Overview of Cattle Diseases Listed Under Category C, D or E in the Animal Health Law for Which Control Programmes Are in Place Within Europe

The COST action “Standardising output-based surveillance to control non-regulated diseases of cattle in the European Union (SOUND control),” aims to harmonise the results of surveillance and control programmes (CPs) for non-EU regulated cattle diseases to facilitate safe trade and improve overall control of cattle infectious diseases. In this paper we aimed to provide an overview on the diversity of control for these diseases in Europe. A non-EU regulated cattle disease was defined as an infectious disease of cattle with no or limited control at EU level, which is not included in the European Union Animal health law Categories A or B under Commission Implementing Regulation (EU) 2020/2002. A CP was defined as surveillance and/or intervention strategies designed to lower the incidence, prevalence, mortality or prove freedom from a specific disease in a region or country. Passive surveillance, and active surveillance of breeding bulls under Council Directive 88/407/EEC were not considered as CPs. A questionnaire was designed to obtain country-specific information about CPs for each disease. Animal health experts from 33 European countries completed the questionnaire. Overall, there are 23 diseases for which a CP exists in one or more of the countries studied. The diseases for which CPs exist in the highest number of countries are enzootic bovine leukosis, bluetongue, infectious bovine rhinotracheitis, bovine viral diarrhoea and anthrax (CPs reported by between 16 and 31 countries). Every participating country has on average, 6 CPs (min–max: 1–13) in place. Most programmes are implemented at a national level (86%) and are applied to both dairy and non-dairy cattle (75%). Approximately one-third of the CPs are voluntary, and the funding structure is divided between government and private resources. Countries that have eradicated diseases like enzootic bovine leukosis, bluetongue, infectious bovine rhinotracheitis and bovine viral diarrhoea have implemented CPs for other diseases to further improve the health status of cattle in their country. The control of non-EU regulated cattle diseases is very heterogenous in Europe. Therefore, the standardising of the outputs of these programmes to enable comparison represents a challenge. © Copyright © 2021 Hodnik, Acinger-Rogić, Alishani, Autio, Balseiro, Berezowski, Carmo, Chaligiannis, Conrady, Costa, Cvetkovikj, Davidov, Dispas, Djadjovski, Duarte, Faverjon, Fourichon, Frössling, Gerilovych, Gethmann, Gomes, Graham, Guelbenzu, Gunn, Henry, Hopp, Houe, Irimia, Ježek, Juste, Kalaitzakis, Kaler, Kaplan, Kostoulas, Kovalenko, Kneževič, Knific, Koleci, Madouasse, Malakauskas, Mandelik, Meletis, Mincu, Mõtus, Muñoz-Gómez, Niculae, Nikitović, Ocepek, Tangen-Opsal, Ózsvári, Papadopoulos, Papadopoulos, Pelkonen, Polak, Pozzato, Rapaliuté, Ribbens, Niza-Ribeiro, Roch, Rosenbaum Nielsen, Saez, Nielsen, van Schaik, Schwan, Sekovska, Starič, Strain, Šatran, Šerić-Haračić, Tamminen, Thulke, Toplak, Tuunainen, Verner, Vilček, Yildiz and Santman-Berends

Corrigendum: Overview of Cattle Diseases Listed Under Category C, D or E in the Animal Health Law for Which Control Programmes Are in Place Within Europe (Front. Vet. Sci., (2021), 8, (688078), 10.3389/fvets.2021.688078)

In the original article, there was an error. We used the phrase “non-regulated” for cattle diseases that are in fact listed in the New Animal Health Law that went into force in 2021. A correction has beenmade toAbstract. The corrected section is shown below. Copyright © 2022, Hodnik, Acinger-Rogić, Alishani, Autio, Balseiro, Berezowski, Carmo, Chaligiannis, Conrady, Costa, Cvetkovikj, Davidov, Dispas, Djadjovski, Duarte, Faverjon, Fourichon, Frössling, Gerilovych, Gethmann, Gomes, Graham, Guelbenzu, Gunn, Henry, Hopp, Houe, Irimia, Ježek, Juste, Kalaitzakis, Kaler, Kaplan, Kostoulas, Kovalenko, Kneževič, Knific, Koleci, Madouasse, Malakauskas, Mandelik, Meletis, Mincu, Mõtus, Muñoz-Gómez, Niculae, Nikitović, Ocepek, Tangen-Opsal, Ózsvári, Papadopoulos, Papadopoulos, Pelkonen, Polak, Pozzato, Rapaliuté, Ribbens, Niza-Ribeiro, Roch, Rosenbaum Nielsen, Saez, Nielsen, van Schaik, Schwan, Sekovska, Starič, Strain, Šatran, Šerić-Haračić, Tamminen, Thulke, Toplak, Tuunainen, Verner, Vilček, Yildiz and Santman-Berends

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta