Aims We describe a novel, practical, and inexpensive method to add video recording during tilt table testing (TTT): Open-Access-Video-TTT. Methods and results The Open-Access-Video-TTT set-up uses... Show moreAims We describe a novel, practical, and inexpensive method to add video recording during tilt table testing (TTT): Open-Access-Video-TTT. Methods and results The Open-Access-Video-TTT set-up uses a personal computer (PC) to capture screen video data from a non-invasive-beat-to-beat (NIBTB) haemodynamic blood pressure (BP) device, combined with video recording of a patient, using Open Broadcaster Software (OBS (R)). The new Open-Access-Video-TTT set up was tested with both the Finometer (model Finapres Nova (R), Medical Systems, the Netherlands) and the Task Force (R) Touch Cardio monitor (CNSystems, Austria). For this, the Finapres Nova (R) was enabled in 'remote' mode and Real Video Network Computing (RealVNC (R)) was installed on the PC/laptop. The Task Force (R) has a DisplayPort (DP) port, for which a DP/ high-definition multimedia interface (HDMI) cable and a video capture card is used to merge the signals to the PC/laptop. With this method the combined images are stored as a new video signal. TTT can be performed with any routine protocol. Conclusions Open Access-Video-TTT worked well for both the Finapres NOVA (R) and the Task Force Monitor (R). This novel method can be used easily by all physicians who wish to add video recording during TTT who do not have access to an electroencephalogram machine. Show less
Bischetti, M.; Feruglio, C.; D'Odorico, V.; Arav, N.; Banados, E.; Becker, G.; ... ; Fiore, F. 2022
Bright quasars, powered by accretion onto billion-solar-mass black holes, already existed at the epoch of reionization, when the Universe was 0.5-1 billion years old(1). How these black holes... Show moreBright quasars, powered by accretion onto billion-solar-mass black holes, already existed at the epoch of reionization, when the Universe was 0.5-1 billion years old(1). How these black holes formed in such a short time isthe subject of debate, particularly asthey lie above the correlation between black-hole mass and galaxy dynamical mass(2,3) in the local Universe. What slowed down black-hole growth, leading towards the symbioticgrowth observed in the local Universe, and when this process started, has hitherto not been known, although black-hole feedback is a likely driver(4). Here we report optical and near-infrared observations of a sample of quasars at redshifts 5.8 less than or similar to z less than or similar to 6.6. About half ofthe quasar spectra reveal broad, blueshifted absorption line troughs, tracing black-hole-driven winds with extreme outflowvelocities, up to 17% of the speed of light. The fraction of quasars with such outflow winds at z greater than or similar to 5.8 approximate to 2.4 is times higher than at z approximate to 2-4. We infer that outflows at z greater than or similar to 5.8 inject large amounts of energy into the interstellar medium and suppress nuclear gas accretion, slowing down black-hole growth. The outflow phase may then mark the beginning of substantial black-hole feedback. The red optical colours of outflow quasars at z greater than or similar to 5.8 indeed suggest that these systems are dusty and may be caught during an initial quenching phase of obscured accretion(5). Show less
Ferrara, A.; Sommovigo, L.; Dayal, P.; Pallottini, A.; Bouwens, R.J.; Gonzalez, V.; ... ; Werf, P.P. van der 2022
