 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. and WEEKES T.C.

Abstract (from CDS):

A survey of binary systems containing pulsars was conducted, with the intention of detecting Galactic sources of very high energy γ-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.

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Journal keyword(s): Gamma Rays: Observations - Stars: Pulsars: General

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 LS I +61 303 HXB 02 40 31.6644419688 +61 13 45.593918580 11.27 11.61 10.75 10.19 9.55 B0Ve 903 2
2 V* V779 Cen HXB 11 21 15.0920532528 -60 37 25.630264596   14.4 12.27     O9III/Veq 1159 0
3 PSR B1257+12 Psr 13 00 03.1075 +12 40 55.155           ~ 546 1
4 CPD-63 2495 HXB 13 02 47.6544015048 -63 50 08.626970292 10.34 10.72 9.98 10.03   O9.5Ve 852 0
5 PSR B1534+11 Psr 15 37 09.9603 +11 55 55.554           ~ 453 1
6 PSR J1641+3627B Psr 16 41 41.0 +36 27 37           ~ 29 1
7 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
8 V* V934 Her LXB 17 06 34.5128222328 +23 58 18.639373836 11.20 9.16 7.62     M3III(e) 165 0
9 PSR J1959+2048 Psr 19 59 36.7643141520 +20 48 14.896407996   21.08 20.16 19.53 18.79 G: 854 3

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