YouTube video by SiIvaGunner

Note: This book safe will only fit compact and subcompact handguns 1.1" in width or less. Please check before ordering. Guaranteed to fit the following guns with standard grips and sights:Beretta Pico, Nano, Tomcat, Bobcat Colt Mustang LiteGlock 48, 42, 43 w/ pinky or +2 mags Kahr P380, CW380, CM380, CT380 K380, K9, P9, MK9, PM9, CM9, CW9 Kahr P40, CW40, PM40, K40, MK40, PM40, CM40, CM45, CT45, CW45, P45, PM45 Keltec P-3AT, P-32, P-11, PF-9 Ruger LC830, LC9/s, SR9c, LCP (w/laser)Sig Sauer P238, P938, P239, P290Smith & Wesson Bodyguard 380, M&P ShieldSpringfield XDsTaurus Concealed Carry, Slim, and Small Frame PistolsMany more A hand-crafted real Bible book storage safe. Precision-cut to fit most compact handguns. Made from a brand new ESV Bible. Designed to be a solution to the common gun storage dilemma: You need fast access to your firearm, but want a better place for it rather than the bottom of a drawer or under a mattress. Book safes allow for storage of firearms hidden in plain sight, giving you quick access to your gun. Safety note: This is not designed to be a locking safe for firearms, and there is no locking mechanism. Please follow all applicable laws regarding firearm storage depending on your location. Gun not included.

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YouTube video by SiIvaGunner

We present observational evidence for three massive, accreting black holes in the $z=5.0167$ galaxy J0148-4214 from JWST/NIRSpec-IFU spectroscopy. The black holes are revealed through broad H$α$ emission (FWHM = 430-2920 km/s) without a forbidden-line counterpart in the bright [O III] doublet. Channel maps of the asymmetric central H$α$ profile isolate two spatially distinct broad line regions (BLRs), separated by $190\pm40$ pc, while a third BLR is found in the galaxy outskirts with a projected separation of 1.7 kpc. Using single-epoch virial relations, we estimate black hole masses of $\log(M_\bullet/M_\odot)=7.9\pm0.4$ (primary central), $5.8\pm0.5$ (secondary central) and $6.3\pm0.5$ (third off-nuclear). We argue that the two central black holes will likely rapidly merge, with a simple dynamical friction time estimate of the order of 700 Myr. Assuming that also the off-nuclear black hole is in the process of sinking towards the centre, it will likely lead to a second merger, and we investigate the detection probability of such mergers with LISA. Alternatively, the third black hole may be the result of previous three-body interaction or a gravitational recoil, where our observations would provide evidence that such black holes may retain their accretion discs and BLRs even in the aftermath of such extreme dynamical interactions. The discovery of a black hole triplet at high redshift, together with other recent results on distant black hole pairs, indicates that multiple massive black hole systems were common in the early Universe. Our results highlight the importance of IFU observations for the detection of massive black hole multiplets in distant galaxies, the progenitors of massive black hole mergers that may be detected with next-generation gravitational wave observatories.

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