Korea Institute of Science and Technology Information

About: Korea Institute of Science and Technology Information is a facility organization based out in Daejeon, South Korea. It is known for research contribution in the topics: Gravitational wave & LIGO. The organization has 1152 authors who have published 2319 publications receiving 93849 citations. The organization is also known as: Korea Institute of Science and Technology Information & KISTI.

Search for gravitational-wave signals associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo

Abstract: We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38 10-6 (modeled) and 3.1 10-4 (unmodeled). We do not find any significant evidence for gravitational-wave signals associated with the other gamma-ray bursts analyzed, and therefore we report lower bounds on the distance to each of these, assuming various source types and signal morphologies. Using our final modeled search results, short gamma-ray burst observations, and assuming binary neutron star progenitors, we place bounds on the rate of short gamma-ray bursts as a function of redshift for z ≤ 1. We estimate 0.07-1.80 joint detections with Fermi-GBM per year for the 2019-20 LIGO-Virgo observing run and 0.15-3.90 per year when current gravitational-wave detectors are operating at their design sensitivities.

First Observation of the Doubly Cabibbo-Suppressed Decay of a Charmed Baryon: Λc+→pK+π-

Abstract: We report the first observation of the decay Lambda(+)(c) -> pK(+)pi(-) using a 980 fb(-1) data sample collected by the Belle detector at the KEKB asymmetric-energy e(+)e(-) collider. This is the first observation of a doubly Cabibbo-suppressed decay of a charmed baryon. We measure the branching ratio of this decay with respect to its Cabibbo-favored counterpart to be B(Lambda(+)(c) -> pK(+)pi(-))/B(Lambda(+)(c) -> pK(-)pi(+)) = (2.35 +/- 0.27 +/- 0.21) x 10(-3), where the uncertainties are statistical and systematic, respectively.

Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs

Abstract: We report results from searches for anisotropic stochastic gravitational-wave backgrounds using data from the first three observing runs of the Advanced LIGO and Advanced Virgo detectors. For the first time, we include Virgo data in our analysis and run our search with a new efficient pipeline called pystoch on data folded over one sidereal day. We use gravitational-wave radiometry (broadband and narrow band) to produce sky maps of stochastic gravitational-wave backgrounds and to search for gravitational waves from point sources. A spherical harmonic decomposition method is employed to look for gravitational-wave emission from spatially-extended sources. Neither technique found evidence of gravitational-wave signals. Hence we derive 95% confidence-level upper limit sky maps on the gravitational-wave energy flux from broadband point sources, ranging from F α , Θ < ( 0.013 – 7.6 ) × 10 − 8 erg cm − 2 s − 1 Hz − 1 , and on the (normalized) gravitational-wave energy density spectrum from extended sources, ranging from Ω α , Θ < ( 0.57 – 9.3 ) × 10 − 9 sr − 1 , depending on direction ( Θ ) and spectral index ( α ). These limits improve upon previous limits by factors of 2.9–3.5. We also set 95% confidence level upper limits on the frequency-dependent strain amplitudes of quasimonochromatic gravitational waves coming from three interesting targets, Scorpius X-1, SN 1987A and the Galactic Center, with best upper limits range from h 0 < ( 1.7 – 2.1 ) × 10 − 25 , a factor of ≥ 2.0 improvement compared to previous stochastic radiometer searches.

Morphological characteristics of the infraorbital foramen and infraorbital canal using three-dimensional models

Abstract: Infraorbital nerve blocking through the infraorbital foramen and infraorbital canal is used to anesthetize the lower eyelid, upper lip, lateral nose, upper teeth and related gingivae. For this, it is important to know the position of the infraorbital foramen, structures around the foramen, and the direction of the injecting needle related to the angle of the infraorbital canal. Many reports have described the anatomical location of the infraorbital foramen; however, not many have described the angle of the infraorbital canal and those structures around the infraorbital foramen that help the physician visualize the correct direction of the needle. Dried skulls of 42 Korean subjects (27 male and 15 female) were studied to analyze structures around the infraorbital foramen. The morphology of the infraorbital canal was also investigated using three-dimensional models. Structures around the infraorbital foramen were classified into four types according to the existence of a distinct tuberosity above the infraorbital foramen, and the degree of prominence of the canine fossa. Types I and II have a tuberosity above the infraorbital foramen, whereas types III and IV have no distinct tuberosity. Types I and III have a prominent canine fossa, whereas this is less prominent in types II and IV. We analyzed the skulls based on the angle of the infraorbital canal to the median plane. We compared the left and right sides and analyzed differences between the sexes, the three canal shapes, and the four structure types around the infraorbital foramen. Type IV was the most common in this series (38%). The infraorbital canal could be classified into three morphologies: ‘tube-like’ (69%), ‘funnel’ (25%) and ‘pinched’ (6%). The mean angle of the infraorbital canal relative to the median plane was 12°, and the angle relative to the Frankfurt plane was 44°. The mean angle between the infraorbital canal and the Frankfurt plane was 4° larger in males than in females in this series of Korean subjects. The operator of the infraorbital nerve block should pay attention towards directing the needle upward at an angle of about 44° for avoiding nerve damage and consider the different angles of the canal according to the individual’s sex.