Multimessenger astronomy with the Einstein Telescope

Gravitational waves (GWs) are expected to play a crucial role in the development of multimessenger astrophysics. The combination of GW observations with other astrophysical triggers, such as from gamma-ray and X-ray satellites, optical/radio telescopes, and neutrino detectors allows us to decipher science that would otherwise be inaccessible. In this paper, we provide a broad review from the multimessenger perspective of the science reach offered by the third generation interferometric GW detectors and by the Einstein Telescope (ET) in particular. We focus on cosmic transients, and base our estimates on the results obtained by ET's predecessors GEO, LIGO, and Virgo.Comment: 26 pages. 3 figures. Special issue of GRG on the Einstein Telescope. Minor corrections include

Astronomical Distance Determination in the Space Age: Secondary Distance Indicators

The formal division of the distance indicators into primary and secondary leads to difficulties in description of methods which can actually be used in two ways: with, and without the support of the other methods for scaling. Thus instead of concentrating on the scaling requirement we concentrate on all methods of distance determination to extragalactic sources which are designated, at least formally, to use for individual sources. Among those, the Supernovae Ia is clearly the leader due to its enormous success in determination of the expansion rate of the Universe. However, new methods are rapidly developing, and there is also a progress in more traditional methods. We give a general overview of the methods but we mostly concentrate on the most recent developments in each field, and future expectations. © 2018, The Author(s)

Teste imunoenzimático com base em anticorpo monoclonal para a detecção de anticorpos contra os herpesvírus bovino tipos 1 e 5

Os herpesvírus bovino tipos 1 (BoHV-1) e 5 (BoHV-5) são agentes virais genética e antigenicamente relacionados, associados com diversas manifestações clínicas em bovinos, incluindo doença respiratória, genital, neurológica e abortos. Estudos epidemiológicos indicam que esses vírus estão amplamente disseminados no rebanho bovino brasileiro. O diagnóstico sorológico, que permite identificar animais portadores da infecção latente, se constitui em importante ferramenta para monitoramento individual e de rebanho. O presente artigo relata a padronização de um teste imunoenzimático do tipo ELISA, com base em anticorpo monoclonal (AcM), para a detecção de anticorpos séricos que reagem contra BoHV-1 e/ou BoHV-5. Inicialmente, determinou-se o AcM mais adequado para a sensibilização das placas, as diluições apropriadas do antígeno e dos soros-teste e o ponto de corte do ensaio. Após a padronização, o ensaio foi validado testando-se 506 amostras de soro bovino, previamente testadas para anticorpos neutralizantes contra BoHV-1 e/ou BoHV-5 pela técnica de soroneutralização (SN). Comparando-se com os resultados da SN frente a BoHV-1, o teste de ELISA apresentou sensibilidade e especificidade de 96,6% e 98,3%, respectivamente. Os valores preditivos positivo e negativo foram de 97,6%, a concordância foi de 97,6% e o índice de correlação kappa entre os testes foi de 0,95, o que indica uma excelente concordância. Comparando-se com os resultados da SN frente o BoHV-5, o ELISA apresentou 94,3% de sensibilidade; 97,9% de especificidade; 97,1% de valor preditivo positivo e 95,9% de valor preditivo negativo. Para BoHV-5, a concordância entre os testes foi de 96,4% e o índice de correlação foi de 0,92, também excelente. Esses resultados demonstram que o teste padronizado apresenta sensibilidade e especificidade adequados para o diagnóstico sorológico das infecções por BoHV-1 e BoHV-5 em nível individual e de rebanho. Dessa forma, o ensaio pode se constituir em alternativa para o teste de SN e para os kits de ELISA importados.Bovine herpesviruses 1 (BoHV-1) and 5 (BoHV-5) are antigenic and genetically related viruses associated with different clinical syndromes in cattle, including respiratory, reproductive, neurological disease and abortion. Epidemiological studies indicate the widespread distribution of both viruses among Brazilian cattle. Serological diagnosis, that allows the identification of latently infected animals, represents an important tool for individual and herd monitoring. The present article describes the standardization of a monoclonal antibody (MAb)-based immunoenzymatic test (ELISA) for detection of antibodies to BoHV-1 and/or BoHV-5. The initial steps involved the determination of the most suitable MAb, the appropriate dilutions of viral antigen and serum samples, and the cut-off value of the assay. After standardization, the ELISA was validated by testing 506 cattle serum samples previously tested for neutralizing antibodies to BoHV-1 and BoHV-5 by virus neutralizing assay (VN). Comparing to the VN for BoHV-1 antibodies, the ELISA presented sensitivity and specificity of 96.6% and 98.3%, respectively. Positive and negative predictive values were 97.6%, the concordance between the tests was 97.6% and the coefficient of correlation k (kappa) was 0.95, demonstrating an excellent correlation. Comparing to the VN for BoHV-5 antibodies, the ELISA presented 94.3% of sensitivity, 97.9% of specificity, 97.1% of positive predictive value, 95.9% negative predictive value, concordance of 96.4% and kappa coefficient of 0.92. These results demonstrate that the ELISA presents suitable specificity and sensitivity to be used for individual and herd serological diagnosis of BoHV-1 and BoHV-5, thus, representing an alternative for VN assays and imported ELISA kits

Science with the space-based interferometer eLISA. III: probing the expansion of the universe using gravitational wave standard sirens

We investigate the capability of various configurations of the space interferometer eLISA to probe the late-time background expansion of the universe using gravitational wave standard sirens. We simulate catalogues of standard sirens composed by massive black hole binaries whose gravitational radiation is detectable by eLISA, and which are likely to produce an electromagnetic counterpart observable by future surveys. The main issue for the identification of a counterpart resides in the capability of obtaining an accurate enough sky localisation with eLISA. This seriously challenges the capability of four-link (2 arm) configurations to successfully constrain the cosmological parameters. Conversely, six-link (3 arm) configurations have the potential to provide a test of the expansion of the universe up to z similar to 8 which is complementary to other cosmological probes based on electromagnetic observations only. In particular, in the most favourable scenarios, they can provide a significant constraint on Ho at the level of 0.5%. Furthermore, (Omega(M), Omega(A)) can be constrained to a level competitive with present SNIa results. On the other hand, the lack of massive black hole binary standard sirens at low redshift allows to constrain dark energy only at the level of few percent