Paramyxovirus Sendai virus-like particle formation by expression of multiple viral proteins and acceleration of its release by C protein

AbstractEnvelope viruses maturate by macromolecule assembly and budding. To investigate these steps, we generated virus-like particles (VLPs) by co-expression of structural proteins of Sendai virus (SeV), a prototype of the family Paramyxoviridae. Simultaneous expression of matrix (M), nucleo- (N), fusion (F), and hemagglutinin-neuraminidase (HN) proteins resulted in the generation of VLPs that had morphology and density similar to those of authentic virus particles, although the efficiency of release from cells was significantly lower than that of the virus. By using this VLP formation as a model of virus budding, roles of individual proteins in budding were investigated. The M protein was a driving force of budding, and the F protein facilitated and the HN protein suppressed VLP release. Either of the glycoproteins, F or HN, as well as the N protein, significantly shifted density of VLPs to that of virus particles, suggesting that viral proteins bring about integrity of VLPs by protein–protein interactions. We further found that co-expression of a nonstructural protein, C, but not V, enhanced VLP release to a level comparable to that of virus particles, demonstrating that the C protein plays a role in virus budding

First Data Release of the Hyper Suprime-Cam Subaru Strategic Program

The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most outstanding questions in astronomy today, including the nature of dark matter and dark energy. The survey has been awarded 300 nights of observing time at the Subaru Telescope and it started in March 2014. This paper presents the first public data release of HSC-SSP. This release includes data taken in the first 1.7 years of observations (61.5 nights) and each of the Wide, Deep, and UltraDeep layers covers about 108, 26, and 4 square degrees down to depths of i~26.4, ~26.5, and ~27.0 mag, respectively (5sigma for point sources). All the layers are observed in five broad bands (grizy), and the Deep and UltraDeep layers are observed in narrow bands as well. We achieve an impressive image quality of 0.6 arcsec in the i-band in the Wide layer. We show that we achieve 1-2 per cent PSF photometry (rms) both internally and externally (against Pan-STARRS1), and ~10 mas and 40 mas internal and external astrometric accuracy, respectively. Both the calibrated images and catalogs are made available to the community through dedicated user interfaces and database servers. In addition to the pipeline products, we also provide value-added products such as photometric redshifts and a collection of public spectroscopic redshifts. Detailed descriptions of all the data can be found online. The data release website is https://hsc-release.mtk.nao.ac.jp/.Comment: 34 pages, 20 figures, 7 tables, moderate revision, accepted for publication in PAS

The Hyper Suprime-Cam SSP survey: Overview and survey design

Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2-m Subaru telescope on the summit of Mauna Kea in Hawaii. A team of scientists from Japan, Taiwan, and Princeton University is using HSC to carry out a 300-night multi-band imaging survey of the high-latitude sky. The survey includes three layers: the Wide layer will cover 1400 deg2 in five broad bands (grizy), with a 5 σ point-source depth of r ≈ 26. The Deep layer covers a total of 26 deg2 in four fields, going roughly a magnitude fainter, while the UltraDeep layer goes almost a magnitude fainter still in two pointings of HSC (a total of 3.5 deg2). Here we describe the instrument, the science goals of the survey, and the survey strategy and data processing. This paper serves as an introduction to a special issue of the Publications of the Astronomical Society of Japan, which includes a large number of technical and scientific papers describing results from the early phases of this survey

Characterization of the Amino Acid Residues of Sendai Virus C Protein That Are Critically Involved in Its Interferon Antagonism and RNA Synthesis Down-Regulation

Sendai virus (SeV) encodes two accessory proteins, V and C, in the alternative reading frames in the P gene that are accessed transcriptionally (V) or translationally (C). The C protein is expressed as a nested set of four C-coterminal proteins, C′, C, Y1, and Y2, that use different initiation codons. Using HeLa cell lines constitutively expressing the various C proteins, we previously found that the smallest (the 175-residue Y2) of the four C proteins was fully capable of counteracting the antiviral action of interferons (IFNs) and inhibiting viral RNA synthesis and that the C-terminal half of 106 residues was sufficient for both of these inhibitory functions (A. Kato et al., J. Virol. 75:3802-3810, 2001, and A. Kato et al., J. Virol. 76:7114-7124, 2002). Here, we further generated HeLa cell lines expressing the mutated C (Cm) proteins with charged amino acids substituted for alanine residues at either positions 77 and 80; 114 and 115; 139 and 142; 151, 153, and 154; 156; or 173, 175, and 176. We found that only the mutations at positions 151, 153, and 154 abolished IFN antagonism. All the Cm proteins lost the ability to bind with STAT1 under our assay conditions, regardless of their ability to inhibit IFN signaling. On the other hand, the Cm proteins that altered the tyrosine phosphorylation and dephosphorylation of STAT1 and STAT2 always retained IFN antagonism. Thus, the abnormality of phosphorylation or dephosphorylation appeared to be a cause of the IFN antagonism by SeV C. Regarding viral RNA synthesis inhibition, all mutants but the mutant with replacements at positions 114 and 115 greatly reduced the inhibitory activity, indicating that anti-RNA synthesis by the C protein is governed by amino acids scattered across its C-terminal half. Thus, amino acid sequence requirements differ greatly between IFN antagonism and RNA synthesis inhibition. In addition, we confirmed that another SeV accessory protein, V, does not antagonize IFN

The Hyper Suprime-Cam SSP survey: Overview and survey design

Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2-m Subaru telescope on the summit of Mauna Kea in Hawaii. A team of scientists from Japan, Taiwan, and Princeton University is using HSC to carry out a 300-night multi-band imaging survey of the high-latitude sky. The survey includes three layers: the Wide layer will cover 1400 deg2 in five broad bands (grizy), with a 5 σ point-source depth of r ≈ 26. The Deep layer covers a total of 26 deg2 in four fields, going roughly a magnitude fainter, while the UltraDeep layer goes almost a magnitude fainter still in two pointings of HSC (a total of 3.5 deg2). Here we describe the instrument, the science goals of the survey, and the survey strategy and data processing. This paper serves as an introduction to a special issue of the Publications of the Astronomical Society of Japan, which includes a large number of technical and scientific papers describing results from the early phases of this survey