Gravitational waves, predicted by Einstein's general theory of relativity, have now been observed by the LIGO and Virgo detectors, heralding an exciting new era of multimessenger astrophysics. IAU S338 explores how space-time and electromagnetic messengers can be correlated, to help us understand many high-energy astrophysical phenomena.
Gravitational waves, predicted by Einstein's general theory of relativity, have now been observed by the LIGO and Virgo detectors, heralding an exciting new era of multimessenger astrophysics. IAU S338 explores how space-time and electromagnetic messengers can be correlated, to help us understand many high-energy astrophysical phenomena.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Produktdetails
Produktdetails
Proceedings of the International Astronomical Union Symposia and Colloquia
1. Revealing short GRB jet structure and dynamics with gravitational wave electromagnetic counterparts Gavin Lamb; 2. Gravitational wave optical counterpart searching based on GRAWITA and DLT40 project during LIGO O2 run Sheng Yang; 3. On the host galaxy properties of stellar binary black hole mergers Youjun Lu; 4. Reanalysis of LIGO black-hole coalescences with alternative prior assumptions Davide Gerosa; 5. High accuracy measurement of gravitational wave back-reaction in the OJ287 black hole binary Mauri Valtonen; 6. Background rejection using convolutional neural networks Adam Zadröny; 7. Merging massive black holes: the right place and the right time Astrid Lamberts; 8. Supermassive black hole binary candidates from the Pan-STARRS1 medium deep survey Tingting Liu; 9. GW170817: swift UV detection of a blue kilonova, and improving the search in O3 Aaron Tohuvavohu; 10. DESGW optical follow-up of BBH LIGO-Virgo events with DECam Robert Butler; 11. Cosmology with gravitational waves in DES and LSST Ken Herner; 12. Observations of GW170817 by DESGW and the DECam GW-EM collaboration James Annis; 13. Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration Lucas Macri; 14. AGILE observations of GW events Francesco Verrecchia; 15. High power in advanced LIGO Terra Hardwick; 16. Strong-lensing of gravitational waves by galaxy clusters Graham Smith; 17. How Einstein's theory of relativity gives us E = mc2 and the atomic bomb Richard Henry.
1. Revealing short GRB jet structure and dynamics with gravitational wave electromagnetic counterparts Gavin Lamb; 2. Gravitational wave optical counterpart searching based on GRAWITA and DLT40 project during LIGO O2 run Sheng Yang; 3. On the host galaxy properties of stellar binary black hole mergers Youjun Lu; 4. Reanalysis of LIGO black-hole coalescences with alternative prior assumptions Davide Gerosa; 5. High accuracy measurement of gravitational wave back-reaction in the OJ287 black hole binary Mauri Valtonen; 6. Background rejection using convolutional neural networks Adam Zadröny; 7. Merging massive black holes: the right place and the right time Astrid Lamberts; 8. Supermassive black hole binary candidates from the Pan-STARRS1 medium deep survey Tingting Liu; 9. GW170817: swift UV detection of a blue kilonova, and improving the search in O3 Aaron Tohuvavohu; 10. DESGW optical follow-up of BBH LIGO-Virgo events with DECam Robert Butler; 11. Cosmology with gravitational waves in DES and LSST Ken Herner; 12. Observations of GW170817 by DESGW and the DECam GW-EM collaboration James Annis; 13. Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration Lucas Macri; 14. AGILE observations of GW events Francesco Verrecchia; 15. High power in advanced LIGO Terra Hardwick; 16. Strong-lensing of gravitational waves by galaxy clusters Graham Smith; 17. How Einstein's theory of relativity gives us E = mc2 and the atomic bomb Richard Henry.
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