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Showing 1 to 20 of 21 for “"SEDS"”.

  1. Sexual-Enhancement Drug Use in College-Age Men

    … to explore the use of sexual-enhancement drugs (SEDs) in college men and to compare the men who had used SEDs to those who had not used them. Eighty-two male college students completed a questionnaire that included open-ended questions about their use of SEDs and items assessing their sexual …

    ku Repository record for Sexual-Enhancement Drug Use in College-Age Men (opens in a new tab)

  2. Search for rapidly star-forming galaxies at high redshift.

    … CCD photometry to locate objects with peculiar SEDs. Using the IR data we should be able to locate rapidly star forming galaxies to z = 25. With a 3σ detection limit of 18.5 at K we have found no objects with z > 5 but we have found several blue objects at z < 4 in 16min² of sky. This suggests …

    arizona-thes Repository record for Search for rapidly star-forming galaxies at high redshift. (opens in a new tab)

  3. The broad spectral energy distributions of accreting white dwarfs

    … on the broad spectral energy distributions (SEDs) of these objects. I perform such a study here, and present the largest collection of broad CV SEDs yet constructed. I define a sample of well-studied, nearby cataclysmic variables of several different CV classes, and gather existing …

    cape-town Repository record for The broad spectral energy distributions of accreting white dwarfs (opens in a new tab)

  4. Star formation in unobscured quasars

    … span a redshift range of 0 < z < 4, and their SEDs give a mean SFR of ~1000M☉/year. When comparing these SFRs to the intrinsic properties of the quasars, we find no clear connections between the quasars and the ongoing star formation events in their hosts. We then look for evidence of AGN …

    vt Repository record for Star formation in unobscured quasars (opens in a new tab)

  5. The FORS Deep Field Spectroscopic Survey

    … were determined using a library of empirical SEDs derived from FDF mean spectra with very high S/N. The characteristics of the observed galaxy spectra are presented and the distribution of redshifts and spectral types are discussed. A first analysis of the excellent data set was carried out …

    heid-diss Repository record for The FORS Deep Field Spectroscopic Survey (opens in a new tab)

  6. 'Training' the Body Politic: Essays on the School Reform Orthodoxy

    … connections between socioeconomic disadvantages (SEDs) and student achievement on standardized tests.</p>

    chapman Repository record for 'Training' the Body Politic: Essays on the School Reform Orthodoxy (opens in a new tab)

  7. Plano Estadual de Assistência Social: o papel das diretorias regionais na formulação, avaliação e apoio à implementação

    … Secretaria Estadual de Desenvolvimento Social (SEDS), o período pós-elaboração do PEAS tem se mostrado um momento desafiador no que se refere à implementação das diretrizes e projetos em âmbito regional. Consideradas como instâncias estratégicas no desdobramento das políticas estaduais de …

    brazil-fgv Repository record for Plano Estadual de Assistência Social: o papel das diretorias regionais na formulação, avaliação e apoio à implementação (opens in a new tab)

  8. Models of Dust and Gas Tori in Active Galactic Nuclei

    … of Seyfert galaxies. However, the model SEDs show too pronounced silicate emission features in the face-on case. This can be overcome with the help of three-dimensional clumpy tori, calculated in a second step. Special emphasis is put on the differences of clumpy and continuous dust …

    heid-diss Repository record for Models of Dust and Gas Tori in Active Galactic Nuclei (opens in a new tab)

  9. The influence of planetary and stellar companions on debris discs

    … sample of 341 multiple star systems, using their SEDs to identify and characterise their debris discs. I find that the stellar separation distributions of disc-bearing and disc-free systems differ with 99.4% confidence. No discs are detected for separations between 25 and 135 au, likely because …

    cambridge Repository record for The influence of planetary and stellar companions on debris discs (opens in a new tab)

  10. Spectral Energy Distribution Modelling of X-ray Selected AGNs and Their Host Galaxies

    … We also find that the use of lower resolution SEDs can lead to repercussions on property inferences such as host galaxy stellar mass, which may provide incorrect assumptions on the relation between AGN and their host galaxies.

    cambridge Repository record for Spectral Energy Distribution Modelling of X-ray Selected AGNs and Their Host Galaxies (opens in a new tab)

  11. The Andromeda Optical and Infrared Disk Survey

    … of resolved stellar populations and panchromatic SEDs. We present the Andromeda Optical and Infrared Disk Survey (ANDROIDS), which adds new near-UV to near-IR (ugriJKs) imaging using the MegaCam and WIRCam cameras at the Canada-France-Hawaii telescope to the available M31 panchromatic dataset. To …

    queens Repository record for The Andromeda Optical and Infrared Disk Survey (opens in a new tab)

  12. Far-UV to Mid-IR Spectral Energy Distributions of Nearby Merging Galaxies

    … galaxy evolution. Spectral energy distributions (SEDs) allow Astrophysicists to disentangle AGN activity from SF. I hypothesize that applying SED analysis to a sample of merging galaxies will show an enhancement in AGN activity over control galaxies. I perform SED analysis from the far-ultraviolet …

    umkc Repository record for Far-UV to Mid-IR Spectral Energy Distributions of Nearby Merging Galaxies (opens in a new tab)

  13. The characterization of volatiles associated with young stellar objects

    … Class II Spectral Energy Distributions (SEDs) have a larger abundance of CO₂ ice with respect to H₂O ice. In addition to intracloud differences, we compared our results with several other star forming regions, high mass YSOs, and background objects. The average abundance of CO₂ with …

    must-thes Repository record for The characterization of volatiles associated with young stellar objects (opens in a new tab)

  14. A high energy perspective of the co-evolution of black holes and their host galaxies

    … luminosity and spectral energy distributions (SEDs) of elusive AGN is of paramount importance. The recent COSMOS survey provides the necessary multiwavelength database to characterize the SEDs of a statistically robust sample of obscured sources. The combination of high X/O and red-colors …

    bologna Repository record for A high energy perspective of the co-evolution of black holes and their host galaxies (opens in a new tab)

  15. Etude de la régulation de l'expression de l'opéron ftsW-psr-pbp5 chez Enterococcus hirae

    … codant pour des protéines de la même famille (SEDS pour FtsW, LCP pour Psr, et les autres PBPs pour PBP5). Nous avons produit et purifié ces différentes protéines avec pour visée principale la possibilité d’obtenir des anticorps spécifiques pouvant servir à localiser les protéines au sein de la …

    liege Repository record for Etude de la régulation de l'expression de l'opéron ftsW-psr-pbp5 chez Enterococcus hirae (opens in a new tab)

  16. Connecting simulations and observations in galaxy formation studies

    … the galaxies' Spectral Energy Distributions (SEDs) using different approaches, including radiative transfer techniques. Comparing the direct results of the simulations with the quantities obtained applying observational techniques to these synthetic SEDs, we are able to make an analysis of the …

    potsdam-diss Repository record for Connecting simulations and observations in galaxy formation studies (opens in a new tab)

  17. Hierarchical Bayesian Spectro-temporal Models of Type Ia Supernovae in the Optical and Near-Infrared: Understanding the Properties of Dust in Supernova Host Galaxies

    … for modelling the spectral energy distributions (SEDs) of SNe Ia in the optical and near-infrared (NIR). I apply this framework to detailed studies of the dust in SN Ia host galaxies – particularly the distribution of the dust law R_V. This model is able to leverage the optical and NIR in a …

    cambridge Repository record for Hierarchical Bayesian Spectro-temporal Models of Type Ia Supernovae in the Optical and Near-Infrared: Understanding the Properties of Dust in Supernova Host Galaxies (opens in a new tab)

  18. Star-forming Galaxies and Quenched Systems throughout Cosmic Time

    … the best sampling of high-redshift galaxy SEDs out to z > 3, I show that measurements of the main sequence to low masses and high redshifts were still strongly dependent on the priors employed in SED fitting (as well as other fitting assumptions). In the first field targeted by JADES, the …

    cambridge Repository record for Star-forming Galaxies and Quenched Systems throughout Cosmic Time (opens in a new tab)

  19. Constraining the Initial Conditions and Final Outcomes of Accretion Processes around Young Stars and Supermassive Black Holes

    … objects at 1000 K that exhibit distinct L-band SEDs. The oldest object in my sample of young companions, 50 My old CD-35 2722 B, appears redder than field dwarfs with similar spectral type based on 1-2.5 μm spectra. This could indicate reduced cloud opacity compared to field dwarfs at the same …

    arizona-thes Repository record for Constraining the Initial Conditions and Final Outcomes of Accretion Processes around Young Stars and Supermassive Black Holes (opens in a new tab)

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