Is Campylobacter fetus subspecies venerealis infection a cause of reproductive failure in dairy cows in Iran?

Summary Bovine genital campylobacteriosis is one of the most economically important diseases of dairy cattle resulting in lowered fertility, embryo mortality and abortion, repeated returns to service, reduced pregnancy rates and extended calving intervals. While the occurrence of repeat breeding syndrome and abortions are reported from many Iranian dairy cattle farms, little information is available regarding the presence of bovine genital campylobacteriosis in Iran. The present report describes detection of Campylobacter fetus subsp. venerealis infection in two out of eight repeat breeder Holstein Friesian cows (Bos Taurus) using a PCR method in a herd with a history of subfertility in Mashhad, in the northeast of Iran

Is Campylobacter fetus subspecies venerealis infection a cause of reproductive failure in dairy cows in Iran?

Summary Bovine genital campylobacteriosis is one of the most economically important diseases of dairy cattle resulting in lowered fertility, embryo mortality and abortion, repeated returns to service, reduced pregnancy rates and extended calving intervals. While the occurrence of repeat breeding syndrome and abortions are reported from many Iranian dairy cattle farms, little information is available regarding the presence of bovine genital campylobacteriosis in Iran. The present report describes detection of Campylobacter fetus subsp. venerealis infection in two out of eight repeat breeder Holstein Friesian cows (Bos Taurus) using a PCR method in a herd with a history of subfertility in Mashhad, in the northeast of Iran

Probing quantum gravity using photons from a flare of the active galactic nucleus Markarian 501 observed by the MAGIC telescope

We analyze the timing of photons observed by the MAGIC telescope during a flare of the active galactic nucleus Mkn 501 for a possible correlation with energy, as suggested by some models of quantum gravity (QG), which predict a vacuum refractive index similar or equal to 1 + (E/M-QGn)(n), n = 1, 2. Parametrizing the delay between gamma-rays of different energies as Delta t = +/-tau E-1 or Delta t = +/-tau E-q(2), we find tau(1) = (0.030 +/- 0.012) s/GeV at the 2.5-sigma level, and tau(q) = (3.71 +/- 2.57) x 10(-6) s/GeV2, respectively. We use these results to establish lower limits M-QG1 > 0.21 X 10(18) GeV and M-QG2 > 0.26 x 10(11) GeV at the 95% C.L. Monte Carlo studies confirm the MAGIC sensitivity to propagation effects at these levels. Thermal plasma effects in the source are negligible, but we cannot exclude the importance of some other source effect

Observation of VHE γ-rays from Cassiopeia A with the MAGIC telescope

Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A Methods: The shell-type supernova remnant Cassiopeia A was observed with the 17 m MAGIC telescope between July 2006 and January 2007 for a total time of 47 h. Results: The source was detected above an energy of 250 GeV with a significance of 5.2σ and a photon flux above 1 TeV of (7.3 ± 0.7_stat ± 2.2_sys) × 10-13 cm-2s-1. The photon spectrum is compatible with a power law dN/dE ∝ E-Γ with a photon index Γ = 2.3 ± 0.2_stat ± 0.2_sys. The source is point-like within the angular resolution of the telescope