Gupta, Ish, Chandra, Koustav, and Sathyaprakash, B S. Foreground signals minimally affect inference of high-mass binary black holes in next-generation gravitational-wave detectors. Retrieved from https://par.nsf.gov/biblio/10591500. Physical Review D 111.10 Web. doi:10.1103/PhysRevD.111.104013.

Gupta, Ish, Chandra, Koustav, & Sathyaprakash, B S. Foreground signals minimally affect inference of high-mass binary black holes in next-generation gravitational-wave detectors. Physical Review D, 111 (10). Retrieved from https://par.nsf.gov/biblio/10591500. https://doi.org/10.1103/PhysRevD.111.104013

Gupta, Ish, Chandra, Koustav, and Sathyaprakash, B S. "Foreground signals minimally affect inference of high-mass binary black holes in next-generation gravitational-wave detectors". Physical Review D 111 (10). Country unknown/Code not available: American Physical Society. https://doi.org/10.1103/PhysRevD.111.104013. https://par.nsf.gov/biblio/10591500.

@article{osti_10591500,
place = {Country unknown/Code not available}, title = {Foreground signals minimally affect inference of high-mass binary black holes in next-generation gravitational-wave detectors}, url = {https://par.nsf.gov/biblio/10591500}, DOI = {10.1103/PhysRevD.111.104013}, abstractNote = {}, journal = {Physical Review D}, volume = {111}, number = {10}, publisher = {American Physical Society}, author = {Gupta, Ish and Chandra, Koustav and Sathyaprakash, B S}, }