A Case Of Nivolumab-Induced Immune-Related Adverse Event In The Upper Gastrointestinal Tract In Recurrence/Metastatic Head And Neck Cancer.

A 61-year-old male patient underwent partial glossectomy and right neck dissection for tongue cancer cT2N1MO. Because of the locoregional recurrence, the patient received neoadjuvant chemotherapy followed by subtotal glossectomy, neck dissection, and reconstruction. However, new locoregional lesions and distant metastasis were detected during postoperative chemotherapy. Seven courses of nivolumab were administered, but the tumor grew. Hence, the chemotherapy regimen was switched to paclitaxel and cetuximab. After eight courses of this regimen, leakage of liquid enteral nutrients around the gastrostoma began, and the patient was hospitalized urgently due to severe abdominal distension and nausea. Upper gastrointestinal endoscopy revealed edematous esophageal and gastric mucosa covered with white coating spots. Histopathological examination of the duodenal mucosa specimen showed CD8-+ natural killer (NK) T-cells infiltrating the lamina propria mucosae, which corresponded with an immune-related adverse event (irAE). Pulse steroid therapy significantly improved the findings of upper gastrointestinal endoscopy and symptoms

Detection of ultra-high energy cosmic ray air showers by Cosmic Ray Air Fluorescence Fresnel lens Telescope for next generation

In the future, ultra-high energy cosmic ray (UHECR) observatory will be expanded due to the small flux. Then, cost reduction is useful strategy to realize a huge scale observatory. For this purpose, we are developing a simple structure cosmic ray detector named as Cosmic Ray Air Fluorescence Fresnel-lens Telescope (CRAFFT). We deployed CRAFFT detectors at the Telescope Array site and performed a test observation. We have successfully observed UHECR air showers. We will report the status and the result of the test observation

Detection of ultra-high energy cosmic ray air showers by Cosmic Ray Air Fluorescence Fresnel lens Telescope for next generation

In the future, ultra-high energy cosmic ray (UHECR) observatory will be expanded due to the small flux. Then, cost reduction is useful strategy to realize a huge scale observatory. For this purpose, we are developing a simple structure cosmic ray detector named as Cosmic Ray Air Fluorescence Fresnel-lens Telescope (CRAFFT). We deployed CRAFFT detectors at the Telescope Array site and performed a test observation. We have successfully observed UHECR air showers. We will report the status and the result of the test observation

AMS法による有孔虫<14>^C年代と海洋深層水循環

P4 core, which is composed mainly of olive grayish mud with well-developed biogenic structures, was raised from the lower continental slope basin off Shikoku at lat. 32°09'N, log. 133°54'E from a depth of 2700m. Each of samples for ^C dating analysis was taken from 19 horizons throughout the core. And we have done the measurement of ^C age differences between benthic and planktonic foraminifera to determine deep ocean ventilation times, using accelerator mass spectrometry. The results suggest that there are clearly two main mode patterns of paleo-circulation here at about 13,000 y.B.P., which may be called glacial and post glacial type. The formar has a slow mode which are difference ages about 1,000 yr, the latter has complicated puls patterns from 2,000 yr to 1,000 years