Cloning and DNA sequence of the 5'-exonuclease gene of bacteriophage T5

AbstractThe nucleotide sequence of the BalI-PstI fragment of T5 DNA, 1347 bp in length, coding for 5'-exonuclease (D15 gene), has been determined. A coding region of the gene contains 873 bp and is preceded by a typical Shine-Dalgarno sequence. The D15 gene belongs to a cluster, consisting of at least 3 genes, in which a termination codon of a preceding gene overlaps an initiation codon of the following one. The sequence contains an open reading frame for 291 amino acid residues. The molecular mass of the 5'-exonuclease calculated from the predicted amino acid sequence is 33400 Da

Construction status and prospects of the Hyper-Kamiokande project

The Hyper-Kamiokande project is a 258-kton Water Cherenkov together with a 1.3-MW high-intensity neutrino beam from the Japan Proton Accelerator Research Complex (J-PARC). The inner detector with 186-kton fiducial volume is viewed by 20-inch photomultiplier tubes (PMTs) and multi-PMT modules, and thereby provides state-of-the-art of Cherenkov ring reconstruction with thresholds in the range of few MeVs. The project is expected to lead to precision neutrino oscillation studies, especially neutrino CP violation, nucleon decay searches, and low energy neutrino astronomy. In 2020, the project was officially approved and construction of the far detector was started at Kamioka. In 2021, the excavation of the access tunnel and initial mass production of the newly developed 20-inch PMTs was also started. In this paper, we present a basic overview of the project and the latest updates on the construction status of the project, which is expected to commence operation in 2027

Prospects for neutrino astrophysics with Hyper-Kamiokande

Hyper-Kamiokande is a multi-purpose next generation neutrino experiment. The detector is a two-layered cylindrical shape ultra-pure water tank, with its height of 64 m and diameter of 71 m. The inner detector will be surrounded by tens of thousands of twenty-inch photosensors and multi-PMT modules to detect water Cherenkov radiation due to the charged particles and provide our fiducial volume of 188 kt. This detection technique is established by Kamiokande and Super-Kamiokande. As the successor of these experiments, Hyper-K will be located deep underground, 600 m below Mt. Tochibora at Kamioka in Japan to reduce cosmic-ray backgrounds. Besides our physics program with accelerator neutrino, atmospheric neutrino and proton decay, neutrino astrophysics is an important research topic for Hyper-K. With its fruitful physics research programs, Hyper-K will play a critical role in the next neutrino physics frontier. It will also provide important information via astrophysical neutrino measurements, i.e., solar neutrino, supernova burst neutrinos and supernova relic neutrino. Here, we will discuss the physics potential of Hyper-K neutrino astrophysics

Uvulopalatoplasty with a severe form of obstructive sleep apnea: Long-term results

Objective. To assess the severity of daytime sleepiness and the level of sleep apnea/hypopnea index (AHI), as well as the possibility of their correction, in the long-term period after uvulopalatoplasty (UPP) in patients suffering from obesity and obstructive sleep apnea syndrome (OSAS). Material and methods. We retrospectively analyzed the data of the patients, who requested a consultation due to nighttime snor-ing, witnessed sleep apneas and daytime drowsiness. We included men and women of ages 40 to 65 (24 male, 17 female) without cardiac or lung insufficiency. Group 1 consisted of 19 patients, who underwent UPP 3-5 years prior to current consultation. Group 2 consisted of 22 patients, who underwent UPP 6-12 earlier, despite prior diagnosis of severe OSAS. We performed car-diorespiratory sleep monitoring, additionally patients completed the Epworth scale and sleep quality scale. Patients were re-inter-viewed 2 months after initiation of CPAP therapy and or intraoral device treatment. Results. Group 1 (n=19) displayed obesity (Body Mass Index 34.2±6.1 kg/m2), severe OSAS (AHI 55.2±18.5), high level of daytime drowsiness (Epworth score 18.7±6.3) and low sleep quality (13.0±6.8 sleep quality score). Group 2 (n=22) displayed reduction in AHI level — significant statistically, but not clinically without changes in daytime drowsiness and sleep quality, which were improved in 29 cases out of 41 with the help of CPAP-therapy (18 cases) or intraoral fixation devices (11 cases). Conclusion. UPP does not exert a clinically significant affect the severity of sleep disturbance in patients with obesity and severe OSAS. Night sleep study is essential before making a decision about UPP. Clinical state correction of patients in the long-term period of UPP is possible with the help of CPAP therapy or intraoral fixation devices. © 2021, Media Sphera Publishing Group. All rights reserved

Baikal-GVD: cascades

Baikal-GVD is a next generation, kilometer-scale neutrino telescope currently under construction in Lake Baikal. GVD is formed by multi-megaton subarrays (clusters) and is designed for the detection of astrophysical neutrino fluxes at energies from a few TeV up to 100 PeV. The design of Baikal-GVD allows one to search for astrophysical neutrinos with flux values measured by IceCube already at early phases of the array construction. We present here preliminary results of the search for high-energy neutrinos via the cascade mode obtained in 2015 and 2016