Catalog of Ultra-diffuse Galaxies in the Coma Clusters from Subaru Imaging Data

We present a catalog of ultra-diffuse galaxies (UDGs) in the Coma cluster. UDGs are a subset of low surface brightness (SB) galaxies with very large effective radii defined by van Dokkum et al. We surveyed the Subaru data archive for deep Suprime-Cam/Subaru R-band images, and used data covering the 1º.7 × 2º.7 region of the Coma cluster. The data are ~1 magnitude deeper than the data of van Dokkum et al (2015a) in limiting SB. This paper explains the details of our sample selection procedure. This UDG catalog includes positions, magnitudes, effective radii, mean and central SBs, and colors (when available). Comparisons with previous galaxy catalogs in the literature are performed, and we show that the current catalog is the largest for UDGs. We also discuss that most of the UDGs are members of the Coma cluster, and the major axis of the UDGs tends to align toward the cluster center (radial alignment)

Lipoprotein(a) is a predictor for cardiovascular mortality of hemodialysis patients

Lipoprotein(a) is a predictor for cardiovascular mortality of hemodialysis patients.BackgroundAlthough hemodialysis (HD) patients have been associated with elevations in serum lipoprotein(a) [Lp(a)] levels, relatively little has been published on the link between Lp(a) and the risk for atherosclerotic cardiovascular death in HD patients.MethodsLipoprotein(a) was measured in 390 HD patients. The relationship between Lp(a) and mortality (overall and cardiovascular) was determined during 28 months of prospective follow-up.ResultsHemodialysis patients demonstrated Lp(a) concentrations that were approximately two times as high as that of healthy controls (median, 16 vs. 8 mg/dl, P < 0.001; mean, 22.9 vs. 12.1 mg/dl, P < 0.01). Lp(a) showed a significant correlation between albumin, total cholesterol, low-density lipoprotein cholesterol, and C-reactive protein. The high-Lp(a) group [Lp(a) ≥ 30 mg/dl] showed significantly higher mortality than the low-Lp(a) group [Lp(a) < 30 mg/dl] in a Kaplan–Meier survival analysis (P < 0.05). Multiple logistic regression analysis demonstrated albumin, age, and diabetic state as significant risk factors for overall death. However, if confined to atherosclerotic cardiovascular death, Lp(a) (P < 0.01), age, and diabetic state were the only independent contributors.ConclusionsLp(a) is an independent risk factor for atherosclerotic cardiovascular death in Japanese patients receiving chronic dialysis therapy

Catalog of Ultra-diffuse Galaxies in the Coma Clusters from Subaru Imaging Data

We present a catalog of ultra-diffuse galaxies (UDGs) in the Coma cluster. UDGs are a subset of low surface brightness (SB) galaxies with very large effective radii defined by van Dokkum et al. We surveyed the Subaru data archive for deep Suprime-Cam/Subaru R-band images, and used data covering the 1º.7 × 2º.7 region of the Coma cluster. The data are ~1 magnitude deeper than the data of van Dokkum et al (2015a) in limiting SB. This paper explains the details of our sample selection procedure. This UDG catalog includes positions, magnitudes, effective radii, mean and central SBs, and colors (when available). Comparisons with previous galaxy catalogs in the literature are performed, and we show that the current catalog is the largest for UDGs. We also discuss that most of the UDGs are members of the Coma cluster, and the major axis of the UDGs tends to align toward the cluster center (radial alignment)

Discovery of New Dwarf Galaxy near The Isolated Spiral Galaxy NGC 6503

We report the discovery of a new dwarf galaxy (NGC6503-d1) during the Subaru extended ultraviolet (XUV) disk survey. It is a likely companion of the spiral galaxy NGC6503. The resolved images, in B, V, R, i, and Halpha, show an irregular appearance due to bright stars with underlying, smooth and unresolved stellar emission. It is classified as the transition type (dIrr/dSph). Its structural properties are similar to those of the dwarfs in the Local Group, with a V absolute magnitude ~ -10.5, half-light radius ~400 pc, and central surface brightness ~25.2. Despite the low stellar surface brightness environment, one HII region was detected, though its Halpha luminosity is low, indicating an absence of any appreciable O-stars at the current epoch. The presence of multiple stellar populations is indicated by the color-magnitude diagram of ~300 bright resolved stars and the total colors of the dwarf, with the majority of its total stellar mass ~4x10^6 Msun in an old stellar population.Comment: Published in ApJL (ApJ, 802, L24). 7 pages, 4 figure

The results of liver function test on workers handling ethanol and isopropanol solvents

Liver function tests such as GOT, GPT, γ-GTP and ornithine carbamyl transferase (OCT) were done on workers handling alcoholic solvents. One was a group of molders working in a foundry where they sprayed ethanol solvent on the surface of a sandbox and burnt it. Another was a group of painters at an iron and steel works and they sprayed paint with isopropanol solvent on iron and steel plates. No statistical differences in the results of tests between the solvent workers and control groups were seen. High correlations were found between GOT/γ-GTP and OCT/γ-GTP. OCT of 4 workers who had drunk alcohol on the day before test showed a statisically high value compared to workers who had not drunk alcohol

Switch from conventional to high-flux membrane reduces the risk of carpal tunnel syndrome and mortality of hemodialysis patients

Switch from conventional to high-flux membrane reduces the risk of carpal tunnel syndrome and mortality of hemodialysis patients. The use of a high-flux membrane, which eliminates larger molecular weight solutes with better biocompatibility, has steadily increased since the discovery of beta-2 microglobulin (β2m) amyloidosis in 1985. The long-term effects of a dialyzer membrane on morbidity and mortality are not completely understood. To examine the membrane effect as a factor of carpal tunnel syndrome onset and mortality, multivariate Cox regression analysis with time-dependent covariate was conducted on 819 patients from March 1968 to November 1994 at a single center. Two hundred and forty-eight of the patients were either switched from the conventional to high-flux membrane or treated only with a high-flux membrane. Fifty-one patients underwent a CTS operation and 206 died. Membrane status (on high-flux or on conventional) was considered as time-dependent covariate and risk was adjusted for age, gender, type of renal disease and calendar year of dialysis initiation. The relative risk of CTS was reduced to 0.503 (P < 0.05) and mortality 0.613 (P < 0.05) by dialysis on the high-flux membrane, compared to the conventional membrane. Serial measurements of β2m indicated significantly lower β2m to persist in patients on the high-flux membrane. The high-flux membrane decreased the risk of morbidity and mortality substantially. Larger molecule elimination was shown important not only for preventing β2m amyloidosis, but for prolonging survival of dialysis patients as well

First Detection of the Molecular Cloud Population in the Extended Ultraviolet (XUV) Disk of M83

We report a CO(3-2) detection of 23 molecular clouds in the extended ultraviolet (XUV) disk of the spiral galaxy M83 with ALMA. The observed 1kpc^2 region is at about 1.24 times the optical radius (R25) of the disk, where CO(2-1) was previously not detected. The detection and non-detection, as well as the level of star formation (SF) activity in the region, can be explained consistently if the clouds have the mass distribution common among Galactic clouds, such as Orion A -- with star-forming dense clumps embedded in thick layers of bulk molecular gas, but in a low-metallicity regime where their outer layers are CO-deficient and CO-dark. The cloud and clump masses, estimated from CO(3-2), range from 8.2x10^2 to 2.3x10^4 Msun and from 2.7x10^2 to 7.5x10^3 Msun, respectively. The most massive clouds appear similar to Orion A in star formation activity as well as in mass, as expected if the cloud mass structure is universal. The overall low SF activity in the XUV disk could be due to the relative shortage of gas in the molecular phase. The clouds are distributed like chains up to 600 pc (or longer) in length, suggesting that the trigger of cloud formation is on large scales. The universal cloud mass structure also justifies the use of high-J CO transitions to trace the total gas mass of clouds, or galaxies, even in the high-z universe. This study is the first demonstration that CO(3-2) is an efficient tracer of molecular clouds even in low-metallicity environments.Comment: Accepted for AAS Journal