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Lonsdale, Carol J.,Lacy, M.,Kimball, A. E.,Blain, A.,Whittle, M.,Wilkes, B.,Stern, D.,Condon, J.,Kim, M.,Assef, R. J.,Tsai, C.-W.,Efstathiou, A.,Jones, S.,Eisenhardt, P.,Bridge, C.,Wu, J.,Lonsdale, Co IOP Publishing 2015 The Astrophysical journal Vol.813 No.1
<P>We present Atacama Large Millimeter/submillimeter Array (ALMA) 870 mu m (345 GHz) data for 49 high-redshift (0.47 < z < 2.85), luminous (11.7 < log(L-bol/L-circle dot) < 14.2) radio-powerful active galactic nuclei (AGNs), obtained to constrain cool dust emission from starbursts concurrent with highly obscured radiative-mode black hole (BH) accretion in massive galaxies that possess a small radio jet. The sample was selected from the Wide-field Infrared Survey Explorer with extremely steep (red) mid-infrared colors and with compact radio emission from NVSS/FIRST. Twenty-six sources are detected at 870 mu m, and we find that the sample has large mid- to far-infrared luminosity ratios, consistent with a dominant and highly obscured quasar. The rest-frame 3 GHz radio powers are 24.7 < log P-3.0 GHz/W Hz(-1)) < 27.3, and all sources are radio-intermediate or radio-loud. BH mass estimates are 7.7 < log(M-BH/M-circle dot) < 10.2. The rest-frame 1-5 mu m spectral energy distributions are very similar to the 'Hot DOGs' (hot dust-obscured galaxies), and steeper (redder) than almost any other known extragalactic sources. ISM masses estimated for the ALMA-detected sources are 9.9 < log (M-ISM/M-circle dot) < 11.75 assuming a dust temperature of 30 K. The cool dust emission is consistent with star formation rates reaching several thousand M-circle dot yr(-1), depending on the assumed dust temperature, but we cannot rule out the alternative that the AGN powers all the emission in some cases. Our best constrained source has radiative transfer solutions with approximately equal contributions from an obscured AGN and a young (10-15 Myr) compact starburst.</P>
Application of MJO simulation diagnostics to climate model simulations
Daehyun Kim,D. E. Waliser,K. R. Sperber,L Donner,J. Gottschalck,H. H. Hendon,W. Higgins,I.-S. Kang,E. D. Maloney,M. W. Moncrieff,S. Schubert,W. Stern,F. Vitart,B. Wang,W. Wang,K. M. Weickmann,M. C. Wh 한국기상학회 2008 한국기상학회 학술대회 논문집 Vol.2008 No.-
Investigating the Evolution of the Dual AGN System ESO 509-IG066
Kosec, P.,Brightman, M.,Stern, D.,Mü,ller-Sá,nchez, F.,Koss, M.,Oh, K.,Assef, R. J.,Gandhi, P.,Harrison, F. A.,Jun, H.,Masini, A.,Ricci, C.,Walton, D. J.,Treister, E.,Comerford, J.,Privon, G American Astronomical Society 2017 The Astrophysical Journal Vol.850 No.2
A Luminous Transient Event in a Sample of <i>WISE</i>-selected Variable AGNs
Assef, R. J.,Prieto, J. L.,Stern, D.,Cutri, R. M.,Eisenhardt, P. R. M.,Graham, M. J.,Jun, H. D.,Rest, A.,Flewelling, H. A.,Kaiser, N.,Kudritzki, R.-P.,Waters, C. American Astronomical Society 2018 The Astrophysical journal Vol.866 No.1
The environments of luminous radio-WISE selected infrared galaxies
Penney, J I,Blain, A W,Wylezalek, D,Hatch, N A,Lonsdale, C,Kimball, A,Assef, R J,Condon, J J,Eisenhardt, P R M,Jones, S F,Kim, M,Lacy, M,Muldrew, S I,Petty, S,Sajina, A,Silva, A,Stern, D,Diaz-Santos, Oxford University Press 2019 MONTHLY NOTICES- ROYAL ASTRONOMICAL SOCIETY Vol.483 No.1
A Radically Configurable Six-State Compound
Barnes, J. C.,Fahrenbach, A. C.,Cao, D.,Dyar, S. M.,Frasconi, M.,Giesener, M. A.,Benitez, D.,Tkatchouk, E.,Chernyashevskyy, O.,Shin, W. H.,Li, H.,Sampath, S.,Stern, C. L.,Sarjeant, A. A.,Hartlieb, K. American Association for the Advancement of Scienc 2013 Science Vol.339 No.6118
<P>Most organic radicals possess short lifetimes and quickly undergo dimerization or oxidation. Here, we report on the synthesis by radical templation of a class of air- and water-stable organic radicals, trapped within a homo[2]catenane composed of two rigid and fixed cyclobis(paraquat-p-phenylene) rings. The highly energetic octacationic homo[2]catenane, which is capable of accepting up to eight electrons, can be configured reversibly, both chemically and electrochemically, between each one of six experimentally accessible redox states (0, 2+, 4+, 6+, 7+, and 8+) from within the total of nine states evaluated by quantum mechanical methods. All six of the observable redox states have been identified by electrochemical techniques, three (4+, 6+, and 7+) have been characterized by x-ray crystallography, four (4+, 6+, 7+, and 8+) by electron paramagnetic resonance spectroscopy, one (7+) by superconducting quantum interference device magnetometry, and one (8+) by nuclear magnetic resonance spectroscopy.</P>
Electrical characterization of single GaN nanowires
Stern, E,Cheng, G,Cimpoiasu, E,Klie, R,Guthrie, S,Klemic, J,Kretzschmar, I,Steinlauf, E,Turner-Evans, D,Broomfield, E,Hyland, J,Koudelka, R,Boone, T,Young, M,Sanders, A,Munden, R,Lee, T,Routenberg, D IOP Pub 2005 Nanotechnology Vol.16 No.12
<P>In this paper a statistically significant study of 1096 individual GaN nanowire (NW) devices is presented. We have correlated the effects of changing growth parameters for hot-wall chemically-vapour-deposited (HW-CVD) NWs fabricated via the vapour–liquid–solid mechanism. We first describe an optical lithographic method for creating Ohmic contacts to NW field effect transistors with both top and bottom electrostatic gates to characterize carrier density and mobility. Multiprobe measurements show that carrier modulation occurs in the channel and is not a contact effect. We then show that NW fabrication runs with nominally identical growth parameters yield similar electrical results across sample populations of >50 devices. By systematically altering the growth parameters we were able to decrease the average carrier concentration for these as-grown GaN NWs ∼10-fold, from 2.29 × 10<SUP>20</SUP> to 2.45 × 10<SUP>19</SUP> cm<SUP>−3</SUP>, and successfully elucidate the parameters that exert the strongest influence on wire quality. Furthermore, this study shows that nitrogen vacancies, and not oxygen impurities, are the dominant intrinsic dopant in HW-CVD GaN NWs.</P>
Yoon, I.K.,Stern, M.D. Asian Australasian Association of Animal Productio 1995 Animal Bioscience Vol.8 No.6
Direct-fed microbials (DFM) have been used to enhance milk production in lactating cattle and to increase feed efficiency and body weight gain in growing ruminants. Primary microorganisms that have been used as DFM for ruminants are fungal cultures including Aspergillus oryzae and Saccharomyces cerevisiae and lactic acid bacteria such as Lactobacillus or Streptococcus. Attempts have been made to determine the basic mechanisms describing beneficial effects of DFM supplements. Various modes of action for DFM have been suggested including : stimulation of ruminal microbial growth, stabilization of ruminal pH, changes in ruminal microbial fermentation pattern, increases in digestibility of nutrients ingested, greater nutrient flow to the small intestine, greater nutrient retention and alleviation of stress, however, these responses have not been observed consistently. Variations in microbial supplements, dosage level, production level and age of the animal, diet and environmental condition or various combinations of the above may partially explain the inconsistencies in response. This review summarizes production responses that have been observed under various conditions with supplemental DFM and also corresponding modification of ruminal fermentation and other changes in the gastrointestinal tract of ruminant animals.
Assef, R. J.,Stern, D.,Noirot, G.,Jun, H. D.,Cutri, R. M.,Eisenhardt, P. R. M. American Astronomical Society 2018 The Astrophysical journal, Supplement series Vol.234 No.2
<P>We present two large catalogs of active galactic nucleus (AGN) candidates identified across 30,093 deg(2) of extragalactic sky from the Wide-field Infrared Survey Explorer's AllWISE Data Release. Both catalogs are selected purely using the Wide-field Infrared Survey Explorer (WISE) W1 and W2 bands. The R90 catalog consists of 4,543,530 AGN candidates with 90% reliability, while the C75 catalog consists of 20,907,127 AGN candidates with 75% completeness. These reliability and completeness figures were determined from a detailed analysis of UV- to near-IR spectral energy distributions of similar to 10(5) sources in the 9 deg(2) Bootes field. The AGN selection criteria are based on those of Assef et al. (2013) recalibrated to the AllWISE data release. We provide a detailed discussion of potential artifacts and excise portions of the sky close to the Galactic Center, Galactic Plane, nearby galaxies, and other expected contaminating sources. These catalogs are expected to enable a broad range of science, and we present a few illustrative cases. From the R90 sample, we identify 45 highly variable AGNs lacking radio counterparts in the FIRST survey. One of these sources, WISEA J142846.71+172353.1, is a changing-look quasar at z = 0.104, which has changed from having broad Ha to being a narrow-lined AGN. We characterize our catalogs by comparing them to large, wide-area AGN catalogs in the literature. We identify four ROSAT X-ray sources that are each matched to three WISE-selected AGNs in the R90 sample within 30.. Spectroscopy reveals that one of these systems, 2RXS J150158.6+691029, consists of a triplet of quasars at z = 1.133 +/- 0.004, suggestive of a rich group or forming galaxy cluster.</P>