High proportion of cactus species threatened with extinction

This is the author accepted manuscript. The final version is available from Nature Publishing Group via the DOI in this record.Consejo Nacional de Ciencia y Tecnologí

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

A 54-Kilodalton Protein Encoded by pBtoxis Is Required for Parasporal Body Structural Integrity in Bacillus thuringiensis subsp. israelensis

Strains of Bacillus thuringiensis such as B. thuringiensis subsp. israelensis (ONR-60A) and B. thuringiensis subsp. morrisoni (PG-14) pathogenic for mosquito larvae produce a complex parasporal body consisting of several protein endotoxins synthesized during sporulation that form an aggregate of crystalline inclusions bound together by a multilamellar fibrous matrix. Most studies of these strains focus on the molecular biology of the endotoxins, and although it is known that parasporal body structural integrity is important to achieving high toxicity, virtually nothing is known about the matrix that binds the toxin inclusions together. In the present study, we undertook a proteomic analysis of this matrix to identify proteins that potentially mediate assembly and stability of the parasporal body. In addition to fragments of their known major toxins, namely, Cry4Aa, Cry4Ba, Cry11Aa, and Cyt1Aa, we identified peptides with 100% identity to regions of Bt152, a protein coded for by pBtoxis of B. thuringiensis subsp. israelensis, the plasmid that encodes all endotoxins of this subspecies. As it is known that the Bt152 gene is expressed in B. thuringiensis subsp. israelensis, we disrupted its function and showed that inactivation destabilized the parasporal body matrix and, concomitantly, inclusion aggregation. Using fluorescence microscopy, we further demonstrate that Bt152 localizes to the parasporal body in both strains, is absent in other structural or soluble components of the cell, including the endospore and cytoplasm, and in ligand blots binds to purified multilamellar fibrous matrix. Together, the data show that Bt152 is essential for stability of the parasporal body of these strains