Barley stripe mosaic Hordeivirus (BSMV) is a positive-strand RNA virus requiring three single-stranded RNAs (alpha, beta, and gamma) for infectivity. A terminal-sequence-dependent cloning strategy was used to clone the entire genome of the CV17 strain. Full-length gamma cDNA clones were obtained when oligonucleotides specific for the 5'-terminal sequence of RNA alpha were used in the cloning procedure, but not when RNA gamma-specific oligonucleotides were used. Sequence analysis of six putative gamma cDNA clones revealed that nucleotides 1-70 possess 89% homology with the first 70 nucleotides of RNA alpha. This leader region is separated from the gamma-specific coding region by an eight-base intervening sequence common to both CV17 RNAs alpha and gamma. Northern and Southern hybridization with oligonucleotide probes specific for either alpha or gamma leader sequences indicated that CV17 gamma cDNA clones are representative of native CV17 gamma RNAs. Furthermore, bioassays indicated that in vitro transcripts derived from these gamma cDNA clones were infectious when coinoculated with in vitro transcripts of full-length alpha and beta cDNA clones. Thus, the evidence suggests that RNA gamma of BSMV strain CV17 is a recombinant molecule which may have arisen as a result of natural recombination between RNAs alpha and gamma.

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams.

The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission from GW151226, adopting the GW event's 3D localization, to less than 2×1051-2×1054 erg.