Search for gravitational-wave transients associated with magnetar bursts in advanced LIGO and advanced Virgo data from the third observing run

Gravitational waves are expected to be produced from neutron star oscillations associated with magnetar giant f lares and short bursts. We present the results of a search for short-duration (milliseconds to seconds) and longduration (∼100 s) transient gravitational waves from 13 magnetar short bursts observed during Advanced LIGO, Advanced Virgo, and KAGRA’s third observation run. These 13 bursts come from two magnetars, SGR1935 +2154 and SwiftJ1818.0−1607. We also include three other electromagnetic burst events detected by FermiGBM which were identified as likely coming from one or more magnetars, but they have no association with a known magnetar. No magnetar giant flares were detected during the analysis period. We find no evidence of gravitational waves associated with any of these 16 bursts. We place upper limits on the rms of the integrated incident gravitational-wave strain that reach 3.6 × 10−²³ Hz at 100 Hz for the short-duration search and 1.1 ×10−²² Hz at 450 Hz for the long-duration search. For a ringdown signal at 1590 Hz targeted by the short-duration search the limit is set to 2.3 × 10−²² Hz. Using the estimated distance to each magnetar, we derive upper limits upper limits on the emitted gravitational-wave energy of 1.5 × 1044 erg (1.0 × 1044 erg) for SGR 1935+2154 and 9.4 × 10^43 erg (1.3 × 1044 erg) for Swift J1818.0−1607, for the short-duration (long-duration) search. Assuming isotropic emission of electromagnetic radiation of the burst fluences, we constrain the ratio of gravitational-wave energy to electromagnetic energy for bursts from SGR 1935+2154 with the available fluence information. The lowest of these ratios is 4.5 × 103

Open data from the third observing run of LIGO, Virgo, KAGRA, and GEO

The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages

A joint Fermi-GBM and Swift-BAT analysis of gravitational-wave candidates from the third gravitational-wave observing run

We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift-BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers

Constraints on the cosmic expansion history from GWTC–3

We use 47 gravitational wave sources from the Third LIGO–Virgo–Kamioka Gravitational Wave Detector Gravitational Wave Transient Catalog (GWTC–3) to estimate the Hubble parameter H(z), including its current value, the Hubble constant H0. Each gravitational wave (GW) signal provides the luminosity distance to the source, and we estimate the corresponding redshift using two methods: the redshifted masses and a galaxy catalog. Using the binary black hole (BBH) redshifted masses, we simultaneously infer the source mass distribution and H(z). The source mass distribution displays a peak around 34 M⊙, followed by a drop-off. Assuming this mass scale does not evolve with the redshift results in a H(z) measurement, yielding ${H}_{0}={68}_{-8}^{+12}\,\mathrm{km}\ \,\ {{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$ (68% credible interval) when combined with the H0 measurement from GW170817 and its electromagnetic counterpart. This represents an improvement of 17% with respect to the H0 estimate from GWTC–1. The second method associates each GW event with its probable host galaxy in the catalog GLADE+, statistically marginalizing over the redshifts of each event's potential hosts. Assuming a fixed BBH population, we estimate a value of ${H}_{0}={68}_{-6}^{+8}\,\mathrm{km}\ \,\ {{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$ with the galaxy catalog method, an improvement of 42% with respect to our GWTC–1 result and 20% with respect to recent H0 studies using GWTC–2 events. However, we show that this result is strongly impacted by assumptions about the BBH source mass distribution; the only event which is not strongly impacted by such assumptions (and is thus informative about H0) is the well-localized event GW190814

Crioconservação de sementes de mamona das variedades nordestina e pernambucana Cryoconservation of nordestina and pernambucana varieties of castor bean seeds

É grande a importância da mamoneira (Ricinus communis L.) para a economia do semi-árido nordestino, que é responsável por 80% da produção nacional, no entanto durante 1970 e 2000, a produção líquida dessa oleaginosa foi reduzida na mesma percentagem. Registrou-se também a existência de aproximadamente 90 tipos diferentes de sementes empregadas no cultivo desta Euforbiaceae. Devido a este problema, o trabalho desenvolvido no Laboratório de Processamento e Armazenamento de Produtos Agrícolas do DEAg/UFPB, objetivou desenvolver técnicas de crioconservação para duas variedades de Ricinus communis, com vistas a uma armazenagem segura e por tempo indefinido. O delineamento experimental utilizado foi o inteiramente casualizado, com os dados obtidos nos 7º e 14º dias depois da semeadura, dispostos em um arranjo fatorial 2 x 3 x 2 x 2 (duas variedades, três períodos de crioconservação, duas temperaturas de crioconservação e dois tipos de acondicionamento) com oito repetições de vinte e cinco sementes cada uma. Os dados obtidos foram submetidos à análise de variância e as médias dos fatores qualitativos comparadas pelo teste de Tukey, a 5% de probabilidade. Com os resultados obtidos concluiu-se que: o nível máximo de umidade para a crioconservação das sementes das duas variedades de Ricinus communis (nordestina e pernambucana) encontra-se entre 4 e 10% base úmida; os melhores resultados de qualidade fisiológica foram obtidos aos 30 dias da crioconservação, podendo essas sementes serem crioconservadas tanto no vapor (-176 ºC) como na imersão (-196 ºC) em nitrogênio líquido; o canister de alumínio utilizado para acondicionar as sementes mostrou-se superior ao de PVC.<br>The castor bean (Ricinus communis L.) has great importance for the economy of the semi-arid region of the northeast of Brazil, responsible for 80% of the national production, but during 1970 and 2000, the net production of this oil crop was reduced. Existence of some 90 different types of seeds used in the cultivation of this Euforbiaceae was also verified. Due to this problem, the Processing and Storage of Agricultural Products Laboratory of DEAg/UFCG, has tried to develop cryoconservation technique for two varieties of Ricinus communis, in order to obtain a secured storage for an indefinite time. The experimental delineation was a completely randomized, with the data obtained on the 7th and 14th day after sowing, in a factorial scheme 2 x 3 x 2 x 2 (2 varieties x 3 cryoconservation periods x 2 cryoconservation temperatures x 2 types of conditioning) with eight repetitions of twenty-five seeds each. The data obtained were submitted to an variance analysis and the means were compared by the Tukey's, test at 5% of probability. From the results obtained it can be concluded that: the maximum level of humidity for the cryoconservation of the seeds of the two varieties of Ricinus communis (nordestina and pernambucana) is between 4 and 10% on wet basis; the best results of physiological quality were obtained after 30 days of cryoconservation and may either be cryoconserved in the vapor (-176 ºC) or by immersion (-196 ºC) in liquid nitrogen; for storage of seeds, canister of aluminum proved to be better than that of PVC

Treatment of incomplete abortion and miscarriage with misoprostol

A literature review was conducted to determine whether misoprostol is an effective treatment for incomplete abortion and, if so, to recommend an appropriate regimen. All English language articles published before October 2007 using misoprostol in at least one of the study arms were reviewed to determine the efficacy of misoprostol when used to treat incomplete abortion in the first trimester. All available unpublished data previously presented at international scientific meetings were also reviewed. Sufficient evidence was found in support of misoprostol as a safe and effective means of non-surgical uterine evacuation. A single dose of misoprostol 600 μg oral is recommended for treatment of incomplete abortion in women presenting with a uterine size equivalent to 12 weeks gestation. © 2007 International Federation of Gynecology and Obstetrics.link_to_subscribed_fulltex