Foreground signals minimally affect inference of high-mass binary black holes in next-generation gravitational-wave detectors American Physical Society 05/01/2025 10591500 10.1103/PhysRevD.111.104013 Physical Review D 2470-0010 111 10 Ish GuptaKoustav ChandraB S Sathyaprakash

❳◗❱❀❄ (❭(❱❀❍(❣ ❄❀▲❂❃❀❄ •▲❞❍ ❱)❀ ⑤❲✟❆▼❰✟◆ ◗❝❄ ⑤❲✟❰▼❆❅✟ |❞(❱❀▲❂❞▲( ◗( ❞❏❱◗❂❝❀❄ ❏❭ ✞(❳◗❍ ✦✤ ✪✵❛ ❬◆❰✍❦ ◗▲◗❍❀❱❀▲ ✭❭❍❏❞❳ ⑤❲✟❆▼❰✟◆ ⑤❲✟❰▼❆❅✟ ❬◗(( ▲◗❱❂❞ q ▼❦❰✽ ▼❦❰❆ ✭❞♣▲❁❀❴•▲◗❍❀ ❱❞❱◗❳ ❍◗(( ✡✚ ✛ ☛ ✚ ❚ ✻✌❦▼❆ ❅✟▼❦❆✟ ▲❂❍◗▲❭ (|❂❝ ❍◗❵❝❂❱♣❄❀ ✜ ✢ ▼❦❆✽ ▼❦✽✌ ✭❀❁❞❝❄◗▲❭ (|❂❝ ❍◗❵❝❂❱♣❄❀ ✜ ✷ ▼❦◆✌ ▼❦❰✻ ▲❂❍◗▲❭ ❱❂❳❱ ✾▲◗❄( ✣ ✢ ❅❦◆❰ ✟❦❆✻ ✭❀❁❞❝❄◗▲❭ ❱❂❳❱ ✾▲◗❄( ✣ ✷ ▼❦❮✽ ✟❦❰✻ ❲✐❂❍♣❱)◗❳ ❂❝❱❀▲(|❂❝ ◗❝❵❳❀ ✾▲◗❄( ✤ ✢✷ ✌❦❰✽ ▼❦❅✌ ❲✐❂❍♣❱)◗❳ |▲❀❁❀((❂❞❝ ❁❞❝❀ ◗❝❵❳❀ ✾▲◗❄( ✤ ✥✦ ▼❦▼✻ ▼❦✌✻ ❊••❀❁❱❂❃❀ ◗❳❂❵❝❀❄ (|❂❝ ✜ ✧★★ ✩✵❦✵✪ ▼❦✟❰ ❊••❀❁❱❂❃❀ |▲❀❁❀((❂❝❵ (|❂❝ ✜ ♣ ▼❦✌❆ ▼❦✽✌ ❲✐❂❍♣❱) ✾▲◗❄( ✤ ❅❦❅▼ ✟❦▼✻ ❞❳◗▲❂✐◗❱❂❞❝ ◗❝❵❳❀ ✾▲◗❄( ✫ ▼❦✻✽ ✟❦❅❮ ✿❂❵)❱ ◗(❁❀❝(❂❞❝ ✾▲◗❄( ✬ ❅❦✟✻ ◆❦✌❰ ❊❀❁❳❂❝◗❱❂❞❝ ✾▲◗❄( ✭ ✩✮❦✯✰ ▼❦✽❆ ✞❝❁❳❂❝◗❱❂❞❝ ◗❝❵❳❀ ✾▲◗❄( ✣ ✥✱ ❅❦❆❆ ❅❦▼❰