Table 9.
Expected number of joint GW+X-ray detections in pointing mode.
ET | ET+CE | ET+2CE | |
---|---|---|---|
Einstein Probe |
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THESEUS-SXI/ |
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Gamow | |||
TAP-WFI |
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Notes. The numbers are relative to one year of observations, for different X-ray instruments operating in pointing mode. We consider BNS mergers with sky-localization uncertainty ΔΩ < 100 deg2 and with a detectable X-ray emission, assuming a tresp = 100 s. The assumed structure is Stru1 and the FS configuration is FS-SGRB.
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