There is a typo in equation (8) of Patricelli et al. (2022). The isotropic-equi v alent luminosity observed at a viewing angle θj is (Salafia et al. 2015, 2019): (Equation Presented). where the relativistic Doppler factor δ appears to the power of three. This modification does not affect any of the results presented in Patricelli et al. (2022), that were obtained using the correct formula (equation 1) and not the one written in equation (8) of Patricelli et al. (2022). ACKNOWLEDGEMENT We thank Om Sharan Salafia for pointing out the typo in our manuscript.
Patricelli B., Bernardini M.G., Mapelli M., D'Avanzo P., Santoliquido F., Cella G., et al. (2022). Erratum: Prospects for multimessenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run (Monthly Notices of the Royal Astronomical Society (2022) 513 (4159) DOI: 10.1093/mnras/stac1167). MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 514(3), 3395-3395 [10.1093/mnras/stac1668].
Erratum: Prospects for multimessenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run (Monthly Notices of the Royal Astronomical Society (2022) 513 (4159) DOI: 10.1093/mnras/stac1167)
Cuoco E.
2022
Abstract
There is a typo in equation (8) of Patricelli et al. (2022). The isotropic-equi v alent luminosity observed at a viewing angle θj is (Salafia et al. 2015, 2019): (Equation Presented). where the relativistic Doppler factor δ appears to the power of three. This modification does not affect any of the results presented in Patricelli et al. (2022), that were obtained using the correct formula (equation 1) and not the one written in equation (8) of Patricelli et al. (2022). ACKNOWLEDGEMENT We thank Om Sharan Salafia for pointing out the typo in our manuscript.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
