6 research outputs found

    Further expansion of distributional range of an introduced spider Badumna insignis in the eastern part of Tottori Prefecture (Results of the surveys in 2017).

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    2017 年の夏から秋にかけて鳥取県の東部を中心として外来種のクロガケジグモ(クモ目ウシオグモ科)の分布範囲を調査した。これまで本種が未確認の鳥取県西部でも数地点(境港市,米子市,大山町,日南町)調べたが,今回も生息は確認できなかった。鳥取県東部では,既知生息範囲から遠く離れた若桜町内や岩美町内でもそれぞれ1 地点で生息を確認した。離れているこれら2 地点を除いたほぼ連続的と考えられる鳥取市周辺の本種の今回の生息確認範囲は2014 年における生息確認範囲よりも広く,西は国道9 号線沿いの白兎海岸,南は国道53 号沿いに河原町布袋,国道29 号線沿いに八頭町下坂まで伸びていた(西へは約2.5 km,南には約6 km 拡大)。いっぽう,交通量の少ない鳥取市南西側の県道沿いには新規の拡大はみられず,本種の分布域の拡大に人の移動や物流が関係していることを示唆した。本種が生息する地点では在来種のクモの個体数が減少していた。クロガケジグモの個体数の多さが目立つのは,早くから本種の生息域となっている湖山町周辺が含まれる千代川以西・国体道路以北の鳥取市街地であった。 We surveyed distribution of an introduced spider Badumna insignis (Araneae: Desidae) in Tottori Prefecture in 2017. There were no sites where B. insignis was found in the western part of Tottori Prefecture, as reported in the former surveys. On the other hand, we found the species in Iwami-cho and Wakasa-cho, where B. insignis had not been found. Continuous range of distribution of the species in Tottori City expanded ca. 2.5 km toward west along the national route 9, and ca. 6 km toward south, along major national routes (Routes 29 and 53). On the other hand, there was no expansion of the species toward southwestern part of the city where only prefectural roads with a few traffic extend. These facts suggest that human movements and logistics help expansion of the spider. The individual number of native spiders at sites where B. insignis inhabits was much fewer than that at sites without B. insignis

    Probing renal pH using hyperpolarized [1-13C]alaninamide

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    Hyperpolarized molecular probes can be effectively used as pH markers. To date, the only two probes reported in vivo as extracellular pH sensors are 13C-bicarbonate, and [1,5-13C2]zymonic acid. Alaninamide is a derivative of alanine which is found to be sensitive to variations of pH in the physiological range. The aim of the present study was to assess the feasibility of using alaninamide as a pH probe in vivo. The alaninamide titration curve was determined by performing 13C NMR measurements at 9.4 T, 37° on a set of 500 mM Ala-NH2∙HCl samples of varying pH referenced to 13C urea. [1-13C]Alaninamide was polarized at 1 K in a 7 T polarizer, then rapidly dissolved in a buffered solution and injected IV into a Sprague Dawley rat (n=6) located in a 9.4 T animal scanner. 13C FIDs were acquired with 30° BIR4 pulses using a single loop 1H / quadrature 13C surface coil placed over the left kidney. The pH was perturbed by injecting acetazolamide IV (10 mg/kg) one hour prior to infusion. The alaninamide titration curve shows a 13C1 chemical shift change of ≈ 8.4 ppm, and a pKa of 7.9. The pH sensitivity of 13C1 results in three distinct alaninamide spectral peaks, corresponding to three different extracellular pH compartments within the kidney (pH = 7.46, pH = 7.22, pH = 6.58) that can be tentatively assigned to the cortex/blood, medulla and calyx/ureter. With acetazolamide treatment, the pH in the first compartment follows the change in pH of the blood, while the pH in the third compartment does not reflect the urine pH and shifts during the brief experiment. No change is observed in the pH value of the second compartment

    Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande

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    International audiencePreceding a core-collapse supernova, various processes produce an increasing amount of neutrinos of all flavors characterized by mounting energies from the interior of massive stars. Among them, the electron antineutrinos are potentially detectable by terrestrial neutrino experiments such as KamLAND and Super-Kamiokande via inverse beta decay interactions. Once these pre-supernova neutrinos are observed, an early warning of the upcoming core-collapse supernova can be provided. In light of this, KamLAND and Super-Kamiokande have been monitoring pre-supernova neutrinos since 2015 and 2021, respectively. Recently, we performed a joint study between KamLAND and Super-Kamiokande on pre-supernova neutrino detection. A pre-supernova alert system combining the KamLAND detector and the Super-Kamiokande detector is developed and put into operation, which can provide a supernova alert to the astrophysics community. Fully leveraging the complementary properties of these two detectors, the combined alert is expected to resolve a pre-supernova neutrino signal from a 15 M_{\odot} star within 510 pc of the Earth, at a significance level corresponding to a false alarm rate of no more than 1 per century. For a Betelgeuse-like model with optimistic parameters, it can provide early warnings up to 12 hours in advance
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