[PDF] Top 20 A consistent estimate for gravitational wave and electromagnetic transient rates

... Gravitational wave transients, resulting from the merger of two stellar remnants, are now ...and rates of these directly relates to the stellar population which gave rise to their progenitors, and ... See full document

... GW150914, announced in [26]. We describe results reported in this announcement that are based on the coherent Waveburst algorithm, along with those obtained by two other analyses using omicron-LALInference-Bursts and ... See full document

... merger rates are obtained from population- synthesis codes, is O’Shaughnessy et ...impact rates: for example, if kicks are preferentially aligned with pre-supernova spin, NS-NS coalescence rates ... See full document

... In the Omega Pipeline search (Abadie et al. 2010b), triggers are first identified by performing a matched filter search with a bank of basis waveforms which are approximately (co)sine- Gaussians. The search assumes that ... See full document

... signal consistent with the location and time of the radio ...not consistent with the radio signal’s sky location, and only signals within 2 minutes of the radio trigger are ... See full document

... a transient gravitational wave signal is a near-simultaneous signal with consistent waveforms in the two ...representative estimate of the expected rate of background triggers, as ... See full document

... a transient gravitational wave signal is a near-simultaneous signal with consistent waveforms in the two ...representative estimate of the expected rate of background triggers, as ... See full document

... rst gravitational-wave ( GW ) -triggered electromagnetic ( EM ) observations were carried out during the 2009 – 2010 science run of the initial LIGO and Virgo detectors ( Abadie et ...were ... See full document

... candidate gravitational-wave (GW) transient events recorded by LIGO and Virgo in their 2009–2010 science ...Image transient detection was used to analyze the collected electromagnetic ... See full document

... A gravitational-wave ( GW ) transient was identi fi ed in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory ( LIGO ) detectors on 2015 September ... See full document

... A gravitational-wave ( GW ) transient was identi fi ed in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory ( LIGO ) detectors on 2015 September ... See full document

... A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September ...detectable ... See full document

... the wavelengths covered. Fluxes were converted to luminosities using the distance previously adopted. We determined the points on the bolometric light curve at epochs when K-band or ultra- violet observations were ... See full document

... event rates with the chirp mass distribution will provide further con- straints on stellar and cosmic evolution models, although care will be needed to account for the impact of chirp mass on detectability of ... See full document

... and wave properties ...but electromagnetic complex wave configurations and light particles are not like “particles” but separated electromagnetic wave packages, 2-dimensionally confined ... See full document

... sound wave is plane the equation of which is obtained from the generalized equation of gravitational waves on the assumption of a and ideality of the ...acoustic wave is not gravitational is ... See full document

... tromagnetic pulse period. The other method works in the fre- quency domain to cover a relatively small, physically motivated range of frequency and spin-down values. The searches use the known frequency and position of ... See full document

... LEE, T, 1977, Estimat10n of Depth to Conductors by the Use of Electromagnetic Transients, Geophysical Prospectmg 25, 61-75 The transient response of a layered structure to plane wave exc[r] ... See full document

... Pan-STARRS-LIGO effort is in collaboration with the LIGO Consortium and supported by Queen’s University Belfast. The Pan-STARRS1 Sky Surveys have been made possible through contributions by the Institute for Astronomy, ... See full document

... the gravitational force strength (F g (mm)) between the matters is so weak compared with the electromagnetic force strength (F c (mm)) between the ... See full document