Observation of the 4f146s2 1S0−4f135d6s2(J=2)4f^{14}6s^{2}~^1S_0- 4f^{13}5d6s^{2}(J=2) clock transition at 431 nm in 171^{171}Yb

We report on the observation of the $4f^{14}6s^{2}~^1S_0- 4f^{13}5d6s^{2}(J=2)$ transition at 431 nm in $^{171}$Yb by depleting atoms in a magneto-optical trap formed by the $6s^{2}~^1S_0-6s6p~^3P_1$ intercombination transition. The absolute frequency of the transition to the $F=3/2$ state is determined to be $695~171~054~858.1(8.2)$~kHz against physical realization of Coordinated Universal Time maintained by the National Metrology Institute of Japan with a frequency comb. The $g$ factor of the transition to the $F=3/2$ state and the A hyperfine constant are measured to be $g_J=1.54(13)$ and 1123.273(13)~MHz, respectively. More precise spectroscopy of this transition can lead to searches for time variation of the fine structure constant and searches for new physics with isotope shift measurements.Comment: 5 pages, 4 figure

A CASE OF DIABETES INSIPIDUS ACCOMPANYING THIRST DISORDER ASSOCIATED WITH HYPEROSMOLAR DIABETIC COMA

The case of a 14-year-old female who suffered from hyperosmolar diabetic coma (HODC) after resection of craniopharyngioma and during treatment for hypopituitarism and diabetes insipidus is presented. In Aug. 1989, craniopharyngioma was diagnosed and she underwent resection surgery and radiotherapy. Since then, she had been on supplemental therapy with hydrocortisone and thyroxin and desmopressin (DDAVP). On Jan. 17, 1992, she fell into HODC upon ingesting a large amount of soft drink to supplement water due to persistent polyuria. She improved quickly when supplementary fluids and insulin were administered. She had demonstrated no abnormality in glucose tolerance prior to this manifestation. Insulin therapy was deemed unnecessary after her recovery from HODC. Because of a disorder in the central nervous thirst mechaninm, she lacked the sense of thirst and concomitantly the thirst-mediated water intake in spite of elevated plasma osmolarity due to dehydration and hyperglycemia. This seemed to be the cause of her accelerating dehydration. The resulting insulin resistance then brought about her HODC. Thus, it is difficult to consider such a case of HODC as symptomatic of diabetes when no abnormality in glucose tolerance either before manifestation or after restoration can be found. It should rather be considered as a case of “dehydration hyperglycemia" and be treated as such

Preliminary Report of Body Mass Index Among People with and Without Schizophrenia in Japan

This cross-sectional study was designed to estimate body mass index (BMI, kg/m^2) of individuals with and without schizophrenia and to examine factors contributing to excessive weight. There were a total of 208 patients (138 men, 70 women) with schizophrenia under hospitalization in a psychiatric hospital and 1,054 controls (797 men, 257 women) without schizophrenia, who underwent overnight medical screening at another university-affiliated hospital in the same area of Japan in 1998. The mean BMI among the 208 patients with schizophrenia was 24.44±4.0 compared with a mean BMI of 23.64±2.7 in healthy controls. There were no significant differences between male patients and male controls ; however, mean BMI was higher in female patients than in female controls, especially among patients under 60 years of age. As weight gain (with increase in BMI) after initiation of medication for schizophrenia is associated more with female gender and younger age, education and support to prevent obesity is particularly important for younger female patients

JASMINE: Near-infrared astrometry and time-series photometry science

The Japan Astrometry Satellite Mission for INfrared Exploration (JASMINE) is a planned M-class science space mission by the Institute of Space and Astronautical Science, the Japan Aerospace Exploration Agency. JASMINE has two main science goals. One is Galactic archaeology with a Galactic Center survey, which aims to reveal the Milky Way’s central core structure and formation history from Gaia-level (∼25 ${\mu}$as) astrometry in the near-infrared (NIR) Hw band (1.0–1.6 ${\mu}$m). The other is an exoplanet survey, which aims to discover transiting Earth-like exoplanets in the habitable zone from NIR time-series photometry of M dwarfs when the Galactic Center is not accessible. We introduce the mission, review many science objectives, and present the instrument concept. JASMINE will be the first dedicated NIR astrometry space mission and provide precise astrometric information on the stars in the Galactic Center, taking advantage of the significantly lower extinction in the NIR. The precise astrometry is obtained by taking many short-exposure images. Hence, the JASMINE Galactic Center survey data will be valuable for studies of exoplanet transits, asteroseismology, variable stars, and microlensing studies, including discovery of (intermediate-mass) black holes. We highlight a swath of such potential science, and also describe synergies with other missions