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We present the first search for gravitational waves from the coalescence of stellar mass and sub-solar mass black holes with masses between $20 - 100~\mathrm{M}_{\odot}$ and $0.01 - 1~\mathrm{M}_{\odot}~($10 - 10^3$~\mathrm{M}_{J})$, respectively.
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Hideaki Mouri and Yoshiaki Taniguchi, “Runaway merging of black holes: analytical constraint on the timescale,” Astrophys. J. Lett. 566
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T. Ertl, H.-Th. Janka, S. E. Woosley, T. Sukhbold, and M. Ugliano, “A TWO-PARAMETER CRITERION FOR CLASSIFYING THE EXPLODABILITY OF MASSIVE STARS BY THE NEUTRINO-DRIVEN MECHANISM,” The Astrophysical Journal 818
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Bruce Allen, “A chi**2 time-frequency discriminator for gravitational wave detection,” Phys. Rev. D 71
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S. E. Woosley, “Pulsational Pair-Instability Supernovae,” Astrophys. J. 836
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Takeshi Chiba and Shuichiro Yokoyama, “Spin Distribution of Primordial Black Holes,” PTEP 2017
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Pablo Marchant, Mathieu Renzo, Robert Farmer, Kaliroe M. W. Pappas, Ronald E. Taam, Selma E. de Mink, and Vassiliki Kalogera, “Pulsational pair-instability supernovae in very close binaries,” Astrophys. J. 882
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