{"author":[{"last_name":"Davelaar","full_name":"Davelaar, Jordy","first_name":"Jordy"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","full_name":"Haiman, Zoltán","first_name":"Zoltán"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_created":"2024-09-05T10:07:30Z","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.2112.05829","open_access":"1"}],"day":"09","status":"public","language":[{"iso":"eng"}],"issue":"19","date_published":"2022-05-09T00:00:00Z","article_type":"original","article_number":"191101","citation":{"mla":"Davelaar, Jordy, and Zoltán Haiman. “Self-Lensing Flares from Black Hole Binaries: Observing Black Hole Shadows via Light Curve Tomography.” <i>Physical Review Letters</i>, vol. 128, no. 19, 191101, American Physical Society, 2022, doi:<a href=\"https://doi.org/10.1103/physrevlett.128.191101\">10.1103/physrevlett.128.191101</a>.","ieee":"J. Davelaar and Z. Haiman, “Self-Lensing flares from black hole binaries: Observing black hole shadows via light curve tomography,” <i>Physical Review Letters</i>, vol. 128, no. 19. American Physical Society, 2022.","ista":"Davelaar J, Haiman Z. 2022. Self-Lensing flares from black hole binaries: Observing black hole shadows via light curve tomography. Physical Review Letters. 128(19), 191101.","apa":"Davelaar, J., &#38; Haiman, Z. (2022). Self-Lensing flares from black hole binaries: Observing black hole shadows via light curve tomography. <i>Physical Review Letters</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevlett.128.191101\">https://doi.org/10.1103/physrevlett.128.191101</a>","short":"J. Davelaar, Z. Haiman, Physical Review Letters 128 (2022).","chicago":"Davelaar, Jordy, and Zoltán Haiman. “Self-Lensing Flares from Black Hole Binaries: Observing Black Hole Shadows via Light Curve Tomography.” <i>Physical Review Letters</i>. American Physical Society, 2022. <a href=\"https://doi.org/10.1103/physrevlett.128.191101\">https://doi.org/10.1103/physrevlett.128.191101</a>.","ama":"Davelaar J, Haiman Z. Self-Lensing flares from black hole binaries: Observing black hole shadows via light curve tomography. <i>Physical Review Letters</i>. 2022;128(19). doi:<a href=\"https://doi.org/10.1103/physrevlett.128.191101\">10.1103/physrevlett.128.191101</a>"},"date_updated":"2024-09-18T09:24:54Z","oa_version":"Preprint","type":"journal_article","publisher":"American Physical Society","oa":1,"month":"05","scopus_import":"1","quality_controlled":"1","doi":"10.1103/physrevlett.128.191101","publication_identifier":{"issn":["0031-9007","1079-7114"]},"year":"2022","publication":"Physical Review Letters","intvolume":"       128","publication_status":"published","abstract":[{"text":"Supermassive black hole (BH) binaries are thought to produce self-lensing flares (SLFs) when the two BHs are aligned with the line of sight. If the binary orbit is observed nearly edge-on, we find a distinct feature in the light curve imprinted by the relativistic shadow around the background (“source”) BH. We study this feature by ray tracing in a binary model and predict that 1% of the current binary candidates could show this feature. Our BH tomography method proposed here could make it possible to extract BH shadows that are spatially unresolvable by high-resolution very long base line interferometry (VLBI).","lang":"eng"}],"external_id":{"arxiv":["2112.05829"]},"article_processing_charge":"No","_id":"17547","extern":"1","volume":128,"title":"Self-Lensing flares from black hole binaries: Observing black hole shadows via light curve tomography"}