The High-Redshift Quasar Luminosity Function from Multi-Epoch Imaging Surveys

Thesis (Ph.D.)--University of Washington, 2016-08

Sefer ha-milim : hu ḳonḳordantsia he-ḥadash ha-otsar kol ha-shemot ṿeha-peʻalim gam milot ha-baʼim be-sifre ḳodesh be-khol neṭiyotehem le-minehem ish ish ʻal digalo ṿe-shorsho, u-marʼeh kol meḳomot himatsʼam ba-Tanakh, ʻim pitron horaʼotehem bi-khelal uvi-feraṭ = Slovar t. e. novai︠a︡ konkordant︠s︡ii︠a︡ /

Mode of access: Internet.

Visits of mercy; or The journals of the Rev. Ezra Stiles Ely, D.D. : Written while he was stated preacher to the hospital and alms-house, in the city of New York. : Vol. I [-II].

Includes two sermons by Ely.

I. An exposition of the symbolic terms of the second part of Faust. II. How this part thus proves itself to be a dramatic treatment of the modern history of Germany worthy of the genius of Goethe and the life he devoted to the task. (The prologues and first act completely explained; the other acts generally).

Mode of access: Internet.

The Questions answered I.-Why should the king maintain a church when there is no congregation? II.-Why should he exact tithes to maintain the priests of such church from persons who differ from it? In a letter of instruction to the people, senators and Lords Morpeth and J.Russell on the Irish Church Bills.

Mode of access: Internet.

Some Scripture facts and prophecies illustrated in a treatise in answer to three questions : I. How did God make man? II. What purpose will he accomplish by making man as he did? III. How will God accomplish his purposes by man? /

Mode of access: Internet.

The qWR star HD 45166 - II. Fundamental stellar parameters and evidence of a latitude-dependent wind

Context. The enigmatic object HD 45166 is a qWR star in a binary system with an orbital period of 1.596 day, and presents a rich emission-line spectrum in addition to absorption lines from the companion star (B7 V). As the system inclination is very small (i = 0.77 degrees +/- 0.09 degrees), HD 45166 is an ideal laboratory for wind-structure studies. Aims. The goal of the present paper is to determine the fundamental stellar and wind parameters of the qWR star. Methods. A radiative transfer model for the wind and photosphere of the qWR star was calculated using the non-LTE code CMFGEN. The wind asymmetry was also analyzed using a recently-developed version of CMFGEN to compute the emerging spectrum in two-dimensional geometry. The temporal-variance spectrum (TVS) was calculated to study the line-profile variations. Results. Abundances and stellar and wind parameters of the qWR star were obtained. The qWR star has an effective temperature of T(eff) = 50 000 +/- 2000 K, a luminosity of log(L/L(circle dot)) = 3.75 +/- 0.08, and a corresponding photospheric radius of R(phot) = 1.00 R(circle dot). The star is helium-rich (N(H)/N(He) = 2.0), while the CNO abundances are anomalous when compared either to solar values, to planetary nebulae, or to WR stars. The mass-loss rate is. M = 2.2 x 10(-7) M(circle dot) yr(-1), and the wind terminal velocity is v(infinity) = 425 km s(-1). The comparison between the observed line profiles and models computed under different latitude-dependent wind densities strongly suggests the presence of an oblate wind density enhancement, with a density contrast of at least 8: 1 from equator to pole. If a high velocity polar wind is present (similar to 1200 km s(-1)), the minimum density contrast is reduced to 4:1. Conclusions. The wind parameters determined are unusual when compared to O-type stars or to typical WR stars. While for WR stars v(infinity)/v(esc) > 1.5, in the case of HD 45166 it is much smaller (v(infinity)/v(esc) = 0.32). In addition, the efficiency of momentum transfer is eta = 0.74, which is at least 4 times smaller than in a typical WR. We find evidence for the presence of a wind compression zone, since the equatorial wind density is significantly higher than the polar wind. The TVS supports the presence of such a latitude-dependent wind and a variable absorption/scattering gas near the equator.

The stellar content of obscured Galactic giant H II regions. VI. W51A

We present K-band spectra of newly born OB stars in the obscured Galactic giant H II region W51A and approximate to 0.8 '' angular resolution images in the J, H, and K(S)-bands. Four objects have been spectroscopically classified as O-type stars. The mean spectroscopic parallax of the four stars gives a distance of 2.0 +/- 0.3 kpc (error in the mean), significantly smaller than the radio recombination line kinematic value of 5.5 kpc or the values derived from maser proper motion observations (6-8 kpc). The number of Lyman continuum photons from the contribution of all massive stars (NLyc approximate to 1.5 x 10(50) s(-1)) is in good agreement with that inferred from radio recombination lines (NLyc = 1.3 x 10(50) s(-1)) after accounting for the smaller distance derived here. We present analysis of archival high angular resolution images (NAOS CONICA at VLT and T-ReCS at Gemini) of the compact region W51 IRS 2. The K(S)-band images resolve the infrared source IRS 2 indicating that it is a very young compact H II region. Sources IRS 2E was resolved into compact cluster (within 660 AU of projected distance) of three objects, but one of them is just bright extended emission. W51d1 and W51d2 were identified with compact clusters of three objects (maybe four in the case of W51d1) each one. Although IRS 2E is the brightest source in the K-band and at 12.6 mu m, it is not clearly associated with a radio continuum source. Our spectrum of IRS 2E shows, similar to previous work, strong emission in Br gamma and He I, as well as three forbidden emission lines of Fe III and emission lines of molecular hydrogen (H(2)) marking it as a massive young stellar object.

The B0.5 IVe CoRoT target HD 49330 II. Spectroscopic ground-based observations

Context. We present spectroscopic ground-based observations of the early Be star HD 49330 obtained simultaneously with the CoRoT-LRA1 run just before the burst observed in the CoRoT data. Aims. Ground-based spectroscopic observations of the early Be star HD 49330 obtained during the precursor phase and just before the start of an outburst allow us to disantangle stellar and circumstellar contributions and identify modes of stellar pulsations in this rapidly rotating star. Methods. Time series analysis (TSA) is performed on photospheric line profiles of He I and Si III by means of the least squares method. Results. We find two main frequencies f1 = 11.86 c d(-1) and f2 = 16.89 c d(-1) which can be associated with high order p-mode pulsations. We also detect a frequency f3 = 1.51 c d(-1) which can be associated with a low order g-mode. Moreover we show that the stellar line profile variability changed over the spectroscopic run. These results are in agreement with the results of the CoRoT data analysis, as shown in Huat et al. (2009). Conclusions. Our study of mid-and short-term spectroscopic variability allows the identification of p-and g-modes in HD 49330. It also allows us to display changes in the line profile variability before the start of an outburst. This brings new constraints for the seimic modelling of this star.

Spectroscopic identification of a dinuclear metal centre in manganese(II)-activated aminopeptidase P from Escherichia coli: implications for human prolidase

Electron paramagnetic resonance (EPR) spectra and X-ray absorption (EXAFS and XANES) data have been recorded for the manganese enzyme aminopeptidase P (AMPP, PepP protein) from Escherichia coli. The biological function of the protein, a tetramer of 50-kDa subunits, is the hydrolysis of N-terminal Xaa-Pro peptide bonds. Activity assays confirm that the enzyme is activated by treatment with Mn2+. The EPR spectrum of Mn2+-activated AMPP at liquid-He temperature is characteristic of an exchange-coupled dinuclear Mn(II) site, the Mn-Mn separation calculated from the zero-field splitting D of the quintet state being 3.5 (+/- 0.1) Angstrom. In the X-ray absorption spectrum of Mn2+-activated AMPP at the Mn K edge, the near-edge features are consistent with octahedrally coordinated Mn atoms in oxidation state +2. EXAFS data, limited to k less than or equal to 12 Angstrom(-1) by traces of Fe in the protein, are consistent with a single coordination shell occupied predominantly by O donor atoms at an average Mn-ligand distance of 2.15 Angstrom, but the possibility of a mixture of O and N donor atoms is not excluded. The Mn-Mn interaction at 3.5 Angstrom, is not detected in the EXAFS, probably due to destructive interference from light outer-shell atoms. The biological function, amino acid sequence and metal-ion dependence of E. coli AMPP are closely related to those of human prolidase, an enzyme that specifically cleaves Xaa-Pro dipeptides. Mutations that lead to human prolidase deficiency and clinical symptoms have been identified. Several known inhibitors of prolidase also inhibit AMPP. When these inhibitors are added to Mn2+-activated AMPP, the EPR spectrum and EXAFS remain unchanged. It can be inferred that the inhibitors either do not bind directly to the Mn centres, or substitute for existing Mn ligands without a significant change in donor atoms or coordination geometry. The conclusions from the spectroscopic measurements on AMPP have been verified by, and complement, a recent crystal structure analysis.

Aldosterone and angiotensin II synergistically stimulate migration in vascular smooth muscle cells through c-Src-regulated redox-sensitive RhoA pathways

Objective - Synergistic interactions between aldosterone (Aldo) and angiotensin II (Ang II) have been implicated in vascular inflammation, fibrosis, and remodeling. Molecular mechanisms underlying this are unclear. We tested the hypothesis that c-Src activation, through receptor tyrosine kinase transactivation, is critically involved in synergistic interactions between Aldo and Ang II and that it is upstream of promigratory signaling pathways in vascular smooth muscle cells (VSMCs). Methods and Results - VSMCs from WKY rats were studied. At low concentrations (10(-10) mol/L) Aldo and Ang II alone did not influence c-Src activation, whereas in combination they rapidly increased phosphorylation (P<0.01), an effect blocked by eplerenone ( Aldo receptor antagonist) and irbesartan (AT1R blocker). This synergism was attenuated by AG1478 and AG1296 ( inhibitors of EGFR and PDGFR, respectively), but not by AG1024 (IGFR inhibitor). Aldo and Ang II costimulation induced c-Src-dependent activation of NAD(P)H oxidase and c-Src-independent activation of ERK1/2 (P<0.05), without effect on ERK5, p38MAPK, or JNK. Aldo/Ang II synergistically activated RhoA/Rho kinase and VSMC migration, effects blocked by PP2, apocynin, and fasudil, inhibitors of c-Src, NADPH oxidase, and Rho kinase, respectively. Conclusions - Aldo/Ang II synergistically activate c-Src, an immediate signaling response, through EGFR and PDGFR, but not IGFR transactivation. This is associated with activation of redox-regulated RhoA/Rho kinase, which controls VSMC migration. Although Aldo and Ang II interact to stimulate ERK1/2, such effects are c-Src-independent. These findings indicate differential signaling in Aldo-Ang II crosstalk and highlight the importance of c-Src in redox-sensitive RhoA, but not ERK1/2 signaling. Blockade of Aldo/Ang II may be therapeutically useful in vascular remodeling associated with abnormal VSMC migration.

Helminth Parasites of Conventionally Maintained Laboratory Mice: II- Inbred Strains with an Adaptation of the Anal Swab Technique

Worm burdens recovered from inbred mice strains, namely C57Bl/6, C57Bl/10, CBA, BALB/c, DBA/2 and C3H/He, conventionally maintained in two institutional animal houses in the State of Rio de Janeiro, RJ, Brazil, were analyzed and compared, regarding their prevalences and mean intensities.Three parasite species were observed: the nematodes Aspiculuris tetraptera, Syphacia obvelata and the cestode Vampirolepis nana. A modification of the anal swab technique is also proposed for the first time as an auxiliary tool for the detection of oxyurid eggs in mice

Federico II de Prusia : el rey flautista

En un momento histórico en el que las tendencias musicales en Europa estaban a medio camino entre el Barroco y el Clasicismo, confluyeron en la corte de Federico el Grande una serie de músicos que trabajaron para el rey prusiano y que compusieron una gran cantidad de música para flauta, instrumento que él tocaba. La actividad musical del Berlín de esos años se convirtió así en relevante para el mundo flautístico. Profundizaremos en este trabajo en la figura del monarca, en la relación de éste con sus músicos y en las características principales de la música de la segunda mitad del siglo XVIII.

Oppimisen tukeminen tieto- ja viestintätekniikan avulla II-asteella

Tutkimuksessa tarkastellaan tieto- ja viestintätekniikan tuomaa lisäarvoa kon-taktiopetukseen sekä Moodle verkko-oppimisalustan hyödyntämistapoja opet-tajan, oppijanja työelämäyhteistyön näkökulmista. Tutkimuksessa on kaksi päätavoitetta: selvittää yleiset verkko-opetusmallit ja verkko-opetusmalleja tukevat työkalut sekä selvittää Etelä-Kymenlaakson am-mattiopistossa käytössä olevan Moodle verkko-oppimisalustan nykyistä laaja-alaisempaan käyttöönottoon liittyvät haasteet ja kehitystarpeet. Kokemusten pohjalta jälkimmäisen tavoitteen suurimmaksi yksittäiseksi haasteeksi nousee verkko-opintojakson aloitus. Opettaja joutuu verkko-opintojakson käynnistämi-sen yhteydessä tekemään liikaa monimutkaisiamäärittelyjä. Kehitystarpeissa puolestaan haetaan ratkaisuja kysymykseen; mitenverkko-oppimisalusta mahdollistaa työelämäyhteyksien parantamisen ja miten se palvelee paremmin oppijoita verkko-opintojaksojen löytämisen suhteen. Tutkimuksen tuloksena rakentui uusi tapa verkko-opintojaksojen luomiseenja kategorisointiin. Kehitetyn toimintatavan ansiosta opettajan ei tarvitse enää luoda opintojaksoa verkko-oppimisalustaan, vaan niiden aihiot luodaan ohjel-mallisesti oppilashallintojärjestelmästä saatavista tiedoista muunnosohjelman välityksellä. Opettajan tehtäväksi jää vain materiaalin tuottaminen ja kyseisellä opintojaksolla tarvitsemiensa työkalujen alustaminen. Uudella kategorisointita-valla ja mielikuvitusrikkaammilla työtilojen hyödyntämistavoilla saavutetaan seuraavat edut: järjestelmä palvelee paremmin työelämäyhteistyötä, oppijoille selkeytyy oma opintokokonaisuus paremmin ja oppijoiden sekä opettajien on helpompi löytää verkko-oppimisalustassa olevat opintojaksot.

Verifique sus conocimientos sobre radiología contrastada (II)

He aquí la segunda parte de las entregas sobre exploraciones radiológicas con contraste de la serie de Nursing sobre las pruebas complementarias. Los medios de contraste radiológicos figuran entre los elementos más comúnmente utilizados como apoyo para obtener una información diagnóstica fidedigna. En la primera entrega se expusieron los aspectos comunes de los medios de contraste utilizados en radiología y las características del contraste de bario, así como las técnicas en las que se utiliza. En esta entrega se muestran las características del contraste yodado y su uso como base de obtención de la imagen diagnóstica junto con la radiación ionizante. El contraste yodado es una sustancia que al ser atravesada por la radiación ionizante, al igual que ocurría con el bario, se traduce en una densidad metálica que se diferencia claramente del resto de densidades y por tanto de estructuras, convirtiéndolo en una de las herramientas más utilizadas en radiología. Es cierto que algunas de estas exploraciones tienden a perder relevancia frente a otras como la tomografía computarizada (TC) y la resonancia magnética (RM), pero su valor desde un punto de vista de eficacia diagnóstica todavía es relevante en los servicios de radiología. En las técnicas con contraste yodado es necesario conocer las preparaciones, la dinámica de las exploraciones y los cuidados posteriores, así como los efectos secundarios y los signos y síntomas de las reacciones adversas.